SPACE SCIENCE
study of everything in outer space. This has sometimes been called astronomy, but recently astronomy has come to be regarded as a division of broader space science, which has grown to include other related fields, such as studying issues related to space travel and space exploration (including space medicine), space archaeology and science performed in outer space (see space research).
Wednesday, February 10, 2016
Monday, January 25, 2016
Thursday, November 5, 2015
Astronomy
In astronomy, a lunar distance (LD) is a measurement of the distance from the Earth to the Moon. The average distance from the center of the Earth to the center of the Moon is 384,400 km (238,900 mi).One astronomical unit is about 389 LD. The actual distance varies over the course of the orbit of the moon, from 363,104 km (225,622 mi) at the perigee and 405,696 km (252,088 mi) at apogee, resulting in a differential range of 42,592 km (26,465 mi).
Millimeter-precision measurements of the lunar distance are made by measuring the time taken for light to travel between LIDAR stations on the Earth and retroreflectors placed on the Moon. Lunar laser ranging measurement data is available from the Paris Observatory Lunar Analysis Center,[2] and the active stations.
The Moon is spiraling away from the Earth at an average rate of 3.8 cm (1.5 in) per year, as detected by the Lunar Laser Ranging Experiment.The recession rate is considered anomalously high.By coincidence, the diameter of corner cubes in retroreflectors on the Moon is also 3.8 cm (1.5 in).
The tidal dissipation rate has varied during the Earth's geological history.
The first person to measure the distance to the Moon was the 2nd-century-BC astronomer and geographer Hipparchus, who exploited the lunar parallax using simple trigonometry, measuring the distance as 400,000 kilometers. He was approximately 26,000 km (16,000 mi) off the actual distance, an error of about 6.8%.
All nine manned missions to the Moon took place as part of the Apollo program over a period of just under four years, from 21 December 1968 to 19 December 1972. Of the 24 people who have flown to the Moon, 17 are still living as of November 2015.
John Young, Eugene Cernan and Jim Lovell are the only three people to have flown to the Moon twice. Young and Cernan each set foot on it during their respective second lunar missions, while Lovell is the only person to have flown to the Moon twice without landing.
During Cernan's first lunar mission on Apollo 10, he tied the present record set by Bill Anders on Apollo 8 as the youngest person to fly to the Moon. Each was 35 years and 65 days old on his launch date and 35 years and 68 days old when he entered lunar orbit. (The oldest person to fly to the Moon was Alan Shepard, who walked on its surface during the Apollo 14 mission. Shepard was 47 years and 74 days old on his launch date and 47 years and 78 days old when he entered lunar orbit.)
Because of Apollo 13's free-return trajectory, Lovell, Jack Swigert and Fred Haise flew higher above the Moon's 180° meridian (opposite Earth) than anyone else has flown (254 km/158 mi). Coincidentally, due to the Moon's distance from Earth at the time, they simultaneously set the present record for humans' greatest distance from Earth, reaching an altitude of 400,171 km (248,655 mi) above sea level at 0:21 UTC on 15 April 1970.
Millimeter-precision measurements of the lunar distance are made by measuring the time taken for light to travel between LIDAR stations on the Earth and retroreflectors placed on the Moon. Lunar laser ranging measurement data is available from the Paris Observatory Lunar Analysis Center,[2] and the active stations.
The Moon is spiraling away from the Earth at an average rate of 3.8 cm (1.5 in) per year, as detected by the Lunar Laser Ranging Experiment.The recession rate is considered anomalously high.By coincidence, the diameter of corner cubes in retroreflectors on the Moon is also 3.8 cm (1.5 in).
The tidal dissipation rate has varied during the Earth's geological history.
The first person to measure the distance to the Moon was the 2nd-century-BC astronomer and geographer Hipparchus, who exploited the lunar parallax using simple trigonometry, measuring the distance as 400,000 kilometers. He was approximately 26,000 km (16,000 mi) off the actual distance, an error of about 6.8%.
Apollo astronauts who flew to the Moon without landing
Besides the twelve people who have walked on the Moon, twelve more have flown to within 0.001 lunar distance of its surface. During each of the six missions with successful lunar landings, one astronaut remained in lunar orbit while the other two landed. In addition, the three-person crews of Apollo 8 and Apollo 10 also entered lunar orbit, and the crew of Apollo 13 looped around the Moon on a free-return trajectory.All nine manned missions to the Moon took place as part of the Apollo program over a period of just under four years, from 21 December 1968 to 19 December 1972. Of the 24 people who have flown to the Moon, 17 are still living as of November 2015.
John Young, Eugene Cernan and Jim Lovell are the only three people to have flown to the Moon twice. Young and Cernan each set foot on it during their respective second lunar missions, while Lovell is the only person to have flown to the Moon twice without landing.
During Cernan's first lunar mission on Apollo 10, he tied the present record set by Bill Anders on Apollo 8 as the youngest person to fly to the Moon. Each was 35 years and 65 days old on his launch date and 35 years and 68 days old when he entered lunar orbit. (The oldest person to fly to the Moon was Alan Shepard, who walked on its surface during the Apollo 14 mission. Shepard was 47 years and 74 days old on his launch date and 47 years and 78 days old when he entered lunar orbit.)
Because of Apollo 13's free-return trajectory, Lovell, Jack Swigert and Fred Haise flew higher above the Moon's 180° meridian (opposite Earth) than anyone else has flown (254 km/158 mi). Coincidentally, due to the Moon's distance from Earth at the time, they simultaneously set the present record for humans' greatest distance from Earth, reaching an altitude of 400,171 km (248,655 mi) above sea level at 0:21 UTC on 15 April 1970.
| Name | Born | Died | Age on mission | Mission | Mission dates | Service | Notes | |
| 1. | Frank Borman | March 14, 1928 (age 87) | 40 | Apollo 8 | December 21–27, 1968 | Air Force | ||
| 2. | Jim Lovell | March 25, 1928 (age 87) | 40 | Navy | also flew on Apollo 13 | |||
| 3. | Bill Anders | October 17, 1933 (age 82) | 35 | Air Force | ||||
| 4. | Tom Stafford | September 17, 1930 (age 85) | 38 | Apollo 10 | May 18–26, 1969 | Air Force | later flew on Apollo–Soyuz Test Project | |
| John Young | September 24, 1930 (age 85) | 38 | Navy | landed on Apollo 16; later flew two space shuttle missions | ||||
| Eugene Cernan | March 14, 1934 (age 81) | 35 | Navy | landed on Apollo 17 | ||||
| 5. | Michael Collins | October 31, 1930 (age 85) | 38 | Apollo 11 | July 16–24, 1969 | Air Force | ||
| 6. | Dick Gordon | October 5, 1929 (age 86) | 40 | Apollo 12 | November 14–24, 1969 | Navy | trained to land, slated for Apollo 18 (cancelled)[8] | |
| Jim Lovell | March 25, 1928 (age 87) | 42 | Apollo 13 | April 11–17, 1970 | Navy | already flown on Apollo 8; intended to land | ||
| 7. | Jack Swigert | August 30, 1931 | December 27, 1982 (aged 51) | 38 | NASA | |||
| 8. | Fred Haise | November 14, 1933 (age 81) | 36 | NASA[9] | intended to land; later trained to land and slated for Apollo 19 (cancelled);[8] flew shuttle on approach / landing tests | |||
| 9. | Stu Roosa | August 16, 1933 | December 12, 1994 (aged 61) | 37 | Apollo 14 | January 31 – February 9, 1971 | Air Force | in rotation to land on Apollo 20 (cancelled) |
| 10. | Al Worden | February 7, 1932 (age 83) | 39 | Apollo 15 | July 26 – August 7, 1971 | Air Force | ||
| 11. | Ken Mattingly | March 17, 1936 (age 79) | 36 | Apollo 16 | April 16–27, 1972 | Navy | later flew two space shuttle missions. | |
| 12. | Ron Evans | November 10, 1933 | April 7, 1990 (aged 56) | 39 | Apollo 17 | December 7–19, 1972 | Navy |
TYPES OF ORBITS AROUND EARTH
-
Examples
- Earth observation satellites and spy satellites use LEO as they are able to see the surface of the Earth more clearly as they are not so far away. They are also able to traverse the surface of the Earth. A majority of artificial satellites are placed in LEO, making one complete revolution around the Earth in about 90 minutes.
- The International Space Station is in a LEO about 400 km (250 mi) above the Earth's surface.
- Since it requires less energy to place a satellite into a LEO and the LEO satellite needs less powerful amplifiers for successful transmission, LEO is still used for many communication applications. Because these LEO orbits are not geostationary, a network (or "constellation") of satellites is required to provide continuous coverage. (Many communication satellites require geostationary orbits, and move at the same angular velocity as the Earth. Some communications satellites including the Iridium phone system use LEO.)
- Lower orbits also aid remote sensing satellites because of the added detail that can be gained. Remote sensing satellites can also take advantage of sun-synchronous LEO orbits at an altitude of about 800 km (500 mi) and near polar inclination. Envisat is one example of an Earth observation satellite that makes use of this particular type of LEO.
Space debris
The LEO environment is becoming congested with space debris due to the frequency of object launches. This has caused growing concern in recent years, since collisions at orbital velocities can easily be dangerous, and even deadly. Collisions can produce even more space debris in the process, creating a domino effect, something known as Kessler Syndrome. The Joint Space Operations Center, part of United States Strategic Command (formerly the United States Space Command), currently tracks more than 8,500 objects larger than 10 cm in LEO. However, a limited Arecibo Observatory study suggested there could be approximately one million objects larger than 2 millimeters, which are too small to be visible from Earth-based observatories.low earth orbit(LEO)
A low Earth orbit (LEO) is an orbit around Earth with an altitude between 160 kilometers (99 mi) (orbital period
of about 88 minutes), and 2,000 kilometers (1,200 mi) (about 127
minutes). Objects below approximately 160 kilometers (99 mi) will
experience very rapid orbital decay and altitude loss.[1][2]
The orbital velocity needed to maintain a stable low Earth orbit is
about 7.8 km/s, but reduces with increased orbital altitude.
With the exception of the manned lunar flights of the Apollo program, all human spaceflights have taken place in LEO (or were suborbital). The altitude record for a human spaceflight in LEO was Gemini 11 with an apogee of 1,374.1 kilometers (853.8 mi). All manned space stations to date, as well as the majority of satellites, have been in LEO.
Comparison of GPS, GLONASS, Galileo and Compass (medium earth orbit) satellite navigation system orbits with the International Space Station, Hubble Space Telescope and Iridium constellation orbits, Geostationary Earth Orbit, and the nominal size of the Earth.[a] The Moon's orbit is around 9 times larger (in radius and length) than geostationary orbit.
The orbital velocity needed to maintain a stable low Earth orbit is about 7.8 km/s, but reduces with increased orbital altitude. Calculated for circular orbit of 200 km it is 7.79 km/s and for 1500 km it is 7.12 km/s.[3] The delta-v needed to achieve low Earth orbit starts around 9.4 km/s. Atmospheric and gravity drag associated with launch typically adds 1.5–2.0 km/s to the launch vehicle delta-v required to reach normal LEO orbital velocity of around 7.8 km/s (28,080 km/h).
Equatorial low Earth orbits (ELEO) are a subset of LEO. These orbits, with low inclination to the Equator, allow rapid revisit times and have the lowest delta-v requirement (i.e., fuel spend) of any orbit. Orbits with a high inclination angle to the equator are usually called polar orbits.
Higher orbits include medium Earth orbit (MEO), sometimes called intermediate circular orbit (ICO), and further above, geostationary orbit (GEO). Orbits higher than low orbit can lead to early failure of electronic components due to intense radiation and charge accumulation.
Although the Earth's pull due to gravity in LEO is not much less than on the surface of the Earth, people and objects in orbit experience weightlessness because they are in free fall.
A low Earth orbit is simplest and cheapest for satellite placement. It provides high bandwidth and low communication time lag (latency), but satellites in LEO will not be visible from any given point on the Earth at all times.
With the exception of the manned lunar flights of the Apollo program, all human spaceflights have taken place in LEO (or were suborbital). The altitude record for a human spaceflight in LEO was Gemini 11 with an apogee of 1,374.1 kilometers (853.8 mi). All manned space stations to date, as well as the majority of satellites, have been in LEO.
Orbital characteristics
Objects in LEO encounter atmospheric drag in the form of gases in the thermosphere (approximately 80–500 km up) or exosphere (approximately 500 km and up), depending on orbit height. Objects in LEO orbit Earth between the atmosphere and below the inner Van Allen radiation belt. The altitude is usually not less than 300 km for satellites, as that would be impractical due to atmospheric drag.The orbital velocity needed to maintain a stable low Earth orbit is about 7.8 km/s, but reduces with increased orbital altitude. Calculated for circular orbit of 200 km it is 7.79 km/s and for 1500 km it is 7.12 km/s.[3] The delta-v needed to achieve low Earth orbit starts around 9.4 km/s. Atmospheric and gravity drag associated with launch typically adds 1.5–2.0 km/s to the launch vehicle delta-v required to reach normal LEO orbital velocity of around 7.8 km/s (28,080 km/h).
Equatorial low Earth orbits (ELEO) are a subset of LEO. These orbits, with low inclination to the Equator, allow rapid revisit times and have the lowest delta-v requirement (i.e., fuel spend) of any orbit. Orbits with a high inclination angle to the equator are usually called polar orbits.
Higher orbits include medium Earth orbit (MEO), sometimes called intermediate circular orbit (ICO), and further above, geostationary orbit (GEO). Orbits higher than low orbit can lead to early failure of electronic components due to intense radiation and charge accumulation.
Use of LEO
Roughly half an orbit of the ISS.
A low Earth orbit is simplest and cheapest for satellite placement. It provides high bandwidth and low communication time lag (latency), but satellites in LEO will not be visible from any given point on the Earth at all times.
persons to step on moon
Thirty-two astronauts were assigned to fly in the Apollo manned lunar landing program. Twenty-four of these left Earth’s orbit and flew around the Moon (Apollo 1 never launched and Apollo 7 and Apollo 9 were low Earth orbit spacecraft testing missions). In addition, nine astronauts flew Apollo spacecraft in the Apollo Applications Programs Skylab and Apollo–Soyuz Test Project.
Twelve of these astronauts walked on the Moon’s surface, and six of those drove Lunar Roving Vehicles on the Moon. While three astronauts flew to the Moon twice, none of them landed on the Moon more than once. The nine Apollo missions to the Moon occurred between December 1968 and December 1972.
Apart from these 24 people who visited the Moon, no human being has gone beyond low Earth orbit. They have, therefore, been farther from the Earth than anyone else. They are also the only people to have directly viewed the far side of the Moon. The twelve who walked on the Moon are the only people ever to have set foot on an astronomical object other than the Earth.
Of the 24 astronauts who flew to the Moon, two went on to command a Skylab mission, one commanded Apollo–Soyuz, one flew as commander for approach and landing tests of the Space Shuttle, and two went on to command orbital Space Shuttle missions. A total of 24 NASA astronauts from the Apollo era flew on the Space Shuttle.
On each of the Apollo 17 extravehicular activities (EVAs), Harrison Schmitt was the second person out of, and the first person back into, the lunar module. Schmitt is thus the twelfth and last person to have stepped onto the Moon. Eugene Cernan, as the second person to enter the lunar module on the final EVA, is the last person to have walked on the Moon.
Alan Shepard was the oldest person to walk on the Moon, at age 47 years and 79 days. Charlie Duke was the youngest, at age 36 years and 201 days.
Jim Lovell and Fred Haise were scheduled to walk on the Moon during the Apollo 13 mission, but the lunar landing was aborted following a major malfunction en route to the Moon. Haise was again scheduled to walk on the Moon as commander of Apollo 19, but Apollo 18 and Apollo 19 were canceled on September 2, 1970.
Joe Engle had trained on the backup crew for Apollo 14 to explore the Moon with Cernan, but Engle was replaced by Schmitt on the primary crew for Apollo 17. Schmitt had previously been crewed with Apollo 12 command module pilot Dick Gordon in anticipation of Apollo 18, but Schmitt replaced Engle on Apollo 17 after the cancellation of Apollo 18 and Apollo 19, leaving Gordon as the last Apollo astronaut to train extensively for lunar exploration without ever landing on the Moon.
Twelve of these astronauts walked on the Moon’s surface, and six of those drove Lunar Roving Vehicles on the Moon. While three astronauts flew to the Moon twice, none of them landed on the Moon more than once. The nine Apollo missions to the Moon occurred between December 1968 and December 1972.
Apart from these 24 people who visited the Moon, no human being has gone beyond low Earth orbit. They have, therefore, been farther from the Earth than anyone else. They are also the only people to have directly viewed the far side of the Moon. The twelve who walked on the Moon are the only people ever to have set foot on an astronomical object other than the Earth.
Of the 24 astronauts who flew to the Moon, two went on to command a Skylab mission, one commanded Apollo–Soyuz, one flew as commander for approach and landing tests of the Space Shuttle, and two went on to command orbital Space Shuttle missions. A total of 24 NASA astronauts from the Apollo era flew on the Space Shuttle.
Apollo astronauts who walked on the Moon
"Moonwalkers" redirects here. For the upcoming film, see Moonwalkers (film).
Twelve people have walked on the Moon. Eight of them are still living as of November 2015. All manned lunar landings took place between July 1969 and December 1972 as part of the Apollo program.| Name | Born | Died | Age at first step |
Mission | Lunar EVA dates | Service | Alma Mater | |
| 01. | Neil Armstrong | August 5, 1930 | August 25, 2012 (aged 82) | 38y 11m 15d | Apollo 11 | July 21, 1969[6] | NASA[7] | Purdue University, University of Southern California |
| 02. | Buzz Aldrin | January 20, 1930 (age 85) | 39y 6m 0d | Air Force | United States Military Academy, MIT | |||
| 03. | Pete Conrad | June 2, 1930 | July 8, 1999 (aged 69) | 39y 5m 17d | Apollo 12 | November 19–20, 1969 | Navy | Princeton University |
| 04. | Alan Bean | March 15, 1932 (age 83) | 37y 8m 4d | Navy | University of Texas, Austin | |||
| 05. | Alan Shepard | November 18, 1923 | July 21, 1998 (aged 74) | 47y 2m 18d | Apollo 14 | February 5–6, 1971 | Navy | United States Naval Academy, Naval War College |
| 06. | Edgar Mitchell | September 17, 1930 (age 85) | 40y 4m 19d | Navy | Carnegie Mellon University, Naval Postgraduate School, MIT | |||
| 07. | David Scott | June 6, 1932 (age 83) | 39y 1m 25d | Apollo 15 | July 31 – August 2, 1971 | Air Force | University of Michigan (freshman year, and later, an honorary doctorate), United States Military Academy, MIT | |
| 08. | James Irwin | March 17, 1930 | August 8, 1991 (aged 61) | 41y 4m 14d | Air Force | United States Naval Academy, University of Michigan | ||
| 09. | John W. Young | September 24, 1930 (age 85) | 41y 6m 28d | Apollo 16 | April 21–23, 1972 | Navy | Georgia Institute of Technology | |
| 10. | Charles Duke | October 3, 1935 (age 80) | 36y 6m 18d | Air Force | United States Naval Academy, MIT | |||
| 11. | Eugene Cernan | March 14, 1934 (age 81) | 38y 9m 7d | Apollo 17 | December 11–14, 1972 | Navy | Purdue University, Naval Postgraduate School | |
| 12. | Harrison Schmitt | July 3, 1935 (age 80) | 37y 5m 8d | NASA | Caltech, University of Oslo (exchange), Harvard University |
Alan Shepard was the oldest person to walk on the Moon, at age 47 years and 79 days. Charlie Duke was the youngest, at age 36 years and 201 days.
Jim Lovell and Fred Haise were scheduled to walk on the Moon during the Apollo 13 mission, but the lunar landing was aborted following a major malfunction en route to the Moon. Haise was again scheduled to walk on the Moon as commander of Apollo 19, but Apollo 18 and Apollo 19 were canceled on September 2, 1970.
Joe Engle had trained on the backup crew for Apollo 14 to explore the Moon with Cernan, but Engle was replaced by Schmitt on the primary crew for Apollo 17. Schmitt had previously been crewed with Apollo 12 command module pilot Dick Gordon in anticipation of Apollo 18, but Schmitt replaced Engle on Apollo 17 after the cancellation of Apollo 18 and Apollo 19, leaving Gordon as the last Apollo astronaut to train extensively for lunar exploration without ever landing on the Moon.
Saturday, October 31, 2015
can stephen halking talk?
Professor Hawking has motor neurone disease and as such is only able to communicate by using a small sensor which is activated by a muscle in his cheek. He uses this sensor to 'type' characters and numbers on his keyboard.
stephen public lectures
Public Lectures
Professor
Hawking has given many lectures to the general public. Below are some of
the more recent public lectures. Included with these lectures is a
Glossary of some of the terms used.
Into a Black Hole 2008
Is it possible to fall in a black hole, and come out in another universe? Can you escape from a black hole once you fall inside? In this lecture I talk about some of the things I've found out about black holes.
The Origin of the Universe 2005
Why are we here? Where did we come from? The answer generally given was that humans were of comparatively recent origin, because it must have been obvious, even at early times, that the human race was improving in knowledge and technology. So it can't have been around that long, or it would have progressed even more.
Godel and the End of Physics 2002In this talk, I want to ask how far can we go in our search for understanding and knowledge. Will we ever find a complete form of the laws of nature? By a complete form, I mean a set of rules that in principle at least enable us to predict the future to an arbitrary accuracy, knowing the state of the universe at one time. A qualitative understanding of the laws has been the aim of philosophers and scientists, from Aristotle onwards.
Space and Time Warps 1999
In science fiction, space and time warps are a commonplace. They are used for rapid journeys around the galaxy, or for travel through time. But today's science fiction, is often tomorrow's science fact. So what are the chances for space and time warps.
Does God Play Dice 1999
This lecture is about whether we can predict the future, or whether it is arbitrary and random. In ancient times, the world must have seemed pretty arbitrary. Disasters such as floods or diseases must have seemed to happen without warning or apparent reason. Primitive people attributed such natural phenomena, to a pantheon of gods and goddesses, who behaved in a capricious and whimsical way. There was no way to predict what they would do, and the only hope was to win favour by gifts or actions.
The Beginning of Time 1996In this lecture, I would like to discuss whether time itself has a beginning, and whether it will have an end. All the evidence seems to indicate, that the universe has not existed forever, but that it had a beginning, about 15 billion years ago. This is probably the most remarkable discovery of modern cosmology. Yet it is now taken for granted. We are not yet certain whether the universe will have an end.
Life in the Universe 1996
In this talk, I would like to speculate a little, on the development of life in the universe, and in particular, the development of intelligent life. I shall take this to include the human race, even though much of its behaviour through out history, has been pretty stupid, and not calculated to aid the survival of the species.
Into a Black Hole 2008
Is it possible to fall in a black hole, and come out in another universe? Can you escape from a black hole once you fall inside? In this lecture I talk about some of the things I've found out about black holes.
The Origin of the Universe 2005
Why are we here? Where did we come from? The answer generally given was that humans were of comparatively recent origin, because it must have been obvious, even at early times, that the human race was improving in knowledge and technology. So it can't have been around that long, or it would have progressed even more.
Godel and the End of Physics 2002In this talk, I want to ask how far can we go in our search for understanding and knowledge. Will we ever find a complete form of the laws of nature? By a complete form, I mean a set of rules that in principle at least enable us to predict the future to an arbitrary accuracy, knowing the state of the universe at one time. A qualitative understanding of the laws has been the aim of philosophers and scientists, from Aristotle onwards.
Space and Time Warps 1999
In science fiction, space and time warps are a commonplace. They are used for rapid journeys around the galaxy, or for travel through time. But today's science fiction, is often tomorrow's science fact. So what are the chances for space and time warps.
Does God Play Dice 1999
This lecture is about whether we can predict the future, or whether it is arbitrary and random. In ancient times, the world must have seemed pretty arbitrary. Disasters such as floods or diseases must have seemed to happen without warning or apparent reason. Primitive people attributed such natural phenomena, to a pantheon of gods and goddesses, who behaved in a capricious and whimsical way. There was no way to predict what they would do, and the only hope was to win favour by gifts or actions.
The Beginning of Time 1996In this lecture, I would like to discuss whether time itself has a beginning, and whether it will have an end. All the evidence seems to indicate, that the universe has not existed forever, but that it had a beginning, about 15 billion years ago. This is probably the most remarkable discovery of modern cosmology. Yet it is now taken for granted. We are not yet certain whether the universe will have an end.
Life in the Universe 1996
In this talk, I would like to speculate a little, on the development of life in the universe, and in particular, the development of intelligent life. I shall take this to include the human race, even though much of its behaviour through out history, has been pretty stupid, and not calculated to aid the survival of the species.
stephen halking publications
Publications
- George and the Unbreakable Code. L. Hawking. S.W.Hawking. Jun 2014. ISBN-13: 978-0857533258
- Information Preservation and Weather Forecasting for Black Holes. S.W. Hawking. Jan 2014. arXiv:1401.5761v1 [hep-th]
- My Brief History. S.W. Hawking, Sep 2013. 144 pp ISBN-13: 978-0345535283
- Vector Fields in Holographic Cosmology. James B.Hartle. S.W. Hawking, Thomas Hertog. May 2013. 17 pp. arXiv:1305.7190v1 [hep-th], DOI: 10.1007/JHEP11(2013)201
- George and the Big Bang. L. Hawking. S.W.Hawking. Aug 2012. ISBN-13: 978-1442440050
- Quantum Probabilities for Inflation from Holography. James B.Hartle. S.W. Hawking, Thomas Hertog. Jul 2012. arXiv:1207.6653v3 [hep-th], DOI: 10.1088/1475-7516/2014/01/015
- Accelerated Expansion from Negative Lambda. James B. Hartle (UC, Santa Barbara), S.W. Hawking (Cambridge U., DAMTP), Thomas Hertog (Leuven U. & Intl. Solvay Inst., Brussels). May 2012. 28 pp. arXiv:1205.3807v3 [hep-th]
- George's Cosmic Treasure Hunt. L. Hawking. S.W.Hawking. May 2011. ISBN-13: 978-1442421752
- The dreams that stuff is made of: The most astounding papers of quantum physics - and how they shook the scientific world. Stephen Hawking, (ed.) (Cambridge U., DAMTP). 2011. 1071 pp. Published in Philadelphia, USA: Running Pr. (2011) 1071 p. ISBN-13: 978-0762434343
- Local Observation in Eternal inflation. James Hartle (UC, Santa Barbara), S.W. Hawking (Cambridge U.,DAMTP), Thomas Hertog (APC, Paris & Intl. Solvay Inst., Brussels). Sep 2010. 4 pp. Published in Phys.Rev.Lett. 106 (2011) 141302. arXiv:1009.2525v2 [hep-th], DOI: 10.1103/PhysRevLett.106.141302
- The Grand Design. S.W.Hawking and L. Mlodinov (Sep 2010), ISBN-13: 978-0553805376
- The No-Boundary Measure in the Regime of Eternal Inflation. James Hartle (UC, Santa Barbara), S.W. Hawking (Cambridge U., DAMTP), Thomas Hertog (APC, Paris & Intl. Solvay Inst., Brussels). Jan 2010. 29 pp. Published in Phys.Rev. D82 (2010) 063510. arXiv:1001.0262v1 [hep-th], DOI: 10.1103/PhysRevD.82.063510
- George's Secret Key to the Universe. L. Hawking. S.W.Hawking. May 2009. ISBN-13: 978-1416985846
- Why did the Universe Inflate? S.W. Hawking (Cambridge U., DAMTP). 2009. 7 pp. DOI: 10.1007/978-0-387-87499-9_10
- The Classical Universes of the No-Boundary Quantum State.
James B. Hartle (UC, Santa Barbara), S.W. Hawking (Cambridge
U.,DAMTP), Thomas Hertog (APC, Paris & Intl. Solvay Inst.,
Brussels). Mar 2008. 46 pp. arXiv:0803.1663 [hep-th], DOI: 10.1103/PhysRevD.77.123537
- No-Boundary Measure of the Universe.
James B. Hartle (UC, Santa Barbara), S.W. Hawking (Cambridge U.,
DAMTP), Thomas Hertog (APC, Paris & Intl. Solvay Inst., Brussels).
Nov 2007. 4 pp. Published in Phys.Rev.Lett. 100 (2008) 201301. arXiv:0711.4630 [hep-th], DOI: 10.1103/PhysRevLett.100.201301
- Volume Weighting in the No Boundary Proposal. S.W. Hawking. Oct 2007. 7 pp. arXiv:0710.2029 [hep-th]
- God created the Integers. S.W.Hawking. Oct 2007. ISBN-13: 978-0762430048
- The measure of the universe. S.W. Hawking (Cambridge U., DAMTP). 2007. 6 pp. Published in AIP Conf.Proc. 957 (2007) 79-84, DOI: 10.1063/1.2823830
- Populating the landscape: A Top down approach. S.W. Hawking (Cambridge U., DAMTP), Thomas Hertog (CERN). CERN-PH-TH-2006-022. Feb 2006. 22 pp. Published in Phys.Rev. D73 (2006) 123527. arXiv:hep-th/0602091, DOI: 10.1103/PhysRevD.73.123527
- Information loss in black holes. S.W. Hawking (Cambridge U., DAMTP). DAMTP-2005-66. Jul 2005. 5 pp. Published in Phys.Rev. D72 (2005) 084013. arXiv:hep-th/0507171, DOI: 10.1103/PhysRevD.72.084013
- A non singular universe. S. Hawking (Cambridge U., DAMTP). 2005. 2 pp. Published in Phys.Scripta T117 (2005) 49-50
- A briefer history of time. S. Hawking (Cambridge U., DAMTP), L. Mlodinow. 2005. 189 pp. Published in Reinbek, Germany: Rowohlt (2005) 189 p. ISBN-13: 978-0553385465
- Black holes and the information paradox. S. Hawking (Cambridge U., DAMTP). Jul 2004. 7 pp. Prepared for Conference: C04-07-18, p.56-62 Proceedings
- The grand Stephen Hawking reader: Life and work. H. Mania, (ed.), S. Hawking. 2004. 291 pp. Published in (rororo. 61655)
- Cosmology from the top down. Stephen W. Hawking (Cambridge U., DAMTP). DAVISINFLATION-2003-PELLY. May 2003. Published in In *Carr, Bernard (ed.): Universe or multiverse?* 91-98. arXiv:astro-ph/0305562
- On the Shoulders of Giants. N. Copernicus, J. Kepler, G. Galalei, I. Newton, A. Einstein (Author), S. Hawking. Dec 2003. ISBN-13: 978-0762416981
- The illustrated theory of everything: The origin and fate of the universe. S.W. Hawking (Cambridge U., DAMTP). 2003. 119 pp. Published in Beverly Hills, USA: New Millennium Pr. (2003) 119 p
- Brane new world.Stephen Hawking (Cambridge U., DAMTP). Aug 2002. 7 pp. Published in Conf.Proc. C0208124 (2002) 1-7
- Why does inflation start at the top of the hill? S.W Hawking, Thomas Hertog (Cambridge U., DAMTP). Apr 2002. 21 pp. Published in Phys.Rev. D66 (2002) 123509. arXiv:hep-th/0204212, DOI: 10.1103/PhysRevD.66.123509
- Sixty years in a nutshell. S. Hawking (Newton Inst. Math. Sci., Cambridge). Jan 2002. Prepared for Workshop on Conference on the Future of Conference: C02-01-07.7
- Chronology protection: Making the world safe for historians. S.W. Hawking. 2002. Published in In *Hawking, S.W. et al.: The future of spacetime* 87-108
- The Future of space-time. S.W. Hawking, K.S. Thorne, I. Novikov, T. Ferris, A. Lightman, R. Price. 2002. 220 pp. Published in New York, USA: Norton (2002) 220 p
- Why does inflation start at the top of the hill? S.W. Hawking (Cambridge U., DAMTP). Nov 2001. Prepared for Conference: C01-11-13.1
- Living with ghosts. S.W. Hawking, Thomas Hertog (Cambridge U., DAMTP). Jul 2001. 13 pp. Published in Phys.Rev. D65 (2002) 103515. arXiv:hep-th/0107088, DOI: 10.1103/PhysRevD.65.103515
- The universe in a nutshell. S. Hawking (Cambridge U., DAMTP). 2001. 224 pp. ISBN-13: 978-0553802023
- Trace anomaly driven inflation.
S.W. Hawking, T. Hertog (Cambridge U., DAMTP), H.S. Reall (Queen Mary,
U. of London). DAMTP-2000-92, QMW-PH-00-10. Oct 2000. 40 pp. Published in Phys.Rev. D63 (2001) 083504. arXiv:hep-th/0010232, DOI: 10.1103/PhysRevD.63.083504
- Large N cosmology.S.W. Hawking (Cambridge U., DAMTP). Sep 2000. Prepared for Conference: C00-09-04.4
- Brane new world. S.W. Hawking, T. Hertog, H.S. Reall (Cambridge U., DAMTP). DAMTP-2000-25. Mar 2000. 28 pp. Published in Phys.Rev. D62 (2000) 043501. arXiv:hep-th/0003052, DOI: 10.1103/PhysRevD.62.043501
- Gravitational waves in open de Sitter space. S.W. Hawking, Thomas Hertog, Neil Turok (Cambridge U., DAMTP). Mar 2000. 17 pp. Published in Phys.Rev. D62 (2000) 063502. arXiv:hep-th/0003016, DOI: 10.1103/PhysRevD.62.063502
- de Sitter entropy, quantum entanglement and AdS / CFT. Stephen Hawking (Cambridge U., DAMTP), Juan Martin Maldacena, Andrew Strominger (Harvard U.). Feb 2000. 14 pp. Published in JHEP 0105 (2001) 001. arXiv:hep-th/0002145, DOI: 10.1088/1126-6708/2001/05/001
- Stability of AdS and phase transitions. S.W. Hawking (Cambridge U., DAMTP). 2000. Published in Class.Quant.Grav. 17 (2000) 1093-1099, DOI: 10.1088/0264-9381/17/5/318
- Brane world black holes. A. Chamblin, S.W. Hawking, H.S. Reall (Cambridge U., DAMTP). DAMTP-1999-133. Sep 1999. 9 pp. Published in Phys.Rev. D61 (2000) 065007. arXiv:hep-th/9909205, DOI: 10.1103/PhysRevD.61.065007
- Charged and rotating AdS black holes and their CFT duals. S.W. Hawking, H.S. Reall (Cambridge U., DAMTP). DAMTP-R-99-108. Aug 1999. 18 pp. Published in Phys.Rev. D61 (2000) 024014. arXiv:hep-th/9908109, DOI: 10.1103/PhysRevD.61.024014
- Primordial black holes: Pair creation, Lorentzian condition, and evaporation. R. Bousso (Stanford U., Phys. Dept.), S.W. Hawking (Cambridge U.). 1999. Published in Int.J.Theor.Phys. 38 (1999) 1227-, DOI: 10.1023/A:1026618832525
- A debate on open inflation. S.W. Hawking (Cambridge U., DAMTP). Nov 1998. Published in AIP Conf.Proc. 478 (1999) 15-22
- Rotation and the AdS / CFT correspondence. S.W. Hawking, C.J. Hunter, Marika Taylor (Cambridge U., DAMTP). Nov 1998. 24 pp. Published in Phys.Rev. D59 (1999) 064005. arXiv:hep-th/9811056, DOI: 10.1103/PhysRevD.59.064005
- Nut charge, anti-de Sitter space and entropy. S.W. Hawking, C.J. Hunter (Cambridge U.), Don N. Page (Alberta U.). DAMTP-98-122. Sep 1998. 13 pp. Published in Phys.Rev. D59 (1999) 044033. arXiv:hep-th/9809035, DOI: 10.1103/PhysRevD.59.044033
- Gravitational entropy and global structure. S.W. Hawking, C.J. Hunter (Cambridge U.). DAMTP-98-104. Aug 1998. 19 pp. Published in Phys.Rev. D59 (1999) 044025. arXiv:hep-th/9808085, DOI: 10.1103/PhysRevD.59.044025
- Open inflation. S.W. Hawking (CAMBRIDGE U.). Aug 1998. Prepared for 2nd Samos Meeting on Cosmology, Geometry and Re Conference: C98-08-31.4
- Lorentzian condition in quantum gravity. Raphael Bousso (Stanford U., Phys. Dept.), Stephen W. Hawking (Cambridge U.). SU-ITP-98-26, DAMTP-98-87. Jul 1998. 14 pp. Published in Phys.Rev. D59 (1999) 103501, Erratum-ibid. D60 (1999) 109903. arXiv:hep-th/9807148, DOI: 10.1103/PhysRevD.60.109903, 10.1103/PhysRevD.59.103501
- Inflation, singular instantons and eleven-dimensional cosmology. S.W. Hawking, Harvey S. Reall (Cambridge U.). DAMTP-98-85. Jul 1998. 19 pp. Published in Phys.Rev. D59 (1999) 023502. arXiv:hep-th/9807100, DOI: 10.1103/PhysRevD.59.023502
- Open inflation, the four form and the cosmological constant. Neil Turok, S.W. Hawking (Cambridge U.). Mar 1998. 11 pp. Published in Phys.Lett. B432 (1998) 271-278. arXiv:hep-th/9803156, DOI: 10.1016/S0370-2693(98)00651-0
- Open inflation without false vacua. S.W. Hawking, Neil Turok (Cambridge U.). Feb 1998. 10 pp. Published in Phys.Lett. B425 (1998) 25-32. arXiv:hep-th/9802030, DOI: 10.1016/S0370-2693(98)00234-2
- Comment on 'quantum creation of an open universe', by Andrei Linde. S.W. Hawking, Neil Turok (Cambridge U.). Feb 1998. 4 pp. arXiv:gr-qc/9802062
- Is information lost in black holes?. S.W. Hawking (Cambridge U.). 1998. Published in In *Wald, R.M. (ed.): Black holes and relativistic stars* 221-240
- Bulk charges in eleven-dimensions. S.W. Hawking, Marika Taylor (Cambridge U.). DAMTP-R-97-52. Nov 1997. 26 pp. Published in Phys.Rev. D58 (1998) 025006. arXiv:hep-th/9711042, DOI: 10.1103/PhysRevD.58.025006
- Evaporation of cosmological black holes. R. Bousso (Stanford U., Phys. Dept.), S.W. Hawking (Cambridge U., DAMTP). Nov 1997. 14 pp. Prepared for Conference: C97-11-11.1
- (Anti)evaporation of Schwarzschild-de Sitter black holes. Raphael Bousso, Stephen W. Hawking (Cambridge U.). DAMTP-R-97-26. Sep 1997. 16 pp. Published in Phys.Rev. D57 (1998) 2436-2442. arXiv:hep-th/9709224, DOI: 10.1103/PhysRevD.57.2436
- Models for chronology selection. M.J. Cassidy, S.W. Hawking (Cambridge U.). DAMTP-R-97-47. Sep 1997. 20 pp. Published in Phys.Rev. D57 (1998) 2372-2380. arXiv:hep-th/9709066, DOI: 10.1103/PhysRevD.57.2372
- Evaporation of primordial black holes. S.W. Hawking (Cambridge U., DAMTP). Aug 1997. Prepared for 6th Conference on Quantum Mechanics of Conference: C97-11-11.1
- Trace anomaly of dilaton coupled scalars in two-dimensions. Raphael Bousso, Stephen W. Hawking (Cambridge U.). DAMTP-R-97-25. May 1997. 11 pp. Published in Phys.Rev. D56 (1997) 7788-7791. arXiv:hep-th/9705236, DOI: 10.1103/PhysRevD.56.7788
- Loss of quantum coherence through scattering off virtual black holes. S.W. Hawking (Cambridge U.), Simon F. Ross (UC, Santa Barbara). DAMTP-R-97-21, UCSB-TH-97-08. May 1997. 29 pp. Published in Phys.Rev. D56 (1997) 6403-6415. arXiv:hep-th/9705147, DOI: 10.1103/PhysRevD.56.6403
- Evolution of near extremal black holes. S.W. Hawking, Marika Taylor (Cambridge U.). DAMTP-R-96-56. Feb 1997. 25 pp. Published in Phys.Rev. D55 (1997) 7680-7692. arXiv:hep-th/9702045, DOI: 10.1103/PhysRevD.55.7680
- Evaporation of cosmological black holes. R. Bousso (Stanford U., Phys. Dept.), S.W. Hawking (Cambridge U., DAMTP). 1997. Published in In *Ambleside 1997, Particle physics and the early universe* 481-494
- The Nature of space and time. S.W. Hawking, R. Penrose. Jul 1996. Published in Sci.Am. 275 (1996) 44-49
- Pair creation of black holes during inflation. Raphael Bousso, Stephen W. Hawking (Cambridge U.). DAMTP-R-96-33. Jun 1996. 29 pp. Published in Phys.Rev. D54 (1996) 6312-6322
- Loss of information in black holes. S. Hawking (Cambridge U., DAMTP). Jun 1996. Prepared for Conference on Geometric Issues in Foundations Conference: C96-06-25.2
- Primordial black holes: Tunneling versus no boundary proposal. Raphael Bousso, Stephen W. Hawking (Cambridge U., DAMTP). DAMTP-R-96-34, C96-05-25. May 1996. 14 pp. Published in Grav.Cosmol.Suppl. 4 (1998) 28-37. arXiv:gr-qc/9608009
- Pair creation and evolution of black holes in inflation. Raphael Bousso, Stephen W. Hawking (Cambridge U.). DAMTP-R-96-35, C96-05-26. May 1996. 8 pp. Published in Helv.Phys.Acta 69 (1996) 261-264. arXiv:gr-qc/9608008, DOI: 10.1103/PhysRevD.54.6312
- The Gravitational Hamiltonian in the presence of nonorthogonal boundaries. S.W. Hawking, C.J. Hunter (Cambridge U.). DAMTP-R-96-9. Mar 1996. 19 pp. Published in Class.Quant.Grav. 13 (1996) 2735-2752. arXiv:gr-qc/9603050, DOI: 10.1088/0264-9381/13/10/012
- Black holes in inflation. R. Bousso, S.W. Hawking (Cambridge U., DAMTP). 1996. Published in Nucl.Phys.Proc.Suppl. 57 (1997) 201-205, DOI: 10.1016/S0920-5632(97)00377-0
- The Nature of space and time. S. Hawking, R. Penrose. 1996. Published in Princeton, USA: Univ. Pr. (1996) 141 p. (The Isaac Newton Institute series of lectures)
- Virtual black holes. S.W. Hawking (Cambridge U.). DAMTP-R-95-50. Oct 1995. 24 pp. Published in Phys.Rev. D53 (1996) 3099-3107. arXiv:hep-th/9510029, DOI: 10.1103/PhysRevD.53.3099
- The Probability for primordial black holes. R. Bousso, S.W. Hawking (Cambridge U.). DAMTP-R-95-33. Jun 1995. 15 pp. Published in Phys.Rev. D52 (1995) 5659-5664. arXiv:gr-qc/9506047, DOI: 10.1103/PhysRevD.52.5659
- Pair production of black holes on cosmic strings. S.W. Hawking, Simon F. Ross (Cambridge U.). DAMTP-R-95-30. Jun 1995. 9 pp. Published in Phys.Rev.Lett. 75 (1995) 3382-3385. arXiv:gr-qc/9506020, DOI: 10.1103/PhysRevLett.75.3382
- Duality between electric and magnetic black holes. S.W. Hawking, Simon F. Ross (Cambridge U.). DAMTP-R-95-8. Apr 1995. 16 pp. Published in Phys.Rev. D52 (1995) 5865-5876. arXiv:hep-th/9504019, DOI: 10.1103/PhysRevD.52.5865
- The Gravitational Hamiltonian, action, entropy and surface terms. S.W. Hawking (Cambridge U.), Gary T. Horowitz (UC, Santa Barbara). DAMTP-R-94-52, UCSBTH-94-37. Jan 1995. 13 pp. Published in Class.Quant.Grav. 13 (1996) 1487-1498. arXiv:gr-qc/9501014, DOI: 10.1088/0264-9381/13/6/017
- Quantum coherence and closed timelike curves. S.W. Hawking (Cambridge U.). DAMTP-R-95-04. Jan 1995. 12 pp. Published in Phys.Rev. D52 (1995) 5681-5686. arXiv:gr-qc/9502017, DOI: 10.1103/PhysRevD.52.5681
- Black holes and baby universes and other essays. S. Hawking. 1995. Published in Toronto, Canada: Bantam Books (1994) 172 p, ISBN-13: 978-0553374117
- Entropy, Area, and black hole pairs.
S.W. Hawking, Gary T. Horowitz (Newton Inst. Math. Sci., Cambridge),
Simon F. Ross (Cambridge U.). NI-94-012, DAMTP-R-94-26, UCSBTH-94-25.
Sep 1994. 24 pp. Published in Phys.Rev. D51 (1995) 4302-4314. arXiv:gr-qc/9409013, DOI: 10.1103/PhysRevD.51.4302
- Nature of space and time. S.W. Hawking (Cambridge U.). Sep 1994. 62 pp. arXiv:hep-th/9409195
- Euclidean quantum gravity. G.W. Gibbons, (ed.), S.W. Hawking, (ed.) (Cambridge U.). 1994. Published in Singapore, Singapore: World Scientific (1993) 586 p
- The Superscattering matrix for two-dimensional black holes. S.W. Hawking (Cambridge U. & Caltech). Nov 1993. 12 pp. Published in Phys.Rev. D50 (1994) 3982-3986. arXiv:hep-th/9401109, DOI: 10.1103/PhysRevD.50.3982
- Quantum coherence in two-dimensions. S.W. Hawking, J.D. Hayward (Cambridge U. & Caltech). CALT-68-1861, DAMTP-R-93-12. Mar 1993. 14 pp. Published in Phys.Rev. D49 (1994) 5252-5256. arXiv:hep-th/9305165, DOI: 10.1103/PhysRevD.49.5252
- Supersymmetric Bianchi models and the square root of the Wheeler-DeWitt equation. P.D. D'Eath, S.W. Hawking (Cambridge U.), O. Obregon (Guanajuato U., FIMEE). DAMTP-R-92-44. Feb 23, 1993. 11 pp. Published in Phys.Lett. B300 (1993) 44-48, DOI: 10.1016/0370-2693(93)90746-5
- The Origin of time asymmetry.
S.W. Hawking (Cambridge U.), R. Laflamme (Cambridge U. &
Los Alamos), G.W. Lyons (Cambridge U.). PRINT-93-0178
(DAMTP,CAMBRIDGE). Feb 12, 1993. 41 pp. Published in Phys.Rev. D47 (1993) 5342-5356. arXiv:gr-qc/9301017, DOI: 10.1103/PhysRevD.47.5342
- Einstein's dream: Expeditions to the frontiers of space-time. Black holes and baby universes and other essays. (In German). S.W. Hawking. 1993. Published in Reinbek, Germany: Rowohlt (1993) 190 p
- Naked and thunderbolt singularities in black hole evaporation. S.W. Hawking, J.M. Stewart (Cambridge U.). PRINT-92-0362 (DAMTP,CAMBRIDGE), DAMTP-R-92-37. Jul 1992. 28 pp. Published in Nucl.Phys. B400 (1993) 393-415. arXiv:hep-th/9207105, DOI: 10.1016/0550-3213(93)90410-Q
- Evaporation of two-dimensional black holes. S.W. Hawking (Caltech & Cambridge U.). CALT-68-1774. Mar 20, 1992. 11 pp. Published in Phys.Rev.Lett. 69 (1992) 406-409. arXiv:hep-th/9203052, DOI: 10.1103/PhysRevLett.69.406
- Kinks and topology change. G.W. Gibbons, S.W. Hawking (Cambridge U.). 1992. Published in Phys.Rev.Lett. 69 (1992) 1719-1721, DOI: 10.1103/PhysRevLett.69.1719
- Evaporation of two-dimensional black holes. S.W. Hawking (Cambridge U.). 1992. Published in In *Trieste 1992, Proceedings, The renaissance of general relativity and cosmology* 274-286
- Selection rules for topology change. G.W. Gibbons, S.W. Hawking (Cambridge U.). PRINT-91-0452 (DAMTP,CAMBRIDGE). Nov 12, 1991. 14 pp. Published in Commun.Math.Phys. 148 (1992) 345-352, DOI: 10.1007/BF02100864
- The no boundary condition and the arrow of time. S.W. Hawking (Cambridge U., DAMTP). Sep 1991. Prepared for NATO Workshop on the Physical Origin of Conference: C91-09-30.4
- The Chronology protection conjecture. S.W. Hawking (Cambridge U.). DAMTP-R-91-15. Jul 1991. 24 pp. Published in Phys.Rev. D46 (1992) 603-611, DOI: 10.1103/PhysRevD.46.603
- Wormholes in string theory. Alex Lyons (Alberta U.), S.W. Hawking (Cambridge U.). ALBERTA-THY-5-91. May 1991. 40 pp. Published in Phys.Rev. D44 (1991) 3802-3818, DOI: 10.1103/PhysRevD.44.3802
- The Alpha parameters of wormholes. S.W. Hawking (Cambridge U.). 1991. Published in Phys.Scripta T36 (1991) 222-227, DOI: 10.1088/0031-8949/1991/T36/023
- The chronology protection conjecture. S.W. Hawking (Cambridge U., DAMTP). 1991. Published
in In *Kyoto 1991, Recent developments in theoretical and experimental
general relativity, gravitation and relativistic field theories, pt.
A* 3-13
- Beginning or end? Inaugural lecture. (In German). S. Hawking, (ed.) (Cambridge U.). 1991. Published in Paderborn, Germany: Junfermann (1991) 43 p
- The Effective action for wormholes. S.W. Hawking (Cambridge U.). PRINT-90-0682 (CAMBRIDGE). Nov 23, 1990. 19 pp. Published in Nucl.Phys. B363 (1991) 117-131, DOI: 10.1016/0550-3213(91)90237-R
- The beginning of the universe. S.W. Hawking (Cambridge U., DAMTP). Sep 1990. Prepared for (IUPAP) International Conference on Primordial Conference: C90-09-04.2
- The spectrum of wormholes.
S.W. Hawking (Santa Barbara, KITP & Cambridge U.), Don N. Page
(Santa Barbara, KITP & Penn State U. & Alberta U.).
NSF-ITP-90-76. Jun 17, 1990. 37 pp. Published in Phys.Rev. D42 (1990) 2655-2663, DOI: 10.1103/PhysRevD.42.2655
- Gravitational radiation from collapsing cosmic string loops. S.W. Hawking (Cambridge U.). DAMTP/R-90-14. Apr 1990. 7 pp. Published in Phys.Lett. B246 (1990) 36-38, DOI: 10.1016/0370-2693(90)91304-T
- Wormholes and nonsimply connected manifolds. S.W. Hawking (Cambridge U.). DAMTP-R-90-13. Jan 1990. 23 pp.
Published in In *Jerusalem 1989, Proceedings, Quantum cosmology and
baby universes* 245-267 and Cambridge Univ. - DAMTP-R-90-13
(90,rec.Jul.) 23 p
- Baby universes. 2. S.W. Hawking (Cambridge U.). 1990. Published in Mod.Phys.Lett. A5 (1990) 453-466, DOI: 10.1142/S0217732390000524
- Wormholes in dimensions 1 - 4. S.W. Hawking (Cambridge U.). 1990. Published
in In *Boston 1990, Proceedings, Particles, strings and cosmology*
623-634. (see HIGH ENERGY PHYSICS INDEX 29 (1991) No.9950)
- The Formation and evolution of cosmic strings. Proceedings, Workshop, Cambridge, UK, July 3-7, 1989. G.W. Gibbons, (ed.), S.W. Hawking, (ed.), T. Vachaspati, (ed.) (Cambridge U. & Tufts U.). 1990. Published in Cambridge, UK: Univ. Pr. (1990) 542 p
- Do Wormholes Fix The Constants Of Nature?. S.W. Hawking (Cambridge U.). Print-89-0795 (CAMBRIDGE), DAMTP/R-89/13. May 1989. 12 pp. Published in Nucl.Phys. B335 (1990) 155, DOI: 10.1016/0550-3213(90)90175-D
- The Edge Of Space-time. S. Hawking (Cambridge U.). 1989. Published in IN *DAVIES, P. (ED.): THE NEW PHYSICS* 61-69
- Baby Universes And The Nonrenormalizability Of Gravity. S.W. Hawking, R. Laflamme (Cambridge U.). Print-88-0290(CAMBRIDGE), DAMTP/R-88/3. Mar 1988. 6 pp. Published in Phys.Lett. B209 (1988) 39, DOI: 10.1016/0370-2693(88)91825-4
- Wormholes in Space-Time. S.W. Hawking (Cambridge U.). 1988. Published in Phys.Rev. D37 (1988) 904-910, DOI: 10.1103/PhysRevD.37.904
- Baby universes. S.W. Hawking (Cambridge U.). 1988. Published in In *Leningrad 1988, Proceedings, A.A. Friedmann:Centenary volume* 81-92.
- A Brief History Of Time. S.W. Hawking. 1988. Published by Bantam (Sep 1988) 212p, ISBN-13: 978-0553380163
- Quantum Cosmology. S.W. Hawking (Cambridge U.). 1988. Published
in IN *FANG, LI-ZHI (ED.), RUFFINI, R. (ED.): QUANTUM COSMOLOGY*,
190-235 AND PREPRINT - HAWKING, S.W. (83,REC.DEC.) 64 P.
- The Quantum Theory Of The Universe. S.W. Hawking (Cambridge U.). 1988. Published in IN *JERUSALEM 1983/84, PROCEEDINGS, INTERSECTION BETWEEN ELEMENTARY PARTICLE PHYSICS AND COSMOLOGY*, 71-97.
- Black Holes From Cosmic Strings. S.W. Hawking (Cambridge U.). Print-88-0310 (CAMBRIDGE). Dec 1987. 5 pp. Published in Phys.Lett. B231 (1989) 237, DOI: 10.1016/0370-2693(89)90206-2
- The Direction Of Time. S.W. Hawking (Cambridge U.). Print-87-0849 (DAMTP). Nov 10, 1987. 10 pp. Published in New Sci. 115 (1987) 46
- How probable is inflation?. S.W. Hawking (Cambridge U.), Don N. Page (Penn State U.). Print-87-0739 (PENN STATE). Jun 1987. 30 pp. Published in Nucl.Phys. B298 (1988) 789-809, DOI: 10.1016/0550-3213(88)90008-9
- The Origin Of The Universe. S.W. Hawking (Cambridge U.). Print-87-0841 (CAMBRIDGE). Jun 1987. 10 pp.
- The Ground State Of The Universe. S.W. Hawking (Cambridge U.). Print-87-0845 (CAMBRIDGE), C87/05/01.2. May 1987. 3 pp. Closing Remarks given at Conference: C87-05-01.2
- Quantum Coherence Down the Wormhole. S.W. Hawking (Cambridge U.). Print-87-0842 (CAMBRIDGE). Apr 1987. 12 pp. Published in Phys.Lett. B195 (1987) 337, DOI: 10.1016/0370-2693(87)90028-1
- The Schrodinger Equation In Quantum Cosmology And String Theory. S.W. Hawking (Cambridge U.). Print-87-0843 (CAMBRIDGE). Mar 1987. 10 pp.
- Three Hundred Years Of Gravitation. S.W. Hawking, (Ed.), W. Israel, (Ed.). 1987. Published in Cambridge, UK: Univ. Pr. (1987) 684 p
- Quantum Cosmology. S.W. Hawking (Cambridge U.). Print-87-0166 (CAMBRIDGE), C87/06/29. Dec 1986. 31 pp. Published
in In *Hawking, S.W. (ed.), Israel, W. (ed.): Three hundred years of
gravitation*, 631-651 and Preprint - Hawking, S.W. (86,rec.Jan.87) 31 p
- A Natural Measure On The Set Of All Universes. G.W. Gibbons, S.W. Hawking, J.M. Stewart (Cambridge U.).PRINT-86-1241. Oct 14, 1986. 19 pp. Published in Nucl.Phys. B281 (1987) 736, DOI: 10.1016/0550-3213(87)90425-1
- The Density Matrix Of The Universe. S.W. Hawking (Cambridge U.). PRINT-86-0918 (CAMBRIDGE). Apr 1986. 10 pp. Published in Phys.Scripta T15 (1987) 151, DOI: 10.1088/0031-8949/1987/T15/020
- Lectures On Quantum Cosmology. S.W. Hawking (Cambridge U.). 1986. Published in In *Kyoto 1985, Proceedings, Quantum Gravity and Cosmology*, 170-206
- Lectures On Quantum Cosmology S.W. Hawking (Cambridge U.). 1986.
Published in In *De Vega, H.j. ( Ed.), Sanchez, N. ( Ed.): Field Theory, Quantum Gravity and Strings*, 1-45
- Who's Afraid Of (higher Derivative) Ghosts?. S.W. Hawking (Cambridge U.). Print-86-0124 (CAMBRIDGE). Sep 1985. 16 pp. Published in IN *BATALIN, I.A. (ED.) ET AL.: QUANTUM FIELD THEORY AND QUANTUM STATISTICS, VOL. 2*, 129-139
- Operator Ordering and the Flatness of the Universe. S.W. Hawking (Cambridge U.), Don N. Page (Penn State U.). PRINT-85-0503 (PENN-STATE). Apr 1985. 21 pp. Published in Nucl.Phys. B264 (1986) 185-196, DOI: 10.1016/0550-3213(86)90478-5
- The Arrow Of Time In Cosmology. S.W. Hawking (Cambridge U.). Print-85-0492 (CAMBRIDGE). Apr 1985.23 pp. Published in Phys.Rev. D32 (1985) 2489, DOI: 10.1103/PhysRevD.32.2489
- Quantum Cosmology - Beyond Minisuperspace. J. Halliwell, S. Hawking (Cambridge U.). 1985. Published in In *Rome 1985, Proceedings, General Relativity, Pt. A*, 65-83
- The Quantum Mechanics Of The Universe. S.W. Hawking (Cambridge U.). 1985. Published in In *Geneva 1983, Proceedings, Large-scale Structure Of The Universe, Cosmology and Fundamental Physics*, 415-422
- The Origin of Structure in the Universe. J.J. Halliwell, S.W. Hawking (Cambridge U. & Munich, Max Planck Inst.). Print-85-0265 (CAMBRIDGE). Oct 1984. 48 pp. Published in Phys.Rev. D31 (1985) 1777, DOI: 10.1103/PhysRevD.31.1777
- Limits On Inflationary Models Of The Universe. S.W. Hawking (Cambridge U.). Print-85-0067 (CAMBRIDGE). Sep 1984. 8 pp. Published in Phys.Lett. B150 (1985) 339, DOI: 10.1016/0370-2693(85)90989-X
- Higher Derivatives In Quantum Cosmology. 1. The Isotropic Case. S.W. Hawking, J.C. Luttrell (Cambridge U.). Print-84-0711 (CAMBRIDGE). Aug 1984. 16 pp. Published in Nucl.Phys. B247 (1984) 250, DOI: 10.1016/0550-3213(84)90380-8
- Nontrivial Topologies In Quantum Gravity. S.W. Hawking (Cambridge U.). Print-84-0714 (CAMBRIDGE). Aug 1984. 16 pp. Published in Nucl.Phys. B244 (1984) 135, DOI: 10.1016/0550-3213(84)90185-8
- Numerical Calculations Of Minisuperspace Cosmological Models. S.W. Hawking, Z.C. Wu (Cambridge U.). Print-84-0913 (CAMBRIDGE). Jul 1984. 18 pp. Published in Phys.Lett. B151 (1985) 15, DOI: 10.1016/0370-2693(85)90815-9
- The Isotropy Of The Universe. Stephen W. Hawking, Julian C. Luttrell (Cambridge U.). Print-84-0479 (CAMBRIDGE). Jun 1984. 8 pp. Published in Phys.Lett. B143 (1984) 83, DOI: 10.1016/0370-2693(84)90809-8
- The Cosmological Constant Is Probably Zero. S.W. Hawking (Cambridge U.).Print-84-0116 (CAMBRIDGE). Feb 1984. 5 pp. Published in Phys.Lett. B134 (1984) 403, DOI: 10.1016/0370-2693(84)91370-4
- Quantum Fluctuations As The Cause Of Inhomogeneity In The Universe. J. Halliwell, S.W. Hawking (Cambridge U.). 1984. Published in In *Moscow 1984, Proceedings, Quantum Gravity*, 509-565
- The Very Early Universe. Proceedings, Nuffield Workshop, Cambridge, Uk, June 21 - July 9, 1982. G.W. Gibbons, (Ed.), S.W. Hawking, (Ed.), S.T.C. Siklos, (Ed.). 1984. Published in Cambridge, Uk: Univ. Pr. ( 1983) 480p
- The Quantum State of the Universe. S.W. Hawking (Cambridge U.). PRINT-84-0117 (CAMBRIDGE). Nov 1983. 28 pp. Published in Nucl.Phys. B239 (1984) 257, DOI: 10.1016/0550-3213(84)90093-2
- The Unification Of Physics. S.W. Hawking (Cambridge U.). Print-84-0115 (CAMBRIDGE). Aug 1983. 10 pp.
- Wave Function of the Universe. J.B.
Hartle (Chicago U., EFI& Santa Barbara, KITP), S.W. Hawking
(Cambridge U. & Santa Barbara, KITP). PRINT-83-0937 (CAMBRIDGE).
Jul 983. 46 pp. Published in Phys.Rev. D28 (1983) 2960-2975, DOI: 10.1103/PhysRevD.28.2960
- Quantum Cosmology. S.W. Hawking (Cambridge U.). PRINT-84-0114 (CAMBRIDGE), C83-06-27.1. Jul 1983. 64 pp. Published
in In *Les Houches 1983, Proceedings, Relativity, Groups and Topology,
Ii*, 333-379 and Preprint - HAWKING, S.W. (83,REC.DEC.) 64p
- Euclidean Approach To The Inflationary Universe. S.W. Hawking (Cambridge U.). Print-83-0318 (CAMBRIDGE). Apr 1983. 10 pp. Published in In *Cambridge 1982, Proceedings, The Very Early Universe*, 287-296 and Preprint -HAWKING, S.W. (REC.APR.83) 12p
- The Boundary Conditions For Gauged Supergravity. S.W. Hawking (Cambridge U.). Print-83-0317 (CAMBRIDGE). Mar 1983. 11 pp. Published in Phys.Lett. B126 (1983) 175, DOI: 10.1016/0370-2693(83)90585-3
- Fluctuations In The Inflationary Universe. S.W. Hawking (Cambridge U.), I.G. Moss (Newcastle upon Tyne U.). PRINT-83-0316 (CAMBRIDGE). Dec 1982. 20 pp. Published in Nucl.Phys. B224 (1983) 180, DOI: 10.1016/0550-3213(83)90319-X
- Thermodynamics of Black Holes in anti-De Sitter Space. S.W. Hawking (Cambridge U.), Don N. Page (Penn State U.). PRINT-83-0019 (CAMBRIDGE). Jul 1982. 18 pp.Published in Commun.Math.Phys. 87 (1983) 577, DOI: 10.1007/BF01208266
- Positive Mass Theorems For Black Holes. G.W.
Gibbons, S.W. Hawking (Cambridge U.), Gary T. Horowitz (Princeton,
Inst. Advanced Study), Malcolm J. Perry (Princeton U.). Print-82-0505
(PRINCETON). Jul 1982. 25 pp. Published in Commun.Math.Phys. 88 (1983) 295, DOI: 10.1007/BF01213209
- The Development of Irregularities in a Single Bubble Inflationary Universe. S.W. Hawking (Cambridge U.). Print-83-0015 (CAMBRIDGE). Jun 1982. 8 pp. Published in Phys.Lett. B115 (1982) 295, DOI: 10.1016/0370-2693(82)90373-2
- The Unpredictability of Quantum Gravity. S.W. Hawking (Cambridge U.). Print-83-0017 (CAMBRIDGE). May 1982. 29 pp. Published in Commun.Math.Phys. 87 (1982) 395-415, DOI: 10.1007/BF01206031
- Bubble Collisions in the Very Early Universe. S.W. Hawking, I.G. Moss, J.M. Stewart (Cambridge U.). Print-82-0180 (CAMBRIDGE). Mar 1982. 33 pp. Published in Phys.Rev. D26 (1982) 2681, DOI: 10.1103/PhysRevD.26.2681
- Supercooled Phase Transitions in the Very Early Universe. S.W. Hawking, I.G. Moss (Cambridge U.). Print-82-0181 (CAMBRIDGE). Dec 1981. 9 pp. Published in Phys.Lett. B110 (1982) 35, DOI: 10.1016/0370-2693(82)90946-7
- The Boundary Conditions Of The Universe. S.W. Hawking (Cambridge U.). PRINT-82-0179 (CAMBRIDGE). Sep 1981. 11 pp. Published in Pontif.Acad.Sci.Scrivaria 48 (1982) 563-574
- The Cosmological Constant And The Weak Anthropic Principle. S.W. Hawking (Cambridge U.). Print-82-0177 (CAMBRIDGE). Aug 1981. 9 pp. Published in In *London 1981, Proceedings, Quantum Structure Of Space and Time*, 423-432
- Is The End In Sight For Theoretical Physics?. S.W. Hawking (Cambridge U.). PRINT-81-0004 (CAMBRIDGE). Jan 1981. 17 pp. Published in Phys.Bull. 32 (1981) 15-17
- The Loss Of Quantum Coherence Due To Virtual Black Holes. S.W. Hawking (Cambridge U.). 1981. Published in In *Moscow 1981, Proceedings, Quantum Gravity*, 19-28
- Why Is The Apparent Cosmological Constant Zero? (talk). S.W. Hawking (Cambridge U.). 1981. Published in In *Muenchen 1981, Proceedings, Unified Theories Of Elementary Particles*, 167-175
- Superspace And Supergravity. Proceedings, Nuffield Workshop, Cambridge, Uk, June 16 - July 12, 1980. S.W. Hawking, (ed.), M. Rocek, (ed.). 1981. Published in Cambridge, Uk: Univ. Pr. ( 1981) 527p
- Interacting Quantum Fields Around A Black Hole. S.W. Hawking (Cambridge U.). Print-81-0251 (CAMBRIDGE). Dec 1980. 40 pp. Published in Commun.Math.Phys. 80 (1981) 421, DOI: 10.1007/BF01208279
- Acausal Propagation In Quantum Gravity. S.W. Hawking (Cambridge U.). PRINT-80-0866 (CAMBRIDGE), C80-04-15. Apr 1980. 22 pp. Published in In *Oxford 1980, Proceedings, Quantum Gravity 2*, 393-415
- The Path Integral Approach To Quantum Gravity. S.W. Hawking (Cambridge U.). 1980. Published in In *Hawking, S.W., Israel, W.: General Relativity*, 746-789
- Introductory Survey. S.W. Hawking (Cambridge U.), W. Israel (Alberta U.). 1980. Published in In *Hawking, S.W., Israel, W.: General Relativity*, 1-23
- Quantum Gravitational Bubbles. S.W. Hawking, Don N. Page, C.N. Pope (Cambridge U.). Print-80-0053 (CAMBRIDGE). Oct 1979. 33 pp. Published in Nucl.Phys. B170 (1980) 283-306, DOI: 10.1016/0550-3213(80)90151-0
- Yang-mills Instantons And The S Matrix. S.W. Hawking, C.N. Pope (Cambridge U.). Print-79-0654 (CAMBRIDGE). Apr 1979. 32 pp. Published in Nucl.Phys. B161 (1979) 93, DOI: 10.1016/0550-3213(79)90128-7
- Space-Time Foam. S.W. Hawking (Cambridge U.). Print-79-0038 (CAMBRIDGE). Jan 1979. 24 pp. Published in Nucl.Phys. B144 (1978) 349-362, DOI: 10.1016/0550-3213(78)90375-9
- Gravitational Multi – Instantons. G.W. Gibbons, S.W. Hawking (Cambridge U.). Print-79-0042 (CAMBRIDGE). Jan 1979. 6 pp. Published in Phys.Lett. B78 (1978) 430, DOI: 10.1016/0370-2693(78)90478-1
- Symmetry Breaking By Instantons In Supergravity. S.W. Hawking, C.N. Pope (Cambridge U.). Print-79-0043 (CAMBRIDGE). Jan 1979. 22 pp. Published in Nucl.Phys. B146 (1978) 381, DOI: 10.1016/0550-3213(78)90073-1
- The Propagation Of Particles In Space-time Foam. S.W. Hawking, Don N. Page, C.N. Pope (Cambridge U.). 1979. Published in Phys.Lett. B86 (1979) 175-178, DOI: 10.1016/0370-2693(79)90812-8
- Classification of Gravitational Instanton Symmetries. G.W. Gibbons, S.W. Hawking (Cambridge U.). 1979. Published in Commun.Math.Phys. 66 (1979) 291-310, DOI: 10.1007/BF01197189
- Relativity Today. S. Hawking (Cambridge U.), W. Israel (Alberta U.). 1979. Published in New Sci. 81 (1979) 761-763
- General Relativity. An Einstein Centenary Survey Pt 1. S.W. Hawking (Cambridge U.), W. Israel (Alberta U.). 1979. Published in Cambridge, United Kingdom: Univ.Pr.(1979) 919p
- Theoretical Advances In General Relativity. S.W. Hawking (Cambridge U.). Print-79-0595 (CAMBRIDGE). Nov 1978. 16 pp.
- Euclidean Quantum Gravity. Stephen W. Hawking (Cambridge U.). PRINT-78-0745 (CAMBRIDGE), C78-07-10.1-2. Jul 1978. 30 pp. Published in NATO Adv.Study Inst.Ser.B Phys. 44 (1979) 145
- Path Integrals and the Indefiniteness of the Gravitational Action. G.W.
Gibbons (Munich, Max Planck Inst. & Cambridge U.), S.W. Hawking,
M.J. Perry (Cambridge U.). PRINT-78-0375 (CAMBRIDGE). Apr 1978. 14 pp. Published in Nucl.Phys. B138 (1978) 141, DOI: 10.1016/0550-3213(78)90161-X
- Quantum Gravity and Path Integrals. S.W. Hawking (Cambridge U. & Caltech). 1978. Published in Phys.Rev. D18 (1978) 1747-1753, DOI: 10.1103/PhysRevD.18.1747
- Generalized Spin Structures in Quantum Gravity. S.W.
Hawking, C.N. Pope (Cambridge U.). Print-78-0374 (CAMBRIDGE). Nov
1977. 6 pp. Published in Phys.Lett. B73 (1978) 42-44, DOI: 10.1016/0370-2693(78)90167-3
- Cosmological Event Horizons, Thermodynamics, and Particle Creation. G.W. Gibbons, S.W. Hawking (Cambridge U.). 1977. Published in Phys.Rev. D15 (1977) 2738-2751, DOI: 10.1103/PhysRevD.15.2738
- The Quantum Mechanics of Black Holes. S.W. Hawking. 1977. Published in Sci.Am. 236 (1977) 34-49, DOI: 10.1038/scientificamerican0177-34
- Black Holes and Unpredictability. S.W. Hawking (Cambridge U.). PRINT-77-0292 (CAMBRIDGE). Dec 1976. 6 pp. Published in Phys.Bull. 29 (1978) 23-24
- Gravitational Instantons. S.W. Hawking (Cambridge U.). Print-77-0294 (CAMBRIDGE). Dec 1976. 8 pp. Published in Phys.Lett. A60 (1977) 81, DOI: 10.1016/0375-9601(77)90386-3
- Zeta Function Regularization of Path Integrals in Curved Space-Time. S.W. Hawking (Cambridge U.). PRINT-77-0293 (CAMBRIDGE). Dec 1976. 29 pp. Published in Commun.Math.Phys. 55 (1977) 133, DOI: 10.1007/BF01626516
- Action Integrals and Partition Functions in Quantum Gravity. G.W. Gibbons, S.W. Hawking (Cambridge U.). PRINT-76-0995 (CAMBRIDGE). Sep 1976. 14 pp. Published in Phys.Rev. D15 (1977) 2752-2756, DOI: 10.1103/PhysRevD.15.2752
- Gamma rays from primordial black holes. Don N. Page, S.W. Hawking. May 1976. 7 pp. Published in Astrophys.J. 206 (1976) 1-7, DOI: 10.1086/154350
- Breakdown of Predictability in Gravitational Collapse. S.W. Hawking (Cambridge U. & Caltech). 1976. Published in Phys.Rev. D14 (1976) 2460-2473, DOI: 10.1103/PhysRevD.14.2460
- Path Integral Derivation of Black Hole Radiance. J.B. Hartle, S.W. Hawking (UC, Santa Barbara & Caltech & Cambridge U.). 1976. Published in Phys.Rev. D13 (1976) 2188-2203, DOI: 10.1103/PhysRevD.13.2188
- Black Holes and Thermodynamics. S.W. Hawking (Caltech & Cambridge U.). 1976. Published in Phys.Rev. D13 (1976) 191-197, DOI: 10.1103/PhysRevD.13.191
- A New Topology for Curved Space-Time Which Incorporates the Causal, Differential, and Conformal Structures. S.W. Hawking (Cambridge U. & Caltech), A.R. King, P.J. Mccarthy. 1976. Published in J.Math.Phys. 17 (1976) 174-181, DOI: 10.1063/1.522874
- Particle Creation by Black Holes. S.W. Hawking (Cambridge U.). Aug 1975. 22 pp. Published in Commun.Math.Phys. 43 (1975) 199-220, Erratum-ibid. 46 (1976) 206-206, DOI: 10.1007/BF02345020
- Black hole explosions. S.W. Hawking (Cambridge U.). Mar 1974. 2 pp. Published in Nature 248 (1974) 30-31, DOI: 10.1038/248030a0
- Black holes in the early Universe. Bernard J. Carr, S.W. Hawking (Cambridge U., Inst. of Astron. & Cambridge U., DAMTP). Feb 1974. 17 pp. Published in Mon.Not.Roy.Astron.Soc. 168 (1974) 399-415
- Causally continuous space-times. S.W. Hawking, R.K. Sachs. 1974. Published in Commun.Math.Phys. 35 (1974) 287-296, DOI: 10.1007/BF01646350
- A Variational principle for black holes. S.W. Hawking. 1973. Published in Commun.Math.Phys. 33 (1973) 323-334, DOI: 10.1007/BF01646744
- The Four laws of black hole mechanics. James M. Bardeen (Yale U.), B. Carter, S.W. Hawking (Cambridge U.). 1973. Published in Commun.Math.Phys. 31 (1973) 161-170, DOI: 10.1007/BF01645742
- The Large scale structure of space-time. S.W. Hawking, G.F.R. Ellis. 1973. 391 pp. Published in Cambridge University Press, Cambridge, 1973. ISBN-13: 978-0521099066
- The rotation and distortion of the universe. C.B. Collins, S.W. Hawking. Jan 1973, Published in Mon.Not.Roy.Astron.Soc. 162 (1973) 307-320
- Why is the Universe isotropic?. C.B. Collins, S.W. Hawking (Cambridge U., DAMTP & Cambridge U.). Sep 1972. 18 pp. Published in Astrophys.J. 180 (1973) 317-334, DOI: 10.1086/151965
- Solutions of the Einstein-Maxwell equations with many black holes. J.B. Hartle, S.W. Hawking. Jun 1972. Published in Commun.Math.Phys. 26 (1972) 87-101, DOI: 10.1007/BF01645696
- Energy and angular momentum flow into a black hole. S.W. Hawking (Cambridge U., DAMTP), J.B. Hartle (UC, Santa Barbara). 1972. Published in Commun.Math.Phys. 27 (1972) 283-290, DOI: 10.1007/BF01645515
- Gravitational radiation - the theoretical aspect. S.W. Hawking (Cambridge U., DAMTP). 1972. Published in Contemp.Phys. 13 (1972) 273-282, DOI: 10.1080/00107517208205681
- Black holes in the Brans-Dicke theory of gravitation. S.W. Hawking (Cambridge U.). 1972. Published in Commun.Math.Phys. 25 (1972) 167-171, DOI: 10.1007/BF01877518
- Theory of the detection of short bursts of gravitational radiation. G.W. Gibbons, S.W. Hawking (Cambridge U., DAMTP). 1972. Published in Phys.Rev. D4 (1971) 2191-2197, DOI: 10.1103/PhysRevD.4.2191
- Black holes in general relativity. S.W. Hawking (Cambridge U.). Oct 1971. Published in Commun.Math.Phys. 25 (1972) 152-166, DOI: 10.1007/BF01877517
- Gravitational radiation from colliding black holes. S.W. Hawking (Cambridge U.). Mar 1971. Published in Phys.Rev.Lett. 26 (1971) 1344-1346, DOI: 10.1103/PhysRevLett.26.1344
- Evidence for black holes in binary star systems. S.W. Hawking, G.W. Gibbons. 1971. Published in Nature 232 (1971) 465, DOI: 10.1038/232465a0
- The Definition and occurrence of singularities in general relativity. Stephen Hawking. 1971. Published in Lect.Notes Math. 209 (1971) 275-279
- Stable and generic properties in general relativity. Stephen Hawking (Cambridge U., Inst. of Astron.). 1971. Published in Gen.Rel.Grav. 1 (1971) 393-400, DOI: 10.1007/BF00759218
- Gravitationally collapsed objects of very low mass. Stephen Hawking. 1971. Published in Mon.Not.Roy.Astron.Soc. 152 (1971) 75
- The Singularities of gravitational collapse and cosmology. S.W. Hawking (Cambridge U.), R. Penrose (Birkbeck Coll.). Jan 1970. 20 pp. Published in Proc.Roy.Soc.Lond. A314 (1970) 529-548, DOI: 10.1098/rspa.1970.0021
- The conservation of matter in general relativity. S. Hawking (Cambridge U., DAMTP). 1970. Published in Commun.Math.Phys. 18 (1970) 301-306, DOI: 10.1007/BF01649448
- Singularities in collapsing stars and universes. Stephen Hawking, Dennis Sciama. 1969. Published in Comments Astrophys. Space Phys. 1 (1969) 1
- On the Rotation of the universe. S.W. Hawking (Cambridge U., Inst. of Astron.). Sep 1968. 13 pp. Published in Mon.Not.Roy.Astron.Soc. 142 (1969) 129-141
- Gravitational radiation in an expanding universe. Stephen Hawking (Cambridge U., DAMTP). Apr 1968. Published in J.Math.Phys. 9 (1968) 598-604, DOI: 10.1063/1.1664615
- The Cosmic black body radiation and the existence of singularities in our universe. G.F.R. Ellis, Stephen Hawking. 1968. Published in Astrophys.J. 152 (1968) 25, DOI: 10.1086/149520
- The Existence of cosmic time functions. Stephen Hawking (Cambridge U., DAMTP). 1968. Published in Proc.Roy.Soc.Lond. A308 (1968) 433-435
- The occurrence of singularities in cosmology. III. Causality and singularities. Stephen Hawking (Cambridge U., DAMTP). 1967. Published in Proc.Roy.Soc.Lond. A300 (1967) 187-201, DOI: 10.1098/rspa.1967.0164
- Perturbations of an expanding universe. S.W. Hawking (Cambridge U., DAMTP). Feb 1966. 11 pp. Published in Astrophys.J. 145 (1966) 544-554, DOI: 10.1086/148793
- Singularities in the universe. S.W. Hawking. 1966. Published in Phys.Rev.Lett. 17 (1966) 444-445, DOI: 10.1103/PhysRevLett.17.444
- Helium production in anisotropic big bang universes. Stephen Hawking, J.R. Tayler (Cambridge U., DAMTP). 1966. Published in Nature 209 (1966) 1278-1279, DOI: 10.1038/2091278a0
- The Occurrence of singularities in cosmology. Stephen Hawking (Cambridge U., DAMTP). 1966. Published in Proc.Roy.Soc.Lond. A294 (1966) 511-521, DOI: 10.1098/rspa.1966.0221
- The Occurrence of singularities in cosmology. II. Stephen Hawking (Cambridge U., DAMTP). 1966. Published in Proc.Roy.Soc.Lond. A295 (1966) 490-493, DOI: 10.1098/rspa.1966.0255
- Singularities and the geometry of space-time. Stephen Hawking. 1966.
- Singularities in homogeneous world models. Stephen Hawking, G.F.R. Ellis (Cambridge U., DAMTP & Cambridge U.). Jun 1965. Published in Phys.Lett. 17 (1965) 246-247, DOI: 10.1016/0031-9163(65)90510-X
- On the Hoyle-Narlikar theory of gravitation. Stephen Hawking (Cambridge U., DAMTP). Feb 1965. Published in Proc.Roy.Soc.Lond. A286 (1965) 313-319, DOI: 10.1098/rspa.1965.0146
- Occurrence of singularities in open universes. Stephen Hawking (Cambridge U., DAMTP). 1965. Published in Phys.Rev. ett. 15 (1965) 689-690, DOI: 10.1103/PhysRevLett.15.689
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