“This book is the biography of general relativity.” Overall, a good story of the individuals involved in the advancement of physics, including General Relativity, the Stand Model, String Theory and to today's Quantum Gravity. Not to technical so a good book for people just looking for a high-level overview. Knowledge enough to be dangerous.
"By measuring the positions of those stars, Eddington had found that the theory of gravity invented by British Science's patron saint, Isaac Newton, a theory that had been accepted as truth for over two centuries, was wrong. In its place, he claimed, belonged a new, correct theory proposed by Albert Einstein, known as the “general theory of relativity.”
“According to Einstein, space and time are intertwined in a cosmic dance as they respond to every single speck of stuff imaginable, from particles to galaxies, weaving themselves into elaborate patterns that can lead to the most bizarre effects.”
“Almost a third of the universe seems to be made up of dark matter, heavy, invisible stuff that swarms around galaxies like a cloud of angry bees. The other two-thirds is in the form of an ethereal substance, dark energy, that pushes space apart. Only 4 percent of the universe is made of the stuff that we are familiar with atoms.”
“The Scottish physicist Hames Clerk Maxwell showed that these two forces could be seen as different manifestations of one underlying force, electromagnetism, and that how they are perceived depends on how an observer is moving. A person sitting next to a bar magnet would experience magnetism but no electricity. But a person whizzing by would experience not only the magnetism but also electricity. Maxwell unified the two forces into one that remains equivalent regardless of an observer’s position or speed.”
“The latter postulate required some adjustments to Newton’s laws. In the classic Newtonian universe, speed is additive. Light emitted from the front of a speeding train moves faster than light coming from a stationary source. In Einstein’s universe, this is no longer the case. Instead, there is a cosmic speed limit set at 299,792 km per second. Bit then odd things happen. So, for example, someone travelling on a train moving at close to the speed of light will age more slowly when observed by someone sitting at a station platform, watching the train go by. And the train itself will look shorter when it is moving than when it is sitting still. Time dilates and space contracts.”
“Sitting in an accelerating spaceship should feel no different from sitting in a spaceship at rest, feeling the pull of gravity. As Einstein has realized, at its simplest level, acceleration is indistinguishable from gravity.”
“In essence, Einstein argued that what we perceive as gravity is nothing more than objects moving in geometry of spacetime. Massive objects affect the geometry, curing space and time. Einstein has finally arrived at his truly general theory of relativity.”
“We can think of light as a collection of waves with different wavelengths corresponding to a different energy state. Red light has a longer wavelength and lower energy state than blue light, at the other end of the spectrum. When we look at a star or galaxy, or any bright object, the light it emits is a mixture of these waves, some more energetic than others. What de Sitter found was that the light of any faraway object would be invariably pushed toward the red, appearing to have a longer wavelength and less energy than similar objects.”
“When a source of light is moving away from an observer, the wavelength in its spectrum appears to stretch. The new effect is that light will look redder. Conversely, is a source of light is moving toward the observer, its spectrum is shifted to shorter wavelengths and will look bluer. This effect, known as the Doppler effect, is something you have probably experienced in the context of sound.”
“Robert Oppenheimer wasn’t particularly interested in the general theory of relativity. He believed in it, as any sensible physicist would, but he didn’t think it was particularly relevant. Which would make it ironic that he would discover on of the strangest, most exotic predictions of Einstein’s theory: the formation of black holes in nature.”
“Oppenheimer showed that is a star is big and dense enough; it will collapse out of sight. As he put it, after a while “the star tends to close itself off from a communication with a distant observer; only its gravitational field persists.”
“Stars had until then been a bit of a mystery. For a start, no one had a clear idea of how they could emit such copious amounts of energy. It was Eddington who came up with a plausible mechanism for how stars are fueled. To understand his idea, we need to take a close look at the simplest atoms. A hydrogen atom is made up of two particles, a proton (which is positively charged) and an electron (which is negatively charged). The proton and electron are held together by electromagnetic force, which causes opposite charged to attract one another. The proton is approximately two thousand times heavier than the electron and so makes up almost all the weight of the hydrogen atom.”
“If most of the sun started in the form of hydrogen, it should be able to burn for almost 9 billion years before its conversion into helium is complete. Given that the Earth is currently about 4.5 billion years old, the numbers seem to add up.”
“After proposing a source for stars’ energy, he explained why they didn’t collapse: they could withstand the pull of gravity by radiating all the energy they produced outward.”
“Quantum physics divided nature into its smallest constituents and put it back together in an outlandish way. It emerged from the bizarre phenomena that were being observed in the nineteenth century when physicists discovered that compounds and chemicals reemit or absorb light in a peculiar fashion.”
“The most notorious result to come out of the new quantum physics was the uncertainty principle. In classical Newtonian physics, objects move in a predictable way in response to outside forces. Once you know the exact positions and velocities of a systems’ constituents and any forces on the system, you can predict all the systems’ future configurations. Prediction becomes particularly easy; all you need to know is each particle’s position in space and the direction and magnitude of its velocity. But in that new quantum theory it was impossible to know both the position and the velocity of a particle with perfect accuracy. A particularly persistent and stubborn experimenter in a lab who tires to pin down the position of a particle with perfect precision will have absolutely no idea what its velocity is.”
“Quantum physics brought uncertainty and randomness into the heart of physics. It was precisely this randomness that could be put to use in solving the problem of white dwarfs.”
“The Manhattan project focused its resources on producing the first atomic bomb, and in just under three years they had achieved their goal. When the two atomic bombs, Little Boy and Fat Man, were dropped in Hiroshima and Nagasaki in August of 1945, around two hundred thousand people were killed.”
“Einstein’s last years were shadowed by illness. In 1948 he was diagnosed with a potentially fatal aneurysm of the abdominal aorta. The aneurysm grow slowly over the years, and Einstein prepared himself for the inevitable. In mid-April, his aneurysm finally burst, and after a few days in the hospital, Einstein died.”
“It had been apparent from the moment Hubble made his groundbreaking measurement. Hubble found that the expansion rate of the universe was approximately 500 kilometers per second per megaparsec. This meant that a galaxy that was about a megaparsec distant from us (roughly 3 million light-years) would be speeding away from us at about 500 kilometers per second. From this number, now know as the Hubble constant, it was possible to use Friedman’s and Lemaitre’s models for the evolution of the universe, wind back the clock, and figure out the exact moment in time when the universe came into being. And by doing this it was possible to work out that the universe was about a billion years old.”
“Radio waves behave just like light waves, but their wavelengths are a billion times longer than those of visible light. The light we can actually see, which makes up the bulk of the sun’s rays, has a wavelength that is less than a millionth of a meter. Radio waves have gigantic wavelengths, ranging from a millimeter all the way up to hundreds of meters.”
“There was something of Einstein is the young Hawking, and indeed his childhood friends would often call him that. He hadn’t shone at school, and if anything, he had been relaxed, playful, and naughty, a slight, untidy boy who delighted in entertaining his colleagues. Hawking has become increasingly interested in science and, on applying to Oxford, had aced the entrance exam and interview. He found Oxford ridiculously easy and had done well enough to impress his tutors and lecturers. It was a Cambridge as a PhD student, under Sciama’s tutelage, that Hawking would be steered toward the cosmos and, finding his scientific voice, would spell out one significant consequence of Penzias and Wilson’s discovery.”
“The equations for quantum physics tells us how the quantum state of a system, such as an electron bound to a proton in a hydrogen atom, evolves with time. It makes a very clear distinction between space and time. Einstein’s special relativity brings space and time together into one indivisible thing – spacetime. It also combines the laws of mechanics and the laws of light into a coherent framework.”
“Particles in the universe can be divided into two types – fermions and bosons. As a rule of thumb, the particles that make up stuff are mostly fermions, and the particles that carry the forces of nature are mostly bosons. Fermions include the building blocks of atoms, such as electrons, protons, and neutrons.”
“The combination of the electroweak and strong theories became known as the standard model and made accurate predictions that were confirmed in laboratories like the gigantic particle accelerator at CERN in Geneva, Switzerland. This almost completely unified, yet powerful and predictive quantum theory of the three forces – electromagnetic, weak, and strong – was universally accepted.”
“Hawking’s calculation was able to show that the temperature with which a black hole shines is inversely proportional to its mass. So, for example, a black hole with a mass of the sun would have the temperature of a billionth of a Kelvin, and a black hole with the mass of the moon would have a temperature of about 6 degrees Kelvin. As the black hole shines, it sheds some of its mass. This process happens incredibly slowly. A black hole with the mass of the sun would take an inordinate long time to shed all its mass, or evaporate, as Hawking described it. But much smaller black holes could evaporate much more quickly.”
“Unlike electromagnetic waves, gravitational waves have proved incredibly difficult to find. They are very inefficient at carrying energy out of a gravitating system. As the Earth orbits around the sun at a distance of 150 million kilometers, it slowly loses energy through gravitational waves and drifts closer to the sun, but the distance between the Earth and the sun shrinks at a minuscule rate, about the width of a proton per day. This means that during its whole lifetime, the Earth will drift closer to the sun by a mere millimeter.”
“In fact, a large fraction of the universe appeared to be in the form of exotic substances we had never seen in a laboratory. Dubbed ‘dark matter’ and ‘dark energy,’ they were out there, affecting spacetime, yet strangely elusive and undetectable. The case for a dark universe emerged forcefully one afternoon when the large-scale structure of the universe was discussed. It was that one topic that had drawn me into cosmology in the first place.”
“The new model of the universe contained a cocktail of atoms, cold dark matter, and a cosmological constant. It was the universe that large-scale structure had been hinting at for a decade but that hardly anyone had been ready to embrace.”
“The cosmological constant was now universally accepted. The fundamental problem remained: the gross inconsistency with what Zel’dovich had predicted from adding up the energy of the virtual particles in the universe and the value that was actually observed, a mismatch of over a hundred orders of magnitude.”
“Stephen Hawking was offered the Lucasian Professorship of Mathematical Physics at Cambridge in 1979. One of the most prestigious chairs in theoretical physics in the world, it has been held by Isaac Newton and Paul Dirac and was now being offered to a realavist not yet in his forties.”
“Supersymmetry imagines a deep symmetry in nature that inextricably links all the particles and forces in the universe. Each elementary particle is suppose to have an invest twin: for every fermion there is a twin boson and vice versa. A theory first proposed in 1976 took supersymmetry one step further and mirrored spacetime itself, creating supergravity.”
“The talk addressed the hallowed belief in physics that given complete information about a physical system, it should always be possible to reconstruct the systems past. Imagine a flying ball by your head. If you know how fast it was moving and its direction of flight, it would be possible for you to reconstruct exactly where it came form and what it passed along the way. Or take a box filled with gas molecules. If you could measure the positions and velocities of every molecule of gas in the box, it would be possible to determine where every particle had been at any moment in the past.”
“In fact strong theory started off as a cottage industry in the late 1960s, trying to explain the behaviour of the whole zoo of exotic new particles that were appearing in particle accelerators experiments. The basic idea is that these particles, time pointlike objects, were better described in terms of microscopic, wiggly pieces of string. Particles with different masses would be nothing more than different vibrations of minute strings that floated around through space. The trick is that only one such object, one string, could describe all the particles. The more a strong wiggled, the more energetic it was and the heavier the particle it would describe. It was unification of sorts, but in a completely different way from what had ever been proposed.”
“A rough estimate let to the possible existence of 10 to the exponent of 500 solutions for each version of string theory, a truly obscure panorama of possible universes that became known as the landscape. String theory remained unable to make unique predictions.”
“Daniel Friedan, a prominent string theorist is the first string revolution of the 1980s, acknowledge sting theory’s shortcomings. As Friedan admits, the long-standing crisis of string theory is its complete failure to explain or predict any large distance physics…String theory cannot give any definite explanations of existing knowledge of the real world and cannot make and definite predictions. The reliability of string theory cannot be evaluated, much less established. String theory has no credibility as a candidate theory of physics. These skeptics remained in the minority and were easily drowned out. If you were to enter the field of quantum gravity in the 1980s or 1990s, you might be forgiven if you thought that the covariant approach had won and string theory was all there was.”
“If fact we have a gigantic black hole sitting right in the middle of our galaxy, the Milky Way. It weights about a hundred million times more than the sun and has a radius of about 10 million kilometers. And just like the Milky Way, all other galaxies should have black holes firmly in their centers like massive engines surrounded by gargantuan spirals of stars.”
“A grander possibility is that spacetime is much vaster than we previously envisioned and our universe is only one of countless universes that together make up the multiverse. All other multiverse, universes are breaking out into existence, growing to cosmic proportions, each one at its own pace and made up its own particular way. If we follow back the existence of our own universe, we find that it is embedded like a pustule in a much wider spacetime that has existed for all eternity. The multiverse is a wild, immense realm of what is ultimately stasis: a steady state of creation and destruction.”