Einstein and the Theory of Relativity | HD |

Summary

This video explores the incredible journey of Albert Einstein's Theory of Relativity, illustrating its profound impact on science and our understanding of the universe. From the inception of general relativity to the confirmation through Eddington's expedition and the eventual acceptance of black holes as a real phenomenon, this narrative captures the transformation of theoretical physics. Eminent scientists such as Roger Penrose and Jocelyn Bell-Burnell contributed to the understanding of these celestial phenomena, confirming the existence of black holes and neutron stars. This tale of discovery continues to challenge and inspire current and future theoretical advancements.

Highlights

• Einstein's Theory of Relativity was a groundbreaking contribution to physics, changing our view on space, time, and gravity. 🌟
• Eddington's 1919 experiment provided substantial evidence for the curvature of space-time predicted by Einstein. 🌞
• The theoretical existence of black holes was eventually confirmed, thanks to contributions from scientists like Roger Penrose and Jocelyn Bell-Burnell. 🌠
• The relationship between quantum mechanics and general relativity continues to intrigue and challenge scientists, pushing the boundaries of our knowledge. 🔬
• Understanding time's relativity and how it changes relative to gravitational forces remains a fundamental question in physics. 🚀

Key Takeaways

• Einstein revolutionized physics with his Theory of Relativity, challenging Newton's centuries-old principles. 🤯
• The Theory of Relativity explains that space and time are interconnected, revolutionizing our understanding of the universe. 🌌
• Einstein's predictions about light bending and black holes were confirmed through observations like Eddington's experiment in 1919. 📸
• Black holes, once a controversial topic, have been evidenced and explored through further scientific discoveries. 🌑
• Time is relative, with its perception changing under different gravitational forces, supported by advanced atomic clocks. ⏳

Overview

Einstein's journey with the Theory of Relativity began with his concept of space-time, revolutionizing the understanding of gravity by proposing that massive objects warp the space around them. This idea fundamentally transformed physics, offering a more comprehensive explanation than Newton's laws ever could.

A pivotal moment in the acceptance of Einstein's ideas was during the 1919 solar eclipse, when Arthur Eddington's observations confirmed the theory's prediction that light would bend around massive objects like the sun. This event significantly boosted Einstein's reputation and validated the scientific community's interest in relativity.

The narrative of relativity didn't stop with Einstein. Later, thinkers such as Roger Penrose and Jocelyn Bell-Burnell expanded on his theories. Their work on black holes and neutron stars confirmed many of Einstein’s predictions, solidifying his legacy and leaving scientists of today with the challenging task of uniting relativity with quantum mechanics.

Chapters

• 00:00 - 00:30: Introduction to Black Holes The chapter titled 'Introduction to Black Holes' begins with a dark and ambient musical backdrop, setting a mysterious tone. The narrator expresses amazement at the capability of modern science to capture the image of a black hole, described as a 'strange star' from which nothing can escape, neither light nor people. This breakthrough is attributed to the equations of general relativity, which were developed a century ago.
• 00:30 - 01:00: The Theory of Relativity Simplified The chapter titled 'The Theory of Relativity Simplified' delves into a theory that experienced a tumultuous journey through its scientific lifecycle. Initially praised, it was later rejected and forgotten, only to be rediscovered at a crucial moment. The narrative captures a dramatic episode where the theory faced near obliteration, metaphorically described as being nearly killed by a 'black hole,' emphasizing the perilous challenges in its acceptance and survival.
• 01:00 - 01:30: The Essence of Relativity The chapter discusses the theory of relativity, aiming to demonstrate that it is not uniquely difficult to understand.
• 01:30 - 02:30: The Legacy of Newton and Einstein Einstein's theory of relativity, though often perceived as strange and complex, is accessible to those willing to engage with it thoughtfully. Albert Einstein, known for his famous equation E = MC² in the 20th century, utilized mathematics to explore and explain the fundamental architecture of the universe through his theory of relativity.
• 02:30 - 03:30: The Principle of Free Fall and Equivalence The chapter discusses the principle of free fall and its relation to the theory of general relativity. General relativity is a gravitational theory that explains the force causing stars and planets to attract each other. Prior to general relativity, Isaac Newton's laws governed our understanding of gravity. This chapter marks a significant shift from Newtonian physics, highlighting how general relativity revolutionized physics and mathematics.
• 03:30 - 04:30: A Leap in Understanding: General Relativity The transcript explains how Einstein's theory of gravity led to a significant paradigm shift from Newton's theory. Einstein introduced the concept of space being curved, which contrasts with Newton's idea of straight space, marking a profound advancement in understanding gravity.
• 04:30 - 06:30: Mercury and Mathematical Challenges In this chapter titled 'Mercury and Mathematical Challenges,' the intertwined nature of space and time is discussed. The narrative explains that the concept of a position at a given time is now obsolete as space and time are actually connected, which requires understanding them in four dimensions. It emphasizes the need for a new geometrical equation to account for this interconnectedness, moving away from traditional equations.
• 06:30 - 08:30: The Issue of Singularities The chapter discusses the concept of singularities in the context of gravity and general relativity. It elaborates on how space-time is affected by gravitational fields, leading to natural phenomena such as planets orbiting the sun and the inability of even light to escape these fields. The discussion is rooted in the principles of free fall, as first recognized by Galileo and observable on the moon.
• 08:30 - 11:30: Einstein's Struggles and Triumphs The chapter titled "Einstein's Struggles and Triumphs" explores significant insights and moments in the life of Albert Einstein. It opens with an illustrative experiment often attributed to Galileo, using a hammer and another object to demonstrate the concept of free fall and its equivalence in physics, highlighting fundamental understandings that influenced Einstein's theories.
• 11:30 - 18:30: Black Holes and Modern Discoveries The chapter discusses Einstein's realization about gravity while working at the patent office in Bern. He thought about how a person in free fall would not feel their own weight. This led him to understand that gravity is unique in how it can disappear due to its own effect.
• 18:30 - 24:00: The Impact and Future of Relativity The chapter begins by exploring the concept of relativity and gravity, emphasizing that in free fall it feels like there's no gravity. It contrasts early experimental limitations with modern advancements. Physicists now have sophisticated tools, such as a German tower designed to eliminate air resistance by creating a vacuum. Within this vacuum, objects and capsules are dropped to observe the effects of free fall, illustrating that weight seemingly disappears. The narrative is complemented by a translator explaining an experiment involving two objects placed on a scale in a capsule to demonstrate these principles.

Einstein and the Theory of Relativity | HD | Transcription

• 00:00 - 00:30 (dark ambient music) - [Narrator] Who would've believed that one day we'd be able to see this image? A black hole in the universe, a strange star from which no light or person can escape. This image was calculated using the equations of general relativity, a scientific theory of space and time developed 100 years ago,
• 00:30 - 01:00 a theory that was in turn praised, rejected, forgotten, and then rediscovered, a theory that this black hole nearly killed, my theory. (dramatic music)
• 01:00 - 01:30 - The theory of relativity is infamous for its difficulty. I want to show that there's nothing peculiarly difficult about it. - Let me illustrate this with an example here, let's imagine that this piece of jelly is the sapce and the presence of matter is to distort the space.
• 01:30 - 02:00 - Einstein's theory of relativity does lead us into very strange and unfamiliar paths. - Relativity is perfect intelligible to anybody who is willing to think. (dramatic music) - [Narrator] In the 20th century, I was known by the name of Albert Einstein and for my equation E = MC squared. I sought to understand nature through mathematics. I had a new vision of the architecture of the universe and I expressed it in a theory,
• 02:00 - 02:30 general relativity. General relativity is a theory about gravity, the mysterious force that attracts stars and planets to each other. For 250 years before my theory, gravity was the realm of the great scientist Issac Newton. My theory revolutionized the worlds of physics and mathematics. (speaking in foreign language)
• 02:30 - 03:00 - [Translator] Newton's theory of gravity, revolutionary in its scope and concision, had held water since the end of the 17th century. It is fascinating to think that to explain just a few changes to this law, everything had to be turned on its head. And that is exactly what Einstein did. His theory of gravity involves several major modifications. Space is no longer straight but curved depending on the matter inside.
• 03:00 - 03:30 Giving a position at a given time no longer makes sense. Positions and times are intertwined and geometry now has to be seen in four dimensions and we can't count on this equation here anymore. It needs to be replaced by one with a radically different form. (dramatic music) - [Narrator] First of all, I discovered that space and time were actually connected, working as one and matter such as stars and planets
• 03:30 - 04:00 bends and curves the space-time. That curvature is the gravitational field obliging the planets to rotate around the sun, nothing, not even rays of light, can escape the curvature. All these discoveries were based on a single observation, that of free fall, known since Galileo, and which can even be observed on the moon. - Well in my left hand I have a feather,
• 04:00 - 04:30 in my right hand a hammer and I'll drop the two of them here and hopefully they'll hit the ground at the same time. Galileo was correct. - [Narrator] I saw and understood free fall differently from all other people. It guided me towards the curvature of space-time. All I had to do was observe closely. - [Translator] Einstein himself tells us about the moment when he understood
• 04:30 - 05:00 that this was the tool that would allow him to form his theory. (speaking in foreign language) In 1907 he wrote, "I was sitting at my desk "in the patent office in Bern "when suddenly, I thought that if somebody was in free fall "they wouldn't feel their own weight and I was surprised." He realized that gravity has the property and is the only force with this property of disappearing as a result of its own effect and that if we're in free fall and so under the effect of gravity
• 05:00 - 05:30 we feel like there's no gravity. - [Narrator] In my day, I was only able to experiment this idea through thought. But 100 years later, the physicists of the 21st century have new tools such as this tower in Germany which can create a vacuum that eliminates air resistance. By dropping objects and capsules into the tower, we can see how, in free fall, our weight disappears. (speaking in foreign language) - [Translator] In this experiment, we put two objects on a scale in this capsule
• 05:30 - 06:00 which will be dropped into free fall in the tower. The needles on both scales will fall back to zero showing, albeit not particularly precisely, how this apple and this one kilo weight fall in exactly the same way in the gravitational field. So it looks like mass doesn't exist anymore which may seem absurd because if we're able to eliminate gravity, then does gravity exist?
• 06:00 - 06:30 Once sealed, the capsule will be raised to a height of 110 meters for a five second free fall in the vacuum.
• 06:30 - 07:00 - So we have the perfect conditions for every experiment that is done in weightlessness. For example, if we have some experiments for space we can test the payload of the equipment in our facility. - Oh, thank you. - You're welcome. (dark ambient music)
• 07:00 - 07:30 - [Hanns] Here we have a view of the inside of the drop tube. - Okay, so three-- - Then, after one second it will go. - Three, two, one. Wow. (crashing) (clapping)
• 07:30 - 08:00 Impressing. So now (mumbles). - So now we have to search for the right time in the video for the five seconds-- - The five seconds, okay. So this is after something is happening. Okay so now, here we are during the free fall, so it was zero on both sides, gravity has disappeared. It worked.
• 08:00 - 08:30 - Yeah. - [Narrator] Until now, this principal, the cornerstone of my theory has proved water tight. Nobody has been able to prove it wrong. A team of French researchers is preparing to test the principal in space. Their satellite microscope, set for launch in 2016 will orbit 700 kilometers above the earth and provide an unprecedented precision of measurement. But let's wait and see. In science, the experiment is our sole judge.
• 08:30 - 09:00 Back in 1907, this idea, today known as the principal of equivalence, led me like a lighthouse in the night to rethink gravity. (dramatic music) I returned to Switzerland in 1912 after five years of work. I returned to the city of my student days.
• 09:00 - 09:30 The two years I spent in Zurich would be the most important of my life. I was offered a professorship in physics at the Zurich Polytechnicum School now known as ETH Zurich. - So here's ETH. - [Narrator] One of my old university friends, Marcel Grossman, had become a professor there.
• 09:30 - 10:00 He was far better than me in geometry. His notebooks inspired me on numerous occasions. - [Translator] Impressive, no? - [Translator] Yes, it's very detailed. - [Translator] The fundamental properties of elliptic functions. He was preparing to work for Einstein, without knowing it, obviously. But that's what was going on. It's really surprising.
• 10:00 - 10:30 I didn't think it happened like that. - [Narrator] What I would have done without Grossman, I really cannot say because the mathematical obstacles before me seemed insurmountable. General relativity made me work like a monomaniac. To see if I was on the right track, I used a flaw in Newton's theory. Newton's gravitational equation
• 10:30 - 11:00 couldn't predict the precise orbit of Mercury around the sun. Mercury's perihelion, it's closest point of the sun during the year, shifted much too fast. This was a perplexing problem that physicists and astronomers just couldn't crack. - [Translator] He arrived at the definitive theories in November 1915, definitive in particular because he determined Mercury's perihelion with incredible position.
• 11:00 - 11:30 - [Narrator] After all these years, I still remember those evenings spent with Marcel Grossman in this cafe on the river Limmat putting the world into equation. Our discussions concerned not only our studies but ranged far beyond over all the topics that could interest young people who kept their eyes wide open. It was here that my theory took form. (speaking in foreign language) - [Translator] The key to describing gravity is the geometry of space-time.
• 11:30 - 12:00 So for the object present in the universe, you have to determine the gravitational field they create, namely the geometry of space-time. - [Narrator] To do so hinged on solving an equation that took me eight years to create. I wrote it as follows, G mu nu is equal to eight pi G over C4 times T mu nu. A single equation and just a few mathematical symbols to describe our universe. - [Translator] Based on a mathematical hypothesis, he opened up a new path,
• 12:00 - 12:30 one that is still relevant today. It's incredible. You could've thought that it wasn't going to work. - [Narrator] But it did work and it was here that the theory started to take on a life of its own, to unveil properties of nature that nobody had foreseen. Curve geometry implied that time didn't pass in the same way in all parts of the universe. Gravity influences time. The stronger the gravity field, the more time slows down.
• 12:30 - 13:00 This threw everybody, myself included. In my day, it was impossible to test this prediction through experiments, gravity on earth is too weak and its effects on time are imperceptible. But technology having evolved, in your day, this difference in time can be measured with amazing precision. The new atomic clocks in the basement of the Observatoire de Paris are the most precise clocks in the world,
• 13:00 - 13:30 a billion times more precise than a quartz clock. Even at this level of precision, my theory still works. The effect is true everywhere. The universe does not tick to a huge universal clock as Newton thought. Each region of the universe has its own time. Each galaxy and each solar system exists in its own space-time. Looking at the universe involves looking at other times.
• 13:30 - 14:00 In 1915 with world war raging, the publication of the theory of general relativity went unnoticed, gravity being elsewhere. But I did receive a letter from the German physicist Karl Schwarzschild. With my equations, he had succeeded in calculating the distortion of space-time generated by a star. This was a titanic achievement given that my equation breaks down into 10 others
• 14:00 - 14:30 and each one of them had to be solved. But his work exposed a sort of minor flaw in the equations that nobody noticed. This flaw would later be called a Schwarzschild singularity. With his solution, Karl Schwarzschild cleared the way for the mathematical exploration of the theory. Unfortunately, this was to be the only letter I received from him. He died in the war in May 1916. The seemingly never ending war,
• 14:30 - 15:00 prevented the circulation of scientific publications but a ray of hope came to me from Great Britain where I was nevertheless considered an enemy. - In Britain in 1915, there was a British astrophysicist called Eddington who was a pacifist who was not at war, in fact was still at his post in Cambridge. Now, it so happens that Eddington was one of the few people in Britain who was capable of understanding what Einstein was writing
• 15:00 - 15:30 and he immediately grasped the significance of this general relativistic theory. - [Narrator] The best physical test to confirm my theory was to measure if the rays of light reaching us from far away actually follow the space-time curvature. The sun is the only close and available mass that can curve space-time in a significant manner but if the sun is in the sky it is day time and the distant stars are invisible.
• 15:30 - 16:00 Our only chance would be to photograph the starry sky during an eclipse. - The war ended in 1918 and the following year he traveled, he led an expedition which went into parts, part to the island of Principe off the coast of Africa and to Brazil. Weather wasn't totally favorable, the observations weren't brilliant but they were sufficient to show that light was bent
• 16:00 - 16:30 in exactly the way Einstein had proposed and when he came back, Eddington did a number of presentations and huge popular lectures about this work and I think in the English-speaking world that launched Einstein. - [Narrator] Eddington presented his results to the Royal Astronomical Society, standing before a large portrait of Newton that had sat there undisturbed for over two centuries.
• 16:30 - 17:00 Reportedly, the whole atmosphere of tense interest was exactly that of a Greek drama. - Napoleon and other great men of his type, they were makers of empires but there is an order of men who get beyond that, they are not makers of empires but they are makers of universe. (applause) When they have made those universes, their hands are unstained by the blood
• 17:00 - 17:30 of any human being on earth. (applause) Galilei made a universe which lasted 1,400 years. Newton also made a universe which has lasted 300 years. Einstein has made a universe and I can't tell you how long that will last. (laughter) - [Narrator] After my theory was confirmed, I received invitations from around the world.
• 17:30 - 18:00 During one of my trips in 1921, I found out that I'd been honored with the Nobel Prize for Physics. Strangely, I didn't receive the prize for general relativity no doubt still too controversial but for my previous work. There was little talk of my theory of relativity. As Charlie Chaplin once said to me, they're cheering us both, you because nobody understands you and me because everybody understands me. When I was in Paris in 1922,
• 18:00 - 18:30 people wanted me to talk about time. I recall people talking about it more in philosophical psalms than in scientific conferences. The fact is, nobody there understood the slightest thing about my theory but my most vivid memory is of a conference at the College de France. A French mathematician Jacques Hadamard stood up and pointed at me threateningly, pointing out a supposed flaw in my theory. He brought up the very mathematical flaw that had escaped me in Schwarzschild's solution.
• 18:30 - 19:00 (speaking in a foreign language) - [Translator] That's the Schwarzschild solution from 1916. - [Translator] If I understand correctly, R is the radius relative to a central point, namely a star? - [Translator] Yes, it's a star and its mass is M. - [Translator] Okay but you can see straight away that there is a problem because if I see a radius equal to 2GM divided by C squared
• 19:00 - 19:30 the coefficient here becomes zero, which isn't right, and here you get one divided by zero equals infinity, which is even worse. Your solution falls flat on its face. - [Translator] That's exactly what Jacques Hadamand said to Einstein in Paris. It was terrible for Einstein because here obviously we're talking about mass but think about physics, which for example determines the geometry around our sun, the sun in the solar system. Imagine we send a satellite towards the sun.
• 19:30 - 20:00 What happens when the satellite gets to this point? Does it stop, does it explode or does it disintegrate? - [Translator] And that must've been seen as a fatal blow to Einstein's theory right? - [Translator] It did pose a major problem for Einstein because his theory was supposed to determine the structure of space-time and for a particular solution, he saw that there were places where the idea of space and the idea of time no longer made sense. The end of the world in equation form. That's right, the edge of the world, what we call the Schwarzschild singularity.
• 20:00 - 20:30 - [Narrator] No doubt this all looks abstract to you, a few symbols on a blackboard but for me, this singularity was a real monster. It resembled a sphere, an impenetrable black bubble, a place in the universe where time seemed to stop and where space no longer existed. The sphere appeared at the center of all celestial objects like a star. Fortunately, after a few calculations,
• 20:30 - 21:00 we discovered that for our sun, the size of the singularity was just three kilometers, hidden inside. For it to become visible in our solar system, we would need to be able to condense the entire mass of the sun into a three kilometer sphere. For astrophysicists then, the singularity remained imaginary but mathematicians had a serious problem on their hands. Would it prove fatal for my relativity? Soon the entire community was talking about this singularity and apart from a few firmly convinced cosmologists,
• 21:00 - 21:30 pretty much everyone dropped my theory. (speaking in foreign language) - [Translator] These were hard times for Einstein. After his glory days when relativity was in all the newspapers, when he was the star of the Parisian salons and spent the 1920s traveling around the world, he was the most heralded scientist of the day. But interest in his theory shrank dramatically and life for people working on relativity became difficult.
• 21:30 - 22:00 - [Narrator] With Elsa, I moved to Caput near Berlin. I took up sailing as a hobby until the day when events forced me to leave my homeland in 1933 forever. - Dr. Einstein, who gave the world its biggest headache, is back in California again with his wife. They've been fog bound all night in St. Peter Harbor. The professor had a theory as to how they could land but before he and the captain could figure it out,
• 22:00 - 22:30 the fog had all gone away. Now he's going to the Institute of Technology in Pasadena to work with other distinguished scientists. There his theory will be thoroughly discussed and analyzed and if it is what he says it is, why then everything will be alright, won't it? (speaking in foreign language) - [Translator] Physicists were extremely wary and not very interested. There was a certain amount of aggression from physicists in particular except for the people who believed it who were few and far between and then there were those
• 22:30 - 23:00 who simply didn't want to try and get their heads around it. (dark ambient music) - [Narrator] The problem of singularity grew as the years went by. The impenetrable sphere, hidden in the heart of the stars remained an obsession, impossible to understand, to imagine,
• 23:00 - 23:30 the edge of the world. Relativistic scientists working on the gravity of stars such as our sun found that according to my theory, stars could die. That really was the limit because the theory appeared to say that in dying the star imploded and its size reduced to approach that of its singularity. - So stars are born and live and die.
• 23:30 - 24:00 The sun's future history is fairly simple, not good for us on earth. The sun will go through several phases including swelling then it will ultimately shrink to one of these white dwarfs and will steadily cool thereafter, just stop producing energy, stop its fusion reactions but still quite hot and cooling. For a star that's much bigger than the sun,
• 24:00 - 24:30 basically what happens is the core of the star collapses to make a neutron star. The rest of the material suddenly finds it's standing on nothing goes rushing down to get a foothold, meets this very, very solid neutron star and burns it out and 90% or 95% of the material goes out and the other little bit remains. - [Narrator] This extremely dense neutron star
• 24:30 - 25:00 with a radius of barely 10 kilometers is coming dangerously close to the Schwarzschild singularity sphere hidden in its center. The risk I immediately saw was that it could be discovered in a theory that stars could condense even further and their singularity escape from within. (speaking in foreign language) - [Translator] The question that immediately comes to mind is do we know any stars who Schwarzschild surface, the edge of the theory, is on the exterior of the celestial body? - [Translator] You would've made an excellent physicist
• 25:00 - 25:30 or even astrophysicist. Can we find any solutions in which we have the star or the celestial body and here the Schwarzschild singularity? - Those are probably created from really massive stars. Once that big star begins to run out of nuclear fuel gravity wins so the star shrinks. That puts up the gravity at the surface of the star so it shrinks which puts up the gravity at the surface of the star
• 25:30 - 26:00 so it shrinks and it shrinks right down and even the atoms, things like this table and chair are made of, the atoms collapse and the nuclei collapse and if you believe the theory, it collapses down to a point which is zero radius. Some people don't like these kinds of points and zeros so that's debated but it goes down to very, very, very small,
• 26:00 - 26:30 having been one of the biggest stars in the universe before. And it's a black hole. (dark ambient music) - [Narrator] All of a sudden, mathematicians and physicists were telling me, Einstein, that the Karl Schwarzschild singularity, the flaw in my theory, could in reality exist in the real universe, stepping out of the world of mathematics like a magical sphere
• 26:30 - 27:00 and a completely black sphere, a place where space and time disappear. I didn't want to believe it. For me, the singularity had to remain a mathematical hypothesis. (speaking in foreign language) - [Translator] A star can't just cave in like that, cave in, not stretch but implode, it's not possible. There's something unbearable about that. - Other people, in particular Eddington,
• 27:00 - 27:30 thought there must be something wrong. He thought there must be something wrong in the calculation but if not, there had to be something wrong in the physics. So he thought, nature shouldn't behave like this but then it is a strange way for nature to behave, it's just very different from the sorts of things that one is used to. - [Translator] The most extraordinary thing in all this was Einstein himself. He didn't want to believe that the Schwarzschild singularity
• 27:30 - 28:00 could really be manifested. So he set out to prove it. The worst paper he ever wrote. He took the conclusion he wanted to reach as the basis for these calculations. - [Narrator] The main result of my research clearly concluded that Schwarzschild's singularities didn't exist in physical reality. - [Translator] It really was a poor paper by Einstein, one of the worst but we can forgive him because he did write some excellent ones too.
• 28:00 - 28:30 - [Narrator] It was all too much for me. My own theory had completely escaped my grasp. Since the mathematicians had invaded the theory of relativity, I did not understand it myself anymore. In the USA in the '50s, I was seen as a sort of fossil made deaf and blind by the years. Ultimately I didn't mind that role. It suited my temperament. Shrouded in this mystery,
• 28:30 - 29:00 I left our planet and I can guarantee you that the most beautiful thing we can experience is the mysterious. (upbeat music) The doubt persisted after my death. The black hole continued to disturb.
• 29:00 - 29:30 A number of competing theories showed that it can't even exist because logically speaking a star cannot simply collapse to zero. But the life of relativity would be changed by the 1960s and the British. - Well according to Einstein's theory, the black hole results from the collapse of a star several times the mass of the sun would be an object several miles in diameter. But if you, say imagine the earth compressed right down
• 29:30 - 30:00 until it became a black hole, the dimension will be a bit less than an inch, something like that. - [Interviewer] That's the earth? - The earth would have to be compressed into that size to be a black hole. - [Narrator] Roger Penrose had, like myself in my day, ideas that came to him entirely unannounced. - At the time I was getting very interested in this which was about 1964, perhaps a little earlier than that, and there was a lot of interest in gravitational collapse at that time. While I was pondering over these issues at one time,
• 30:00 - 30:30 I was at this time at Birkbeck College where I was a lecturer and a colleague of mine, Ivor Robinson, who also had an important influence on many aspects of general relativity, and he was talking to me very excitedly about certain things, I forget what they were, I'm afraid, but we came to a road and when we crossed the road, the conversation stopped and when we get to the other side, instead of walking into a wall
• 30:30 - 31:00 I forget the idea I had which was crossing the street here, you see, and then he goes off later and then I try to remember why I feel happy. Why do I feel happy? I have no idea. So I think, my breakfast? No, ordinary breakfast so on all through the day and I think, aha, I had this idea
• 31:00 - 31:30 about how you could characterize a collapse of a star to a point where it is gone too far, a point of no return and this was a surface which I call a trap surface and this surface can be irregular, can be not symmetrical, but it has a very curious property that the light on both sides is focused inwards and I knew I could use this condition
• 31:30 - 32:00 to try to prove a theorem. (upbeat music) - [Narrator] Roger Penrose put into an equation the black hole that had thwarted so many physicists before him, myself included. He proved definitively that when a star collapses, all its constituent matter condenses into a single central point, an infinite density of matter, a point where time stops. Roger Penrose worked with some important people and most decisively with the young physicist Stephen Hawking.
• 32:00 - 32:30 The two earned a medal from the Royal Astronomical Society for their work on black holes. - Well, I haven't seen this before. Yes, proposal for the Eddington medal, that's what it was, yes. I talked to Stephen at that time and we had quite a long discussion on the details of this type of argument and this had a big effect on what he did later.
• 32:30 - 33:00 He generalized the argument to cosmological situations and then further, later on we got together and had a general theorem which seemed to encompass pretty well all the things that had occurred earlier. - [Narrator] I'd been dead for 10 years, I think, and this time I had to accept that my theory predicted the existence of black holes. Despite everything, even if the work of Roger Penrose was convincing, nothing proved that these singular celestial bodies arising from the death of stars,
• 33:00 - 33:30 actually existed. It was all purely theoretical. But new means of astronomical observation were developed in the '60s and a young British scientist was to change our vision of the universe forever. Her name is Jocelyn Bell-Burnell. - Radio astronomy revealed new kinds of objects, things that did not look particularly conspicuous or spectacular to the optical astronomer. My first two years were spent working in the field
• 33:30 - 34:00 constructing a radio telescope. By the time end of my PhD I could swing a sledgehammer which was not a skill I expected to acquire but I did. We started observations in the summer of 1967 and after about a few weeks of observing,
• 34:00 - 34:30 there was the first indication of a curious signal. (dramatic music) So then I turnt my attention to this thing which meant going out to the observatory each day just before the telescope turned to it, switching to a high speed recording and it turned out to be this string of pulses
• 34:30 - 35:00 about one and a third seconds apart which was not something I expected, I have to say. We hadn't known about anything like that. We hadn't imagined that anything like that could exist. - [Narrator] But the universe doesn't change in a day. Jocelyn Bell-Burnell came under heavy criticism until she detected, after months of enflaging work a second similar source. - Ha, what's that?
• 35:00 - 35:30 That looks a bit like the first signal that we've been chasing. That bit of sky will be seen by the telescope at two o'clock in the morning. It was very cold and the equipment wasn't working properly in cold weather, it was some problem with the receivers and of course when I got there, it wasn't working properly but I got it to work properly for five minutes and it was the right five minutes as the telescope was looking in that direction
• 35:30 - 36:00 and it was the right beam setting and in came pulse, pulse, pulse, pulse. And that for me was actually the eureka moment, the sweet moment, 'cause you know it's not the equipment at the fault, you know it's not interference, it really does begin to look like a new class of object,
• 36:00 - 36:30 still don't know what. - Well these signals that we're picking up are entirely new, nothing like this has been seen in radio astronomy before. - Here is a discovery which illustrates the universe is far more complex than we at present believe. (dramatic music) - It's not showing any sign of tiring
• 36:30 - 37:00 which means it's got lots of energy which means it's big but because it's going fast, it's small, so it's big and it's small. That didn't make sense for awhile until we got our questions a little sharper. It's small in the sense of how wide it is but it's big in the sense that it's got a lot of mass. Not that it's physically big but it's got a lot of mass
• 37:00 - 37:30 and we can see with hindsight that these very, very dense stars which are small and massive actually explained it. - [Narrator] Jocelyn Bell-Burnell had discovered a pulsar and everything seemed to suggest that a pulsar was a neutron star. The remnants of the death of an extremely dense star, neutron stars are the closest thing to a black hole.
• 37:30 - 38:00 So my theory was right and in the end, I was wrong to doubt it. Anyone who has never made a mistake has never tried anything new. - [Translator] It became clear then that all the theoretical hypotheses posited earlier on, what was possible and how stars evolved, how they died and how they can collapse to become neutron stars were true and correspond to phenomena in the real universe which also meant that the next step,
• 38:00 - 38:30 i.e. if you have a dead star but one that is too massive to be a neutron star and so according to Einstein's theory has to be a black hole was that black holes exist too. And after the discovery of pulsars, the conceptual landscape changed and everyone considered it clear that not only did neutron stars have to exist but that black holes had to exist too and that we would find them one day. (machine clicking)
• 38:30 - 39:00 - The gravity on a pulsar is very, very strong. You've got the mass of the sun, thousand million, million, million, million tons all in a ball 10 kilometers across and this produces some curious effects, curious to our minds. They're explainable by general relativity. One is that the gravity bends light rays. So if I look that way on the surface of the pulsar I actually see over the horizon.
• 39:00 - 39:30 I see over the horizon in every direction and it also effects clocks. If I'm on a pulsar and you can see my watch, you see the second hand is making one tick every two seconds because the gravity has slowed the clock so much. I can use my watch, take my own pulse, and it's okay but that's because the gravity
• 39:30 - 40:00 has slowed my heart the same way and my metabolism and actually I have problems getting onto the neutron star, the pulsar, because as i come down to land I am pulled down by this very strong gravity but there's a very strong gradient of gravity, the force on my feet is much stronger than the force on my head. (slurping) Your body gets stretched. There's a technical term for this. It's called spaghettification after spaghetti
• 40:00 - 40:30 but actually the difference in force between the bottom of your body and the top of your body is so strong it breaks, your body gets pulled apart. Your feet get pulled off your legs, your legs get pulled off your body, your head separates from your body and the different bits of your body drop onto the neutron star one after the other. So don't go there, not a healthy space.
• 40:30 - 41:00 (dark ambient music) - [Narrator] The universe is far stranger than I dared to imagine. The famous Schwarzschild singularity, an impenetrable sphere, actually represented the edge of a black hole. But what actually happens if we try to cross it?
• 41:00 - 41:30 - [Translator] This surface has an extraordinary property. It isn't material and yet it separates space-time into two zones, each with different properties. You can cross it in one direction and send light from the exterior to the interior but you can't send light from the interior to the exterior. - [Translator] It's a trap you never get out of. (energetic music)
• 41:30 - 42:00 - [Narrator] A black hole is above all a solution to the theory of general relativity. It is a mathematical solution, a space-time configuration, a universe and the question is finding out if this solution actually corresponds to something in the physical world. - [Translator] We aren't sure that black holes exist in the real universe.
• 42:00 - 42:30 There are strong signs though they remain indirect. (speaking in foreign language) But the entire evolution of astrophysics in the 20th century, the fact that stars are born and die, that very dense, dead stars exist such as neutron stars, and that neutron stars have a maximum mass, all this strongly indicates that black holes must exist in the real universe. (speaking in foreign language) Maybe we will find absolute proof in a few years.
• 42:30 - 43:00 (speaking in foreign language) (dramatic music) - [Narrator] Finally, my theory of general relativity has found its field of application. It describes the infinitely large. Astronomers today are following in the footsteps of Roger Penrose, Jocelyn Bell-Burnell, Thibault Damour and many others as they search for the existence of black holes
• 43:00 - 43:30 hidden in the immensity of our universe. Without relativity, there would be no big bang theory, no relativistic astrophysics and not even a scientific cosmology with which to speculate on the origin of our universe and its future. That said, as always in science, each new discovery brings with it new questions and the black hole concealed yet another surprise over its horizon. - [Translator] So if you go inside a black hole,
• 43:30 - 44:00 you should find a point at its center because if a star collapses in on itself, it crosses the horizon. But what does it do after that? It collapses. And what happens? General relativity says that the fabric of space-time tears and that a true space-time singularity now exists at the center of the black hole. In other words, space-time has ceased to exist. - It gets swallowed by the hole
• 44:00 - 44:30 and then that information is lost to the universe. Now you see this is not something people like. I can see there's some feeling of unhappiness from you on this position point. You're not unique in this, I may say. And it's probably the majority view amongst physicists now that the information somehow has to get back in. Maybe into another universe, maybe gets out through some curious effects of quantum mechanics,
• 44:30 - 45:00 one way or the other. Personally, I think it has to be lost. - [Narrator] Today, I enjoy watching all these relativistic scientists from afar as they try to resolve new mysteries. From string theory and loop theory to non commutative geometry and twisters, a number of ideas have emerged to try and go beyond my theory. One such speculative idea has been developed by Carlo Rovelli.
• 45:00 - 45:30 (speaking in foreign language) - [Translator] General relativity works very well but it clearly tells us that it doesn't work in the center of the black hole where a singularity takes hold. And this is where we need quantum mechanics and for which we have a theory of quantic gravity that should tell us what is going on. What that theory tells us or suggests is that afterwards it bounces out and boom. - [Translator] Hold on, if you say that it bounces out then you should be able to see loads of little explosions everywhere so why don't you? - [Translator] Exactly.
• 45:30 - 46:00 That's the magic of the theory. Because if you were on the star and strong enough to resist all that pressure, then that rebound would be practically immediate, a few milliseconds. - [Translator] Except that in general relativity, Time passes at different speeds in different places. - [Translator] In a black hole, that effect becomes enormous, very, very strong. According to our calculations, a millisecond inside a black hole corresponds to billions of years outside.
• 46:00 - 46:30 So if this image is correct what is a black hole? It's a star that becomes extremely small, a plank star, and then bounces out and explodes but seen from the outside the whole thing happens in slow motion, extreme slow motion, taking billions and billions of years. (speaking in foreign language)
• 46:30 - 47:00 - [Translator] I think that a mystery lies at the heart of physics, a mystery that is yet to be solved. And that mystery is the nature of time. What really is the passing of time? We've discovered that time is not universal as understood by Newton, we've discovered that each person has their own time, we've discovered lots of things about time but what really is the passing of time? We don't know. The theory my colleagues and I are working on, loop quantum gravity,
• 47:00 - 47:30 has a set of equations limited to general relativity in one case and quantum mechanics in another. (speaking in foreign language) These equations are special because they have no time parameter in them. So time is not a fundamental ingredient of the universe. (speaking in foreign language) Obviously, as with all theories of quantum gravity, we are not sure because we have not yet to establish measurements providing theory but I think that on the whole, everyone is convinced
• 47:30 - 48:00 that putting general relativity and quantum mechanics together changes something fundamental in our understanding of space and time. (speaking in foreign language) (dark ambient music) - [Narrator] To tell you the truth, I would never had wagered that 100 years later my theory would still be around. I thought by this stage, you would've replaced it with a better one. Now you have to unite quantum theory with my theory of general relativity.
• 48:00 - 48:30 I'm convinced that this will once again revolutionize our vision of space and time, as my theory revolutionized the vision of Newton. (speaking in foreign language) - [Translator] Issac Newton, with Einstein, was able more than anyone else to see further, to see more things and discover more things in the world. In a letter he wrote at the end of his life, there's a beautiful sentence in which he says
• 48:30 - 49:00 that he doesn't know exactly how others will see him or how they will remember him but he sees himself as a child on a beach playing with pebbles, a child who is happy because he has found some particularly beautiful pebbles while in front of him, lies the immense ocean of all the things he is yet to understand. And I'm sure that Einstein shared that same sense of the immensity of all we have yet to know.
• 49:00 - 49:30 (dramatic music)