Hawking Radiation explained by Himself. (Subs en castellano)
The great astrophysicist Stephen Hawking explains his wonderful theories about black holes, in a movie that's a jewel. It's the movie: "A brief history of time", since I had the book, years ago, I struggled to get the full movie... and... I finally got it! :)
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Aharonov-Bohm Effect and Hawking Radiation
Lecturer: Ulf Leonhardt "50 years of the Aharonov-Bohm Effect", An international convention held at the Tel Aviv University, 11-14.10.09
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Funckarma - Hawking Radiation [HQ]
more@ disphunktional.blogspot.com TRACKLISTING : 1. Hawking Radiation 2. Moor 3. Solaz Flair (Digital Only) 4. Delibel 5. Sovtron 6. Nays of Dight - Herrmutt Lobby Remix - (Digital Only)* www.funckarma.com www.myspace.com/funckarma
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Hawking Radiation
See more clips at worldsciencefestival.com Remember that bet Stephen Hawking made with Kip Thorne in the 90s about whether information could escape a black hole? (No, not the infamous one wagered between the two physicists in the 70s involving a subscription to Penthouse.) The stakes for this bet were much tamer: an encyclopedia collection of the winner's choosing. The debate was over the behavior of Hawking radiation, the black hole information paradox, and whether the conservation of energy can be violated at the event horizon of a black hole. But before you can even begin to wrap you head around all of that, you must first understand what Hawking radiation is. Here, Kip Thorne—in front of Stephen Hawking himself, 2010 Festival honoree—provides expert analysis of the strange phenomenon.
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Stephen Hawking on CNN [NEW] ستيفن هوكينغ
Translated to arabic by: www.youtube.com Stephen William Hawking, CH, CBE, FRS, FRSA (born 8 January 1942) is a British theoretical physicist and cosmologist, whose scientific career spans over forty years. His books and public appearances have made him an academic celebrity and he is an Honorary Fellow of the Royal Society of Arts, a lifetime member of the Pontifical Academy of Sciences, and in 2009 was awarded the Presidential Medal of Freedom, the highest civilian award in the United States. Hawking was the Lucasian Professor of Mathematics at the University of Cambridge for thirty years, taking up the post in 1979 and retiring on 1 October 2009. He is also a Fellow of Gonville and Caius College, Cambridge and a Distinguished Research Chair at the Perimeter Institute for Theoretical Physics in Waterloo, Ontario. He is known for his contributions to the fields of cosmology and quantum gravity, especially in the context of black holes. He has also achieved success with works of popular science in which he discusses his own theories and cosmology in general; these include the runaway best seller A Brief History of Time, which stayed on the British Sunday Times bestsellers list for a record-breaking 237 weeks. Hawking's key scientific works to date have included providing, with Roger Penrose, theorems regarding gravitational singularities in the framework of general relativity, and the theoretical prediction that black holes should emit radiation, which is today known as <b>...</b>
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Q-Stephen Hawking Master Part 1
Stephen William Hawking, CH, CBE, FRS, FRSA (born 8 January 1942[1]) is a British theoretical physicist, whose world-renowned scientific career spans over 40 years. His books and public appearances have made him an academic celebrity and he is an Honorary Fellow of the Royal Society of Arts,[2] a lifetime member of the Pontifical Academy of Sciences,[3] and in 2009 was awarded the Presidential Medal of Freedom, the highest civilian award in the United States.[4] Hawking was the Lucasian Professor of Mathematics at the University of Cambridge for thirty years, taking up the post in 1979 and retiring on 1 October 2009.[5][6] He is also a Fellow of Gonville and Caius College, Cambridge and a Distinguished Research Chair at the Perimeter Institute for Theoretical Physics in Waterloo, Ontario.[7] He is known for his contributions to the fields of cosmology and quantum gravity, especially in the context of black holes. He has also achieved success with works of popular science in which he discusses his own theories and cosmology in general; these include the runaway best seller A Brief History of Time, which stayed on the British Sunday Times bestsellers list for a record-breaking 237 weeks.[8][9] Hawking's key scientific works to date have included providing, with Roger Penrose, theorems regarding singularities in the framework of general relativity, and the theoretical prediction that black holes should emit radiation, which is today known as Hawking radiation (or sometimes <b>...</b>
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Pt 7 of 8 The Story of Everything By Stephen Hawking.
Stephen William Hawking, CH, CBE, FRS, FRSA (born 8 January 1942) is a British theoretical physicist and cosmologist, whose scientific career spans over forty years. His books and public appearances have made him an academic celebrity and he is an Honorary Fellow of the Royal Society of Arts, a lifetime member of the Pontifical Academy of Sciences, and in 2009 was awarded the Presidential Medal of Freedom, the highest civilian award in the United States. Hawking was the Lucasian Professor of Mathematics at the University of Cambridge for thirty years, taking up the post in 1979 and retiring on 1 October 2009. He is also a Fellow of Gonville and Caius College, Cambridge and a Distinguished Research Chair at the Perimeter Institute for Theoretical Physics in Waterloo, Ontario. He is known for his contributions to the fields of cosmology and quantum gravity, especially in the context of black holes. He has also achieved success with works of popular science in which he discusses his own theories and cosmology in general; these include the runaway best seller A Brief History of Time, which stayed on the British Sunday Times bestsellers list for a record-breaking 237 weeks. Hawking's key scientific works to date have included providing, with Roger Penrose, theorems regarding gravitational singularities in the framework of general relativity, and the theoretical prediction that black holes should emit radiation, which is today known as Hawking radiation (or sometimes as <b>...</b>
Stephen Hawking Universe Portal Black Worm Hole Planets Stars Space Ships Crafts Rockets Solar System Cosmos World Earth Big Bang Atoms Sun Star Gravity Milky Way Jupiter Saturn Venus Mars Mercury Moon Astroid WR104 Orbit Super Nova Gamma Radiation Rays Science Mission Tunnel Stargate Past Future Paradox Satellight Apollo 11 TV Channel Lindasufos
Q-Stephen Hawking master Part 2
Stephen William Hawking, CH, CBE, FRS, FRSA (born 8 January 1942[1]) is a British theoretical physicist, whose world-renowned scientific career spans over 40 years. His books and public appearances have made him an academic celebrity and he is an Honorary Fellow of the Royal Society of Arts,[2] a lifetime member of the Pontifical Academy of Sciences,[3] and in 2009 was awarded the Presidential Medal of Freedom, the highest civilian award in the United States.[4] Hawking was the Lucasian Professor of Mathematics at the University of Cambridge for thirty years, taking up the post in 1979 and retiring on 1 October 2009.[5][6] He is also a Fellow of Gonville and Caius College, Cambridge and a Distinguished Research Chair at the Perimeter Institute for Theoretical Physics in Waterloo, Ontario.[7] He is known for his contributions to the fields of cosmology and quantum gravity, especially in the context of black holes. He has also achieved success with works of popular science in which he discusses his own theories and cosmology in general; these include the runaway best seller A Brief History of Time, which stayed on the British Sunday Times bestsellers list for a record-breaking 237 weeks.[8][9] Hawking's key scientific works to date have included providing, with Roger Penrose, theorems regarding singularities in the framework of general relativity, and the theoretical prediction that black holes should emit radiation, which is today known as Hawking radiation (or sometimes <b>...</b>
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Pt 8 of 8 The Story of Everything By Stephen Hawking.
Stephen William Hawking, CH, CBE, FRS, FRSA (born 8 January 1942) is a British theoretical physicist and cosmologist, whose scientific career spans over forty years. His books and public appearances have made him an academic celebrity and he is an Honorary Fellow of the Royal Society of Arts, a lifetime member of the Pontifical Academy of Sciences, and in 2009 was awarded the Presidential Medal of Freedom, the highest civilian award in the United States. Hawking was the Lucasian Professor of Mathematics at the University of Cambridge for thirty years, taking up the post in 1979 and retiring on 1 October 2009. He is also a Fellow of Gonville and Caius College, Cambridge and a Distinguished Research Chair at the Perimeter Institute for Theoretical Physics in Waterloo, Ontario. He is known for his contributions to the fields of cosmology and quantum gravity, especially in the context of black holes. He has also achieved success with works of popular science in which he discusses his own theories and cosmology in general; these include the runaway best seller A Brief History of Time, which stayed on the British Sunday Times bestsellers list for a record-breaking 237 weeks. Hawking's key scientific works to date have included providing, with Roger Penrose, theorems regarding gravitational singularities in the framework of general relativity, and the theoretical prediction that black holes should emit radiation, which is today known as Hawking radiation (or sometimes as <b>...</b>
Stephen Hawking Universe Portal Black Worm Hole Planets Stars Space Ships Crafts Rockets Solar System Cosmos World Earth Big Bang Atoms Sun Star Gravity Milky Way Jupiter Saturn Venus Mars Mercury Moon Astroid WR104 Orbit Super Nova Gamma Radiation Rays Science Mission Tunnel Stargate Past Future Paradox Satellight Apollo 11 TV Channel Lindasufos
Into the Universe - The Story of Everything p4
Stephen William Hawking, CH, CBE, FRS, FRSA (born 8 January 1942) is a British theoretical physicist and cosmologist, whose scientific career spans over forty years. His books and public appearances have made him an academic celebrity and he is an Honorary Fellow of the Royal Society of Arts, a lifetime member of the Pontifical Academy of Sciences, and in 2009 was awarded the Presidential Medal of Freedom, the highest civilian award in the United States. Hawking was the Lucasian Professor of Mathematics at the University of Cambridge for thirty years, taking up the post in 1979 and retiring on 1 October 2009. He is also a Fellow of Gonville and Caius College, Cambridge and a Distinguished Research Chair at the Perimeter Institute for Theoretical Physics in Waterloo, Ontario. He is known for his contributions to the fields of cosmology and quantum gravity, especially in the context of black holes. He has also achieved success with works of popular science in which he discusses his own theories and cosmology in general; these include the runaway best seller A Brief History of Time, which stayed on the British Sunday Times bestsellers list for a record-breaking 237 weeks. Hawking's key scientific works to date have included providing, with Roger Penrose, theorems regarding gravitational singularities in the framework of general relativity, and the theoretical prediction that black holes should emit radiation, which is today known as Hawking radiation (or sometimes as <b>...</b>
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Eminence - Hawking Radiation & Stainer (Live, Belo Horizonte, Brazil 20.05.2011)
Eminence performing Hawking Radiation & Stainer. Concert recorded at Lapa Multshow in Belo Horizonte, Brazil. Eminence no Conexão Vivo 2011. www.eminence.com.br
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10 Questions for Stephen Hawking
The renowned physicist has a new book, "The Grand Design." Stephen Hawking will now take your questions.
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Stephen Hawking's Universe. Episode 2 - Cosmic Microwave Background Radiation
Edwin Hubble has made his measurements and Albert Einstein has conceded to the idea of the expansion of the universe but debate still continues between Big Bang proponents and supporters of a steady state model of the Universe. Lesson P1b 7.2 of the UK AQA syllabus.
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Interview Edgar Fouche: Area 51 Aurora and Alien UFO tech
[reissued] For 16 years, Aviation Week & Space Technology has investigated myriad sightings of a two-stage-to-orbit system that could place a small military spaceplane in orbit. Considerable evidence supports the existence of such a highly classified system, . . . that. . . US intelligence agencies may have quietly mothballed a highly classified two-stage-to-orbit spaceplane system designed in the 1980s for reconnaissance, satellite-insertion and, possibly, weapons delivery. It could be a victim of shrinking federal budgets strained by war costs, or it may not have met performance or operational goals. . . . A large "mothership," closely resembling the US Air Force's historic XB-70 supersonic bomber (note from the editor: now succeeded by the SR-75 Penetrator), carries the orbital component conformally under its fuselage, accelerating to supersonic speeds at high altitude before dropping the spaceplane. The orbiter's engines fire and boost the vehicle into space. If mission requirements dictate, the spaceplane can either reach low Earth orbit or remain suborbital. THE REAL STORY - WELL ONE OF THE REASONS WHY THE BLACKSTAR SYSTEM HAS BEEN MOTHBALLED is because it is no longer needed since other R&D projects have bornesome very ripe fruit ready to be pickedfor operational duty. Introducing the TR3b Astra Space Plane (not my designation. . . it's an aviation folklore designation) using principles firstexplored by Townsend Brown and Nicola Tesla. The basic principle is as <b>...</b>
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Large Hadron Collider Black Hole
Stop the LHC! The consequences of collisions at the Large Hadron Collider were studied by the LHC Safety Study Group. "The LHC reproduces in the laboratory, under controlled conditions, collisions at centre-of-mass energies less than those reached in the atmosphere by some of the cosmic rays, that have been bombarding the Earth for billions of years. We recall the rates for the collisions of cosmic rays with astronomical bodies at energies higher than the LHC. The stability of astronomical bodies indicates that such collisions cannot be dangerous." lsag.web.cern.ch Incorrect analogy. They compare two completely different types of conditions! The First. Natural cosmic rays in the atmosphere. The Second. Collisions inside the artificial device. Under the surface of the Earth. Cosmic rays are balanced in such a way that probability of artificial anomaly is almost zero. In other words, cosmic rays represent natural conditions that existed during billions of years, and therefore they are safe. Collisions inside the LHC can't be compared with natural cosmic rays. Large Hadron Collider is an artificial device created by man. There's no similar devices in the sky or on astronomical bodies. So, we have no sufficient basis for correct analogy to tell whether the experiment is dangerous or not. Collisions inside the artificial device under the surface of the Earth may be unbalanced. Probability of anomaly inside the LHC may be very high. And scientists do not know how such possible <b>...</b>
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Black Holes at the Large Hadron Collider - Prof Elizabeth Winstanley at ANU
We may think we live in a 3D world, but the latest advances in theoretical physics suggest we may occupy just a small slice of reality with many more dimensions. One consequence of these theories is that huge amounts of mini black holes may be formed by collisions at the Large Hadron Collider (LHC) at the European Organization for Nuclear Research (CERN). In this talk, Professor Elizabeth Winstanley will describe how these mini black holes are created, and what happens to them once they have been produced. In particular, she will discuss why these black holes will not swallow up the entire Earth. Professor Winstanley studied undergraduate mathematics at St Hugh's College, Oxford University. She then continued to study a PhD in theoretical physics at Oxford University. After her doctoral studies, she was appointed as Fellow and Lecturer in Applied Mathematics at Oriel College, Oxford University, teaching a wide range of mathematics and theoretical physics courses. In September 2000, she was appointed as a Lecturer in the Department of Applied Mathematics at the University of Sheffield, where she has worked ever since. She was promoted to Professor of Mathematical Physics in January 2009. Professor Winstanley's research interests include general relativity, quantum gravity and quantum field theory in curved space-time. Her research focuses on the physics of black holes, particularly black holes in general relativity and the Hawking radiation of black holes as might be <b>...</b>
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BBC Horizon 2005: 2/7 The Hawking Paradox
Hawking and his fellow physicist embarked on an extraordinary intellectual expedition - to tame the black hole. The period from the early 70s to the early 80s became known as the "Golden Age" of black hole research. Slowly physicists were coming to understand its nature. But Hawking realised that there was something missing from the picture that was emerging. All work on black holes to that point used the physics of the large-scale Universe. The physics of gravity - first developed by Newton and then refined by Einstein's general theory of relativity. Hawking realised that to come to a full understanding of black holes, physicists would also have to use the physics of the small-scale Universe; the physics that had been developed to explain the movements of atoms and sub-atomic particles known as quantum mechanics. The only problem was that no one had ever combined these two areas of physics before. This didn't deter Hawking. He set about developing a new way to force the physics of quantum mechanics to co-exist with Einstein's relativity within the intense gravity of a black hole. After months of work, Hawking came up with a remarkable result. His equations were showing him that something was coming out of the black hole. This was supposed to be impossible - the one thing that everyone thought they knew about black holes was that things went in but nothing, not even light itself, could escape. The more Hawking checked, the more he was convinced he was right. He could see <b>...</b>
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Stephen Hawking - Campus Party speech (2006)
Prof Stephen Hawking speech to Campus Party 2006 Hawking's principal fields of research are theoretical cosmology and quantum gravity. In 1971, in collaboration with Sir Roger Penrose, he proved the first of many singularity theorems; such theorems provide a set of sufficient conditions for the existence of a singularity in space-time. This work showed that, far from being mathematical curiosities which appear only in special cases, singularities are a fairly generic feature of general relativity. Hawking also suggested that, after the Big Bang, primordial or mini black holes were formed. With Bardeen and Carter, he proposed the four Laws of black hole mechanics, drawing an analogy with thermodynamics. In 1974, he calculated that black holes should thermally create and emit subatomic particles, known as Hawking radiation, until they exhaust their energy and evaporate. In collaboration with Jim Hartle, Hawking developed a model in which the Universe had no boundary in space-time, replacing the initial singularity of the classical Big Bang models with a region akin to the North pole; while one cannot travel North of the North pole, there is no boundary there. While originally the no-boundary proposal predicted a closed Universe, discussions with Neil Turok led to the realization that the no-boundary proposal is consistent with a Universe which is not closed also.
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Virtual Force Theory 2|Energy Source
The energy source for the Virtual Force is explored as the source for the four general forces of physics and the two special forces, Dark Matter and Dark Energy. The Hawking Radiation Theory is compared as both theories depend upon virtual particles producing energy.
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Stephen Hawking on Science in the 21st Century - Part 3 (1998)
March 6, 1998 www.amazon.com Watch the full program: thefilmarchived.blogspot.com Almost as soon as he arrived at Cambridge, he started developing symptoms of amyotrophic lateral sclerosis (ALS, known colloquially in the United States as Lou Gehrig's disease), a type of motor neuron disease which would cost him almost all neuromuscular control. During his first two years at Cambridge, he did not distinguish himself, but, after the disease had stabilised and with the help of his doctoral tutor, Dennis William Sciama, he returned to working on his Ph.D. Hawking was elected as one of the youngest Fellows of the Royal Society in 1974, was created a Commander of the Order of the British Empire in 1982, and became a Companion of Honour in 1989. Hawking is a member of the Board of Sponsors of the Bulletin of the Atomic Scientists. Hawking's achievements were made despite the increasing paralysis caused by the ALS. By 1974, he was unable to feed himself or get out of bed. His speech became slurred so that he could only be understood by people who knew him well. In 1985, he caught pneumonia and had to have a tracheotomy, which made him unable to speak at all. A Cambridge scientist built a device that enables Hawking to write onto a computer with small movements of his body, and then have a voice synthesizer speak what he has typed. Hawking's principal fields of research are theoretical cosmology and quantum gravity. In the late 1960s, he and his Cambridge friend and colleague <b>...</b>
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Conflict of Principles
See more clips at worldsciencefestival.com Stephen Hawking's premise was sound; his math irrefutable. As matter falls into a black hole, quantum events cause it to emit particles. These particles—what became known as Hawking radiation—lead to the eventual evaporation of the black hole, and any information about the matter that fell in would be lost forever. But for physicists Leonard Susskind and Gerard 't Hooft, something didn't sit right. In fact, it seemed to go against the very laws of physics—a contradiction which ultimately led to the radical possibility of the knowable universe as encoded information. They discuss with moderator John Hockenberry the delicate challenges of arguing with a man whose theories were for all intents and purposes "unassailable."
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Darla Dimple's Rampage of Displacement and Volume
A black hole, according to the general theory of relativity, is a region of space from which nothing, including light, can escape. It is the result of the deformation of spacetime caused by a very compact mass. Around a black hole there is an undetectable surface which marks the point of no return, called an event horizon. It is called "black" because it absorbs all the light that hits it, reflecting nothing, just like a perfect black body in thermodynamics.[1] Under the theory of quantum mechanics, black holes possess a temperature and emit Hawking radiation, but for black holes of stellar mass or larger this temperature is much lower than that of the cosmic background radiation. Despite its invisible interior, a black hole can be observed through its interaction with other matter. A black hole can be inferred by tracking the movement of a group of stars that orbit a region in space. Alternatively, when gas falls into a stellar black hole from a companion star, the gas spirals inward, heating to very high temperatures and emitting large amounts of radiation that can be detected from earthbound and Earth-orbiting telescopes. Astronomers have identified numerous stellar black hole candidates, and have also found evidence of supermassive black holes at the center of galaxies. In 1998, astronomers found compelling evidence that a supermassive black hole of more than 2 million solar masses is located near the Sagittarius A* region in the center of the Milky Way galaxy, and <b>...</b>
Worm Holes
In physics, a wormhole is a hypothetical topological feature of spacetime that is fundamentally a 'shortcut' through space and time. Spacetime can be viewed as a 2D surface (to simplify understanding) that, when 'folded' over, allows the formation of a wormhole bridge. A wormhole has at least two mouths that are connected to a single throat or tube. If the wormhole is traversable, then matter can 'travel' from one mouth to the other by passing through the throat. While there is no observational evidence for wormholes, spacetimes containing wormholes are known to be valid solutions in general relativity. The term wormhole was coined by the American theoretical physicist John Archibald Wheeler in 1957. However, the idea of wormholes had already been theorized in 1921 by the German mathematician Hermann Weyl in connection with his analysis of mass in terms of electromagnetic field energy.[1] This analysis forces one to consider situations...where there is a net flux of lines of force through what topologists would call a handle of the multiply-connected space and what physicists might perhaps be excused for more vividly terming a wormhole. —John Wheeler in Annals of Physics
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"Before the Big Bang?" (2005), the original lecture by Roger Penrose (part 1 of 9)
"Before the Big Bang? A new perspective on the Weyl curvature hypothesis" This is the original lecture by Roger Penrose on his fascinating new model of the universe, its origin and future, and of the "Big Bang"; held at the Isaac Newton Institute for Mathematical Sciences (November 7th 2005). Originally published at www.newton.ac.uk See also www.youtube.com and www.perimeterinstitute.ca for other lectures by Penrose on this theory. See also www.youtube.com for an interview with Roger Penrose on his new model. See also accelconf.web.cern.ch for Penrose's academic article about his theory. See also arxiv.org for an article about Penrose's "Before the Big Bang" idea, verifying that some of Penrose's basic predictions are mathematically correct. NOTE TO THOSE POSTING COMMENTS ON THESE VIDEOS: Please stay focused on the topic. All irrelevant comments will be removed without warning. SUMMARY: There is now a great deal of evidence confirming the existence of a very hot and dense early stage of the universe. Much of this data comes from a detailed study of the cosmic microwave background (CMB)—radiation from the early universe that was most recently measured by NASA's WMAP satellite. But the information presents new puzzles for scientists. One of the most blatant examples is an apparent paradox related to the second law of thermodynamics. Although some have argued that the hypothesis of inflationary cosmology solves some of the puzzles, profound issues remain. In this talk <b>...</b>
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"Before the Big Bang?" (2005), the original lecture by Roger Penrose (part 3 of 9)
"Before the Big Bang? A new perspective on the Weyl curvature hypothesis" This is the original lecture by Roger Penrose on his fascinating new model of the universe, its origin and future, and of the "Big Bang"; held at the Isaac Newton Institute for Mathematical Sciences (November 7th 2005). Originally published at www.newton.ac.uk See also www.youtube.com and www.perimeterinstitute.ca for other lectures by Penrose on this theory. See also www.youtube.com for an interview with Roger Penrose on his new model. See also accelconf.web.cern.ch for Penrose's academic article about his theory. See also arxiv.org for an article about Penrose's "Before the Big Bang" idea, verifying that some of Penrose's basic predictions are mathematically correct. NOTE TO THOSE POSTING COMMENTS ON THESE VIDEOS: Please stay focused on the topic. All irrelevant comments will be removed without warning. SUMMARY: There is now a great deal of evidence confirming the existence of a very hot and dense early stage of the universe. Much of this data comes from a detailed study of the cosmic microwave background (CMB)—radiation from the early universe that was most recently measured by NASA's WMAP satellite. But the information presents new puzzles for scientists. One of the most blatant examples is an apparent paradox related to the second law of thermodynamics. Although some have argued that the hypothesis of inflationary cosmology solves some of the puzzles, profound issues remain. In this talk <b>...</b>
physics cosmology astrophysics quantum mechanics quantum cosmology mathematics maximum entropy space-time geometry phase-space inflation thermodynamics thermal equilibrium dark energy black hole singularity time asymmetry quantum gravity equivalence space-time curvature astigmatism thermalization spherical symmetry Minkowski space conformal geometry gravitational free field Imperator Aquila
"Before the Big Bang?" (2005), the original lecture by Roger Penrose (part 4 of 9)
"Before the Big Bang? A new perspective on the Weyl curvature hypothesis" This is the original lecture by Roger Penrose on his fascinating new model of the universe, its origin and future, and of the "Big Bang"; held at the Isaac Newton Institute for Mathematical Sciences (November 7th 2005). Originally published at www.newton.ac.uk See also www.youtube.com and www.perimeterinstitute.ca for other lectures by Penrose on this theory. See also www.youtube.com for an interview with Roger Penrose on his new model. See also accelconf.web.cern.ch for Penrose's academic article about his theory. See also arxiv.org for an article about Penrose's "Before the Big Bang" idea, verifying that some of Penrose's basic predictions are mathematically correct. NOTE TO THOSE POSTING COMMENTS ON THESE VIDEOS: Please stay focused on the topic. All irrelevant comments will be removed without warning. SUMMARY: There is now a great deal of evidence confirming the existence of a very hot and dense early stage of the universe. Much of this data comes from a detailed study of the cosmic microwave background (CMB)—radiation from the early universe that was most recently measured by NASA's WMAP satellite. But the information presents new puzzles for scientists. One of the most blatant examples is an apparent paradox related to the second law of thermodynamics. Although some have argued that the hypothesis of inflationary cosmology solves some of the puzzles, profound issues remain. In this talk <b>...</b>
physics cosmology astrophysics quantum mechanics quantum cosmology mathematics maximum entropy space-time geometry phase-space inflation thermodynamics thermal equilibrium dark energy black hole singularity time asymmetry quantum gravity equivalence space-time curvature astigmatism thermalization spherical symmetry Minkowski space conformal geometry gravitational free field Imperator Aquila
Atheist Rap Song "I Dont go to church"
Like me on Facebook www.facebook.com Artist Name Young Inc Song name "I Don't go to church" This is a good track to listen to on a Sunday morning.
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Black Holes
Black holes are the evolutionary endpoints of stars at least 10 to 15 times as massive as the Sun. If a star that massive or larger undergoes a supernova explosion, it may leave behind a fairly massive burned out stellar remnant. With no outward forces to oppose gravitational forces, the remnant will collapse in on itself. The star eventually collapses to the point of zero volume and infinite density, creating what is known as a " singularity ". As the density increases, the path of light rays emitted from the star are bent and eventually wrapped irrevocably around the star. Any emitted photons are trapped into an orbit by the intense gravitational field; they will never leave it. Because no light escapes after the star reaches this infinite density, it is called a black hole.
Cosmic Tunnels stars gravitation gravitational forces general relativity event horizon science supermassive black while worm hole singularity Hawking radiation frame dragging time travel New Paradigm
Sonic Riders 2 - 90s Boulevard
90s Boulevard Billy Hatcher Hang On (Bike) The final course in the game, at least in order of the course select screen, is 90s Boulevard. This place probably makes you wonder how a modern metropolis looking place can be in the same world as the rest of the game, which sports a futuristic feel. Well, the game explains it assomething the black hole regurgitated after the events of the Master Core ABIS's defeat. (See the Mobius Strip course for more information about this event.) Nevermind the fact that nothing can come out of a black hole but Hawking radiation... Anyway, 90s Boulevard is the other SEGA-themed course and pays homage to the second half of the history of the company since it got into video games. (They aren't all from the 90s.) You'll see a Virtua Fighter reference right from the beginning, and as I go through the course, you'll also see references to Sonic the Hedgehog (as a series), NiGHTS into Dreams, House of the Dead, Crazy Taxi, Jet Grind Radio, Space Channel 5, and Billy Hatcher and the Giant Egg. Billy Hatcher is one of the most recent additions to the SEGA family, so it only makes sense that I save him for this place. Contributing to the anachronism stew, I put him on the Hang On. Billy Hatcher is a boy granted chicken powers from wearing a chicken suit. His main gimmick is the ability to roll eggs around. He can use them as transportation and as weapons, and he'll always get a pleasant surprise when they hatch. He saves the folks of Morning Land from <b>...</b>
sonic riders zero gravity sega billy hatcher 90s boulevard extreme gear racing Overhazard
Dhorpatan uses Holographic Principle Based Physics as Alternatives to the Holographic Principle
Of the 17 "alternative" solutions given, 12 were actually based directly on the holographic principle. 6 of these were repeats presented as separate solutions. Of the 5 remaining solutions 2 are physically impossible, and the holographic principle is vastly more compelling than the remaining 3 -which could be true but don't tie into much else either. Links: 1.) Dhorpatan's original video: www.youtube.com 2.) Wikipedia article (for #9): en.wikipedia.org 3.) The Zhu-Ren-Singleton's paper (for #14): arxiv.org 4.) (for #15): Abstract for the Zhang-Cai-You-Zhan paper: www.sciencedirect.com 5.) Nikolic's paper (for #17): arxiv.org Physics of the Hidden World (for #17): www.youtube.com
Dhorpatan Holographic principle Bekenstein bound wikipedia Maldacena Hawking Radiation Black hole evaporation Black hole Quantum gravity Physics of the Hidden World Hrvoje Nikoli Douglass Singleton Baocheng Zhang Stephen Hawking Roger Penrose information brane string theory loop quantum gravity Shannon entropy Johanan Raatz