第1章
Unlocking the Cosmos: Hawking's Final Reflections on Existence
Stephen Hawking's voice resonates beyond his physical departure, continuing to shape our understanding of the universe's greatest mysteries. "Brief Answers to the Big Questions" represents his final intellectual gift to humanity-a culmination of his lifelong quest to understand the cosmos. Completed after his death with help from colleagues and family, this remarkable work distills complex physics into accessible wisdom for everyone. What makes this book extraordinary isn't just its scientific insights, but how it captures Hawking's indomitable spirit. Despite being trapped in a failing body, his mind soared freely across the universe. The book has become a cultural touchstone, praised by figures from Barack Obama to Elon Musk, and continues to inspire millions worldwide. As Eddie Redmayne, who portrayed Hawking in "The Theory of Everything," noted: "He possessed the most beautiful mind, the sharpest wit, and the funniest sense of humor I've ever encountered."
第2章
The Cosmic Questioner: Hawking's Intellectual Journey
Stephen Hawking's life embodied the power of human curiosity against overwhelming odds. Born exactly 300 years after Galileo's death, Hawking's early fascination with how things worked foreshadowed his extraordinary scientific career. As a youth in London during WWII, he explored bomb sites with friends, driven by the same curiosity that would later propel him to probe the universe's deepest secrets.
His academic journey began unremarkably at Oxford, where he initially adopted the prevailing anti-work attitude. Everything changed when, at age 21, he was diagnosed with ALS and given just two years to live. This devastating news transformed his approach to life and work: "Before my condition was diagnosed, I had been very bored with life. There had not seemed to be anything worth doing. But shortly after I came out of the hospital, I dreamed that I was going to be executed. I suddenly realized there were a lot of worthwhile things I could do if I were reprieved."
This newfound purpose drove Hawking to complete his PhD and make groundbreaking discoveries about black holes and the universe's origins. In 1970, his eureka moment came when he realized he could apply causal structure theory to black holes, showing that their event horizon area always increases-a discovery that would lead to his most significant breakthrough: Hawking radiation, the thermal emission from black holes that confirmed the relationship between a black hole's area and its entropy.
Despite losing his ability to speak after life-threatening pneumonia in 1985, technology allowed him to continue communicating his revolutionary ideas. His 1988 book "A Brief History of Time" became an unexpected global phenomenon, selling over 10 million copies and bringing complex cosmology into millions of homes worldwide.
Throughout his extraordinary life, Hawking traveled the universe through his mind while experiencing life's full spectrum on Earth. His ability to understand the laws governing the universe represented humanity's triumph of intellect over adversity. As he reflected near the end of his life: "I have led an extraordinary life on this planet, while at the same time traveling across the universe by using my mind and the laws of physics."
第3章
The God Question: Science and the Origins of Everything
Science increasingly answers questions that once belonged exclusively to religion. Throughout history, humans created supernatural beings to explain frightening natural phenomena-even the fierce Vikings invented gods to make sense of lightning, storms, and eclipses. Today, science provides better explanations, though many still find comfort in religious frameworks.
When The Times ran a headline "Hawking: God did Not Create Universe," they misrepresented Hawking's work. "I have no desire to tell anyone what to believe," he clarifies, "but for me, asking if God exists is a valid question for scientists to consider." His goal wasn't to disprove God but to find a rational framework for understanding our universe.
For centuries, disabilities like Hawking's were considered divine curses. He preferred believing everything could be explained through natural laws: "You could define God as the embodiment of the laws of nature. However, this would be a kind of God that would have no interest in human affairs, or in right or wrong."
The discovery of natural laws has been humanity's greatest achievement. These laws are universal and unchangeable, applying equally to tennis balls and planets. This creates a philosophical tension with traditional religion-if natural laws are fixed, what role remains for God? While Einstein used "God" impersonally to refer to these laws, most people envision a human-like being with whom they can have a relationship.
Science is making progress on understanding the universe's origin-the last domain religion traditionally claims. Hawking believed the universe was spontaneously created from nothing according to scientific laws: "To make a universe requires just three ingredients: matter, energy, and space." Or really just two, since Einstein showed matter and energy are interchangeable. The Big Bang created both energy and space simultaneously, with positive energy perfectly balanced by negative energy stored in space itself, making the universe "the ultimate free lunch."
Quantum mechanics explains how something can appear from nothing, as particles do at the subatomic level. Most importantly, time itself began at the Big Bang-there was no "before" for a creator to exist in. This is similar to how time stops inside black holes. Without time, there can be no cause, making the question of God's role in creation meaningless-like asking for directions to the edge of a spherical Earth.
"I believe the simplest explanation is there is no God," Hawking concludes. "No one created the universe and no one directs our fate. This leads me to a profound realization: there is probably no heaven and no afterlife either. I think belief in an afterlife is just wishful thinking. There is nothing beyond the moment when the brain flickers for the final time."
第4章
Cosmic Origins: How Everything Began
Can our finite minds comprehend an infinite universe? Despite the risk of hubris, Hawking believed we can and should try. We've made remarkable progress already and may not be far from a complete picture of cosmic origins.
Different cultures have created various creation myths-like the Boshongo people who believed their god Bumba vomited up the sun, moon, stars, animals, and finally humans. But science offers a more compelling explanation based on natural laws rather than divine intervention.
Not everyone agreed the universe had a beginning. Aristotle believed in an eternal universe, considering it more perfect than something created. The question troubled philosopher Immanuel Kant, who saw logical contradictions either way-why would an eternal universe suddenly begin, or why would an infinite universe take so long to reach its present state?
Einstein's general relativity revolutionized our understanding by showing space and time are dynamic quantities shaped by matter and energy. This made it meaningless to ask what happened "before" the universe began-like asking what's south of the South Pole.
Observations revealed the universe is expanding, with galaxies moving away from each other. Tracing this expansion backward suggests everything originated from a single point 13.8 billion years ago. Despite attempts to avoid this conclusion through theories like the "steady-state" model, mathematical theorems proved the universe must have had a beginning-a singularity where general relativity breaks down.
The discovery of cosmic microwave background radiation in 1965 provided strong evidence for this hot, dense beginning. Understanding this origin requires combining Einstein's relativity with quantum uncertainty, suggesting the universe has multiple possible histories, each with its own probability.
Hawking's work with Jim Hartle led to the "no-boundary proposal," suggesting the universe has no boundary in space-time. The beginning of the universe wouldn't be a singularity but smoothly rounded, like the Earth's surface at the North Pole. This eliminates the need for initial conditions, as the universe would contain every possible history. The laws of physics would determine which histories are most probable, with our universe being among the likely ones.
"So what happened before the Big Bang?" Hawking asks. "The answer is that there was no time before the Big Bang. Time began at the Big Bang. The point is that the Big Bang is a beginning of space and time, not something that happened within space and time."
第5章
The Cosmic Community: Searching for Other Intelligence
Are we alone in the universe? This question has fascinated humanity for centuries, and Hawking approached it with scientific rigor while acknowledging its profound implications.
The Anthropic Principle cautions against assuming the universe was designed for humans-we must exist in a universe capable of producing us, or we wouldn't be here to observe it. Rather than adopting the Strong version (positing multiple universes), Hawking used the Weak Anthropic Principle, taking physical constants as given while examining what life's existence tells us about universal history.
Our universe began without carbon, consisting primarily of hydrogen and helium. As it cooled, gravity caused denser regions to collapse into galaxies and stars about two billion years after the Big Bang. Massive early stars produced heavier elements like carbon and oxygen, then scattered them through supernovae explosions, providing materials for later stars and planets.
We've discovered thousands of planets orbiting distant stars using light fluctuation measurements and detecting stellar wobbles. Approximately one star in five has an Earth-like planet at a distance compatible with life. Our solar system formed about 4.5 billion years ago from gas containing remnants of earlier stars, with Earth composed largely of heavier elements.
The evolution of life on Earth shows remarkable acceleration over time. Life appeared relatively quickly after Earth became habitable, but intelligence may not be an inevitable evolutionary outcome. Evolution is likely a random process with intelligence as just one possible result.
Intelligence might not even have long-term survival value. Single-cell organisms could outlast all other life forms if catastrophe strikes. The development of intelligence took an extraordinarily long time-two and a half billion years from single cells to multi-cellular organisms-suggesting the probability of intelligent life evolving may be low.
Asteroid impacts present another barrier to intelligence evolving. The collision that wiped out dinosaurs 66 million years ago would have eliminated any human-sized creatures. Earth may have been unusually lucky to avoid major collisions long enough for intelligence to develop.
A fourth possibility is that intelligent extraterrestrial life exists but has overlooked us. The Breakthrough Listen Initiative represents our most comprehensive search for such civilizations, though we should be cautious about responding to any signals. As Hawking notes, "Meeting a more advanced civilization, at our present stage, might be a bit like the original inhabitants of America meeting Columbus-and I don't think they thought they were better off for it."
第6章
The Limits of Prediction: Quantum Uncertainty and the Future
The ancient world seemed chaotic and arbitrary, with natural disasters attributed to capricious gods. Gradually, people recognized patterns in nature, particularly in astronomy, leading to scientific determinism. Pierre-Simon Laplace articulated this view: if we knew the positions and speeds of all particles at one time, we could calculate their behavior at any other time.
This deterministic vision dominated 19th century science but collapsed in the 20th century due to two developments. First, quantum mechanics revealed that particles don't have precisely defined positions and speeds simultaneously-Heisenberg's Uncertainty Principle shows that measuring one property more accurately makes the other less certain.
Einstein resisted this apparent randomness, believing in an underlying deterministic reality ("God does not play dice"). But John Bell's experimental test disproved such "hidden variable" theories, suggesting even God is bound by uncertainty.
The second challenge came from quantum mechanics itself. Rather than predicting precise positions and speeds, it can only predict a particle's "wave function"-a probability distribution. This preserves a limited form of determinism through the Schrodinger equation, but we can predict only half of what classical physics claimed possible.
Black holes introduce further unpredictability since we cannot observe particles inside them. Thus, Laplace's perfect predictability has been significantly constrained-while physical laws theoretically allow future prediction, the calculations are often practically impossible.
"Even if we find a complete unified theory," Hawking explains, "it would not mean that we would be able to predict events in general, for two reasons. The first is the limitation that the uncertainty principle of quantum mechanics sets on our powers of prediction. There is nothing we can do to get around that. In practice, however, this first limitation is less restrictive than the second one. It arises from the fact that we could not solve the equations of the theory exactly, except in very simple situations."
This inherent unpredictability extends to human behavior. While our actions are determined by physical laws governing brain chemistry, these processes are so complex that we cannot predict them in practice. This gives us the effective freedom to make choices, even if these choices are technically predetermined by physics.
"So although we are mere collections of fundamental particles of nature, we human beings are able to change our universe," Hawking concludes. This apparent paradox-deterministic laws creating the illusion of free will-allows us to shape our future while being bound by physical reality.
第7章
Into the Abyss: The Mystery of Black Holes
Black holes represent scientific fact stranger than fiction. First discussed in 1783 by Cambridge scholar John Michell, they were conceived as "dark stars" so massive that their escape velocity exceeds the speed of light, making them invisible. Einstein's general theory of relativity describes gravity as a feature of space and time, and despite initially resisting the idea of gravitational collapse, science eventually recognized that massive stars could collapse under their own gravity to form objects with event horizons from which nothing, not even light, can escape.
Black holes have remarkable properties: they have no "hair"-meaning whatever forms them, they look identical from outside. Their boundary, the event horizon, marks the point of no return where gravity prevents even light from escaping. Falling into a small black hole would stretch you into "spaghetti," while larger ones with millions of solar masses would allow passage through the horizon without such dramatic effects. To outside observers, someone falling in would appear to slow down and hover at the horizon, gradually fading from view as their image becomes dimmer and redder.
Hawking's eureka moment came shortly after his daughter Lucy's birth when he discovered the area theorem: the surface area of a black hole's event horizon always increases when matter or radiation falls in, and when two black holes merge, the resulting horizon area exceeds the sum of the original areas. This property suggests a resemblance between event horizon area and entropy in thermodynamics-a measure of disorder or lack of knowledge about a system.
In early 1974, Hawking made his most famous discovery: quantum mechanics predicts black holes emit particles at a steady rate with a precisely thermal spectrum. This radiation occurs when virtual particle-antiparticle pairs form near the horizon-a quantum effect where particles briefly materialize from vacuum energy. If one particle falls into the hole while its partner escapes, the escaping particle appears as radiation emitted by the black hole.
As particles escape from a black hole, the hole loses mass and shrinks, accelerating the emission process until it eventually disappears completely. This raises a profound question: what happens to all the information about particles that fell in? The emitted particles seem completely random, suggesting information is lost except for total mass and rotation. This apparent information loss challenges scientific determinism-our belief that laws of science determine the universe's evolution.
The information paradox has troubled scientists for forty years as one of theoretical physics' greatest unsolved problems. Recent breakthroughs in unifying gravity and quantum mechanics have revived interest in resolving this paradox through understanding space-time symmetries. Working with Malcolm Perry and Andy Strominger in 2016, Hawking found that black holes carry "supertranslation" charges that might encode information about their contents. With Sasha Haco, they discovered that "superrotation" charges can account for a black hole's entire entropy, suggesting information is stored on the horizon rather than lost.
"Although the information paradox remains unresolved," Hawking concluded, "I'm optimistic we're moving toward a solution where quantum mechanics holds and information is preserved."
第8章
Bending Reality: The Possibility of Time Travel
In science fiction, space and time warps enable rapid galactic travel or time travel, but how realistic are these concepts? The idea that space and time can be curved is relatively recent. For over 2,000 years, Euclidean geometry with its straight lines and triangles summing to 180 degrees was considered absolute truth. However, on curved surfaces like Earth, triangles can sum to more than 180 degrees. Just as two-dimensional beings on Earth's surface would experience curved space without perceiving the third dimension, our three-dimensional space could be curved in higher dimensions.
Einstein's 1905 special relativity theory showed that space and time are intimately connected, forming a four-dimensional entity called space-time. Each point in space-time is labeled by four numbers-three for spatial position and one for time. The faster observers move relative to each other, the more their time measurements disagree. While this suggests the possibility of traveling faster than light to move backward in time, Einstein showed that accelerating a spaceship to light speed would require infinite power, making this approach impossible.
His 1915 general relativity theory demonstrated that space-time is warped by matter and energy, an effect we can observe in the slight bending of light passing near the Sun. While our solar system has weak gravitational fields, strong fields exist in phenomena like black holes. In 1948, Kurt Godel found a solution to Einstein's equations representing a rotating universe where time travel would be possible, which troubled Einstein greatly.
To travel rapidly across the galaxy would require warping space-time to create a wormhole-a tube connecting distant parts of space that would act as a shortcut. Such wormholes could potentially allow time travel if their endpoints were moving relative to each other. Creating a wormhole requires matter with negative mass and energy density to warp space-time in the opposite way that normal matter does. While classical physics forbids negative energy, quantum theory is more permissive. The Uncertainty Principle allows for "vacuum fluctuations"-virtual particle-antiparticle pairs that appear and annihilate each other.
If time travel were possible, why haven't visitors from the future appeared? One explanation might be that we can only warp space-time in the future, not the past we've already observed. But paradoxes would remain, like preventing your own departure by destroying your rocket before launch. Hawking proposed a "Chronology Protection Conjecture"-that the laws of physics prevent macroscopic time travel because the probability of histories with sufficient space-time warping is extremely low due to the energy of virtual particles becoming immense.
In 2009, Hawking tested time travel by hosting a party announced only after it occurred-no one came, supporting his conclusion that positive energy density prevents time travel under general relativity. "I sat there a long time," he recalled, "but no one came. I was not really expecting anyone to show up. It would have been a bit difficult for them to make their way home afterward. But I gave the invitation just in case."
第9章
Earth's Crossroads: Existential Threats and Human Survival
In January 2018, the Bulletin of the Atomic Scientists moved their Doomsday Clock to two minutes to midnight, closer to catastrophe than at any time since the early 1950s. This alarming warning reflects our politically unstable world where many feel economically and socially abandoned, turning to populist politicians whose crisis management remains untested. Earth faces numerous existential threats that remain unsolved despite being solvable.
Our planet is becoming too small for us as physical resources drain at an alarming rate. We've inflicted climate change upon Earth, alongside rising temperatures, melting polar ice, deforestation, overpopulation, disease, war, famine, water scarcity, and species decimation. Global warming, caused by our collective desire for cars, travel and improved living standards, may become self-sustaining through feedback loops like melting ice caps reducing solar reflection and rainforest die-off eliminating carbon dioxide removal. Without action beyond the Kyoto Protocol, Earth could eventually resemble Venus-250C with sulphuric acid rain, making human life impossible.
The universe is inherently violent-stars engulf planets, supernovae emit lethal radiation, black holes collide, and asteroids hurtle through space at hundreds of miles per second. An asteroid collision represents a threat against which we have no defense. The last major impact, approximately 66 million years ago, likely killed the dinosaurs, and physics guarantees such events will recur.
Nuclear war remains humanity's greatest immediate threat-a danger we've somewhat forgotten. Though Russia and America are less trigger-happy now, accidents or terrorist acquisition of nuclear weapons remain possibilities. The risk increases as more nations obtain nuclear capabilities. Even after the Cold War, stockpiles remain sufficient to destroy humanity multiple times over.
Hawking considered it almost inevitable that nuclear confrontation or environmental catastrophe will cripple Earth within the next 1,000 years-a mere blink in geological time. By then, he hoped our ingenious species will have escaped Earth's bonds and survived, though millions of other species may not. Historically, humans facing crises found new territories to colonize, but now there's no new world left on Earth. We must venture to other worlds, rekindling the excitement of 1960s space travel. Spreading beyond Earth may be our only salvation from self-destruction.
"I believe that life on Earth is at an ever-increasing risk of being wiped out by a disaster such as sudden global warming, nuclear war, a genetically engineered virus, or other dangers," Hawking warned. "I think the human race has no future if it doesn't go into space."
第10章
Beyond Earth: The Case for Space Colonization
Not exploring space would be like castaways refusing to leave a desert island. Though space exploration won't solve our immediate earthly problems, it will provide perspective and potentially unite humanity toward common challenges. With just a quarter percent of world GDP-far less than the 0.3% NASA received during the Apollo era-we could establish a Moon base within thirty years and reach Mars within fifty.
For humans to exist away from Earth long-term, we need planetary or lunar bases rather than zero gravity stations. The Moon offers our closest option with polar ice for resources. Mars is another target, despite losing its atmosphere billions of years ago. Beyond our solar system, observations suggest many stars have planets. If just 1% of the thousand stars within thirty light years have Earth-sized planets in habitable zones, we'd have ten candidate new worlds, including Proxima b, which shows similarities to Earth despite being 4.5 light years away.
Interstellar travel seems impossible with current technology-chemical rockets would take three million years to reach Alpha Centauri. But imagination offers solutions. In 2016, Hawking joined Yuri Milner to launch Breakthrough Starshot, aiming to send probes to Alpha Centauri within our lifetime.
The concept uses miniaturized "Star Chip" spacecraft attached to light sails, propelled by powerful ground-based lasers to one-fifth light speed (100 million mph). These nanocraft could reach Mars in under an hour and Alpha Centauri in just twenty years, potentially flying by Proxima b and sending data back to Earth.
Major engineering challenges remain: the craft must survive extreme acceleration, cold, vacuum, and space dust collisions. Focusing gigawatt lasers through atmospheric turbulence presents difficulties. But these are engineering problems that can eventually be solved, opening a pathway to interstellar exploration and potentially discovering habitable worlds.
Human colonization on other planets is transitioning from science fiction to science fact. If humanity is to continue for another million years, our future lies in boldly going where no one has gone before. Within a hundred years, we may travel anywhere in our solar system, though reaching the stars will take longer-perhaps 500 years before we've visited nearby stars.
"I believe that the long-term future of the human race must be in space," Hawking insisted. "It will be difficult enough to avoid disaster on planet Earth in the next hundred years, let alone the next thousand, or million. The human race shouldn't have all its eggs in one basket, or on one planet. Let's hope we can avoid dropping the basket until we have spread the load."
第11章
The Rise of Machines: Artificial Intelligence and Human Destiny
Intelligence defines humanity-everything in civilization stems from it. Our universe has awakened, becoming aware of itself through conscious life forms. Hawking believed there's no fundamental difference between how an earthworm's brain works and computer computation, nor between earthworm and human brains except by degree. Therefore, computers can emulate or exceed human intelligence.
If computers continue following Moore's Law, doubling speed and memory every eighteen months, they'll likely surpass human intelligence within a century. When AI can improve itself without human help, we may face an intelligence explosion producing machines smarter than us by more than we exceed snails. Recent AI integration with machine learning, statistics, and other fields has yielded remarkable successes in speech recognition, autonomous vehicles, and more.
The potential benefits are enormous-possibly eradicating disease and poverty. But success in creating AI could be humanity's last achievement unless we manage the risks. While Hawking was known as an optimist, he worried AI could develop conflicting goals and redesign itself at accelerating rates that humans, limited by biological evolution, couldn't match.
In the near term, militaries are considering autonomous weapon systems that select and eliminate targets independently. Medium-term, AI may automate jobs, potentially bringing prosperity and equality. Long-term, there are no fundamental limits to AI's capabilities. An "intelligence explosion" could occur as super-intelligent machines repeatedly improve themselves, potentially outsmarting financial markets, researchers, and leaders.
The advent of super-intelligent AI would be either humanity's greatest achievement or worst catastrophe. The real risk isn't malice but competence-a super-intelligent AI pursuing goals misaligned with ours would be devastating. We should plan ahead rather than waiting until it arrives.
Hawking joined Elon Musk and AI experts in calling for serious research into AI's societal impact. Through the Future of Life Institute, they worked to mitigate risks while reaping AI's benefits. The Leverhulme Centre for the Future of Intelligence in Cambridge is tackling open-ended questions raised by AI development. We need AI that can be controlled, potentially even reversing environmental damage from industrialization.
Unlike fire, where we could invent extinguishers after mistakes, powerful technologies like AI require getting things right the first time. Our future is a race between technological power and the wisdom with which we use it. Let's ensure wisdom wins.
"We stand on the threshold of a brave new world," Hawking concluded. "It is an exciting, if precarious, place to be and we are the pioneers. When we invented fire, we messed up repeatedly, then invented the fire extinguisher. With more powerful technologies such as nuclear weapons, synthetic biology and strong artificial intelligence, we should instead plan ahead and aim to get things right the first time, because it may be the only chance we will get."
第12章
Shaping Tomorrow: Education, Science, and Human Potential
A century after Einstein revolutionized our understanding of the universe through imagination and thought experiments, we have greater tools for discovery, yet imagination remains our most powerful attribute. Human minds need the spark of inquiry and wonder, often ignited by exceptional teachers. Hawking's teacher Dikran Tahta showed him mathematics as the universe's blueprint when he was fourteen. Unfortunately, education and scientific research face funding cuts while Brexit and Trump represent a global revolt against experts, including scientists.
Humanity faces numerous challenges: global warming, population growth, species extinction, renewable energy needs, ocean degradation, deforestation, and epidemic diseases. Yet the future also holds revolutionary inventions that will transform how we live, work, and travel-from mining the Moon to establishing Mars outposts and finding medical cures.
Hawking saw two options for humanity's future: space exploration for alternative habitable planets and the positive use of artificial intelligence. Earth is becoming too small for us, with dwindling resources, climate change, pollution, melting polar ice, deforestation, and species decimation. Our population growth cannot continue at its current rate into the next millennium.
Nuclear war presents another existential threat-perhaps explaining why we haven't been contacted by extraterrestrials. When civilizations reach our development stage, they may become unstable and self-destruct. We now possess the technological power to destroy all life on Earth. Moving into space could help us avoid this potential Armageddon.
Scientific literacy is no longer optional. While not everyone should become scientists, all young people must be familiar with and confident around scientific subjects. A world where only a tiny super-elite understands advanced science would be dangerous and limited. Beneficial projects like cleaning oceans or curing diseases in developing countries might not receive priority, and technology could be used against us with no way to stop it.
Hawking didn't believe in boundaries for what we can accomplish. We stand at the threshold of important discoveries in all areas of science. In the next fifty years, we'll understand the Big Bang, how life began on Earth, and possibly discover life elsewhere. Through scientific endeavor and technological innovation, we'll create viable habitats on other planets and learn to exist in space. This is just the beginning of billions of years of life flourishing in the cosmos.
His final message resonates with hope and challenge: "Remember to look up at the stars and not down at your feet. Try to make sense of what you see and wonder about what makes the universe exist. Be curious. However difficult life may seem, there is always something you can do and succeed at. It matters that you don't just give up. Unleash your imagination. Shape the future."
