Jamal Awil

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A Brief History of Time cover

A Brief History of Time

Author
Hawking, Stephen
Highlights
44
Responses
0
First Highlight
Jul 25, 2026
Last Highlight
Jul 25, 2026

A good theory is characterized by the fact that. [fact]

As philosopher of science Karl Popper has emphasized, a good theory is characterized by the fact that it makes a number of predictions that could in principle be disproved or falsified by observation.

Hawking, Stephen, A Brief History of Time, loc. 32

It can in fact never reach the speed. [contrarian]

It can in fact never reach the speed of light, because by then its mass would have become infinite, and by the equivalence of mass and energy, it would have taken an infinite amount of energy to get it there.

Hawking, Stephen, A Brief History of Time, loc. 53

Einstein made the revolutionary suggestion that gravity. [fact]

Einstein made the revolutionary suggestion that gravity is not a force like other forces, but is a consequence of the fact that space-time is not flat, as had been previously assumed: it is curved, or “warped,” by the distribution of mass and energy in it.

Hawking, Stephen, A Brief History of Time, loc. 65

Or a force acts, it affects the. [fact]

when a body moves, or a force acts, it affects the curvature of space and time—and in turn the structure of space-time affects the way in which bodies move and forces act.

Hawking, Stephen, A Brief History of Time, loc. 72

The singularity theorems really show is that there must. [fact]

the singularity theorems really show is that there must have been a time in the very early universe when the universe was so small that one could no longer ignore the small-scale effects of the other great partial theory of the twentieth century, quantum mechanics.

Hawking, Stephen, A Brief History of Time, loc. 101

On the other hand. [fact]

The basic idea of GUTs is as follows: as was mentioned above, the strong nuclear force gets weaker at high energies. On the other hand, the electromagnetic and weak forces, which are not asymptotically free, get stronger at high energies. At some very high energy, called the grand unification energy, these three forces would all have the same strength and so could just be different aspects of a single force.

Hawking, Stephen, A Brief History of Time, loc. 133

Thus our very existence could be regarded as. [fact]

Thus our very existence could be regarded as a confirmation of grand unified theories, though a qualitative one only; the uncertainties are such that one cannot predict the numbers of quarks that will be left after the annihilation, or even whether it would be quarks or antiquarks that would remain.

Hawking, Stephen, A Brief History of Time, loc. 143

In some cases they may explode or manage. [fact]

In some cases they may explode or manage to throw off enough matter to reduce their mass below the limit and so avoid catastrophic gravitational collapse, but it was difficult to believe that this always happened, no matter how big the star.

Hawking, Stephen, A Brief History of Time, loc. 153

For example, observations with the Hubble telescope. [fact]

For example, observations with the Hubble telescope of the galaxy known as M87 reveal that it contains a disk of gas 130 light-years across rotating about a central object two thousand million times the mass of the sun.

Hawking, Stephen, A Brief History of Time, loc. 173

It would just BE. [fact]

The universe would be completely self-contained and not affected by anything outside itself. It would neither be created nor destroyed. It would just BE.

Hawking, Stephen, A Brief History of Time, loc. 238

I realized that I had made a mistake. [fact]

I realized that I had made a mistake: the no boundary condition implied that disorder would in fact continue to increase during the contraction.

Hawking, Stephen, A Brief History of Time, loc. 268

In other words, quantum theory allows the energy density. [fact]

In other words, quantum theory allows the energy density to be negative in some places, provided that this is made up for by positive energy densities in other places, so that the total energy remains positive.

Hawking, Stephen, A Brief History of Time, loc. 290

According to this viewpoint. [fact]

According to this viewpoint, you could not go back in time unless history showed that you had already arrived in the past and, while there, had not killed your great-great-grandfather or committed any other acts that would conflict with your current situation in the present.

Hawking, Stephen, A Brief History of Time, loc. 297

Of course, extra space-time dimensions are a commonplace. [fact]

Of course, extra space-time dimensions are a commonplace of science fiction indeed, they provide an ideal way of overcoming the normal restriction of general relativity that one cannot travel faster than light or back in time (see Chapter 10).

Hawking, Stephen, A Brief History of Time, loc. 317

Ten million million million GeV (1 followed by nineteen. [fact]

If one had a particle with an energy above what is called the Planck energy, ten million million million GeV (1 followed by nineteen zeros), its mass would be so concentrated that it would cut itself off from the rest of the universe and form a little black hole.

Hawking, Stephen, A Brief History of Time, loc. 328

But even before the first atomic bomb. [fact]

But even before the first atomic bomb had been detonated, he was publicly warning of the dangers of nuclear war and proposing international control of nuclear weaponry.

Hawking, Stephen, A Brief History of Time, loc. 347

Galileo, perhaps more than any other single person. [fact]

Galileo, perhaps more than any other single person, was responsible for the birth of modern science. His renowned conflict with the Catholic Church was central to his philosophy, for Galileo was one of the first to argue that man could hope to understand how the world works, and, moreover, that we could do this by observing the real world.

Hawking, Stephen, A Brief History of Time, loc. 349