Uh-oh, it looks like your Internet Explorer is out of date.

For a better shopping experience, please upgrade now.

Reinventing Gravity: A Physicist Goes Beyond Einstein

Reinventing Gravity: A Physicist Goes Beyond Einstein

by John W. Moffat

See All Formats & Editions

Einstein's gravity theory—his general theory of relativity—has served as the basis for a series of astonishing cosmological discoveries. But what if, nonetheless, Einstein got it wrong?

Since the 1930s, physicists have noticed an alarming discrepancy between the universe as we see it and the universe that Einstein's theory


Einstein's gravity theory—his general theory of relativity—has served as the basis for a series of astonishing cosmological discoveries. But what if, nonetheless, Einstein got it wrong?

Since the 1930s, physicists have noticed an alarming discrepancy between the universe as we see it and the universe that Einstein's theory of relativity predicts. There just doesn't seem to be enough stuff out there for everything to hang together. Galaxies spin so fast that, based on the amount of visible matter in them, they ought to be flung to pieces, the same way a spinning yo-yo can break its string. Cosmologists tried to solve the problem by positing dark matter—a mysterious, invisible substance that surrounds galaxies, holding the visible matter in place—and particle physicists, attempting to identify the nature of the stuff, have undertaken a slew of experiments to detect it. So far, none have.

Now, John W. Moffat, a physicist at the Perimeter Institute for Theoretical Physics in Waterloo, Canada, offers a different solution to the problem. The cap­stone to a storybook career—one that began with a correspondence with Einstein and a conversation with Niels Bohr—Moffat's modified gravity theory, or MOG, can model the movements of the universe without recourse to dark matter, and his work chal­lenging the constancy of the speed of light raises a stark challenge to the usual models of the first half-million years of the universe's existence.

This bold new work, presenting the entirety of Moffat's hypothesis to a general readership for the first time, promises to overturn everything we thought we knew about the origins and evolution of the universe.

Editorial Reviews

Publishers Weekly

Gravity has long been the problem child of physics, creating difficulties in finding a Theory of Everything. To complicate matters, most scientists believe that there is a mysterious, unidentified "dark matter" that makes up most of the universe, and that an equally baffling "dark energy" is pushing the universe apart. Moffat, an affiliate member of the cutting-edge Perimeter Institute for Theoretical Physics in Canada, has developed a new theory that he calls Modified Gravity (MOG). Moffat says that both Newton and Einstein were wrong, and that Newton's gravitational constant is not constant across distances as large as galaxies and galaxy clusters. Scientists haven't been able to find dark matter because it doesn't exist: MOG values help account for rates of galaxy rotation. Perhaps more revolutionary is Moffat's claim that black holes don't exist either. His theory predicts a "grey star," a massive object with many but not all of the properties of a black hole. Moffat's theory thus far has withstood many objections. If MOG stands the test of time, Moffat will have created a paradigm shift not seen since Newton. Illus. (Oct.)

Copyright © Reed Business Information, a division of Reed Elsevier Inc. All rights reserved.
Kirkus Reviews
Canadian theoretical physicist Moffat describes efforts to explain several distressing new cosmological phenomena that don't fit comfortably into the theory of relativity. Readers will easily follow the first-time author's lucid prose as he lays out the story of gravitation research from the time of Aristotle (who taught that objects fell to earth because they belonged there) through Newton to Einstein, whose theory of relativity explains a great deal but not everything. For 50 years astronomers have known that gravitational attraction from visible matter can't explain the movements of stars and galaxies. For Einstein's theory to work, 90 percent of matter in the universe must be invisible. (Gas and dust don't qualify because astronomers can detect them.) This "dark matter" must consist of strange subatomic particles that no particle accelerator has yet produced. In 1998 more flies entered the ointment with the discovery that the expansion of the universe is accelerating, requiring an immense, hypothetical "dark energy." Explaining these has led to Rube Goldberg-like theories featuring many so-far undetected particles (supersymmetry) or complex mathematical systems impossible to verify (string theory). Twenty years ago, Moffat and others began suggesting that gravity can vary. This violates relativity but eliminates the need for dark matter and perhaps even dark energy. After initially turning up its nose, the establishment softened, and now a respectable minority of physicists is working to modify the theory of gravity. Following in the nuts-and-bolts footsteps of Brian Greene (The Elegant Universe, 1999) and Dan Hooper (Nature's Blueprint, 2008), Moffat does a fine job recounting hisfield's history until well into the 20th century, but readers who have forgotten their first-year college physics may struggle to understand the controversies that disturb today's theoretical physicists. Solid, mainstream popular science.

Product Details

HarperCollins Publishers
Publication date:
Sold by:
Sales rank:
File size:
952 KB

Read an Excerpt

Reinventing Gravity
A Physicist Goes Beyond Einstein

Chapter One

The Greeks to Newton

Is there any phenomenon in physics as obvious as the force of gravity? Gravity keeps the planets in their orbits around the sun and holds stars together in galaxies. It prevents us from floating off the Earth, makes acorns and apples fall down from trees, and brings arrows, balls, and bullets to the ground in a curved path.

Yet gravity is so embedded in our environment that many thousands of years passed before humans even perceived gravity and gave it a name. In fact, the everyday evidence of gravity is extremely difficult to "see" when one lives on one planet, without traveling to another for comparison. The little prince in Saint-Exupéry's tale would have formed a vastly different idea of gravity from living only on his small asteroid. To early human beings, just as to most of us today, the behavior of falling objects is a practical experience taken for granted rather than an example of a universal force. Because the Earth is large and we only experience gravity from the effects of Earth, and not some other object, we tend to think of gravity as "down," without realizing that gravity is a property of bodies in general. In contrast, electromagnetism is a much more obvious force. We see it in lightning and magnets and feel it in static electricity. But it took many centuries to discover gravity, and some promising ideas along the way turned out to be completely wrong. It wasn't until the late seventeenth century that Isaac Newton recognized that the same force of attraction or "togetherness" that ruled on the Earth also bound objects in theheavens. The paradigm shift that Newton wrought was in understanding gravity as a universal force.

The story of the discovery of gravity is also the story of astronomy, especially the evolving ideas about the solar system. Western science originated with the Greeks, whose model of an Earth-centered universe dominated scientific thought for almost 2,000 years. The Greek mind was abstract, fond of ideals and patterns, and slipped easily into Christianity's Earth- and human-centered theology. It took many centuries for thinkers such as Copernicus, Kepler, Galileo, and Newton to break with the enmeshed Platonic and Christian views of the universe, to turn astronomy and physics into sciences, and to develop the idea of gravity.

Greek astronomy and gravity

Plato's most famous student was Aristotle (384-322 bc), whose system of thought formed the basis of Western science and medicine until the Renaissance. For Aristotle, four elements composed matter: Earth, Water, Air, and Fire. Earth, as the basest and heaviest of the elements, was at the center of the universe. Although Aristotle did not use the Greek equivalent of the word "gravity," he believed that people and objects did not fall off the Earth because they were held by the "heaviness" of Earth.

Plato had taught that nature's most perfect shapes were the circle, in two dimensions, and the sphere in three. Aristotle's cosmology in turn relied heavily on circles and spheres. Around Aristotle's Earth, several "crystalline spheres" revolved. First were the Earth-related spheres of Water, Air, and Fire. Spheres farther out contained the heavenly bodies that appeared to move around the Earth: the moon, sun, and the five planets known to the Greeks (Mercury, Venus, Mars, Jupiter, and Saturn). Beyond these was the sphere of the "fixed stars," while the final sphere was the dwelling place of God, the Prime Mover of all the spheres. This cosmology needed spheres for the heavenly bodies to move on because Aristotle believed that objects could move only when in contact with another moving object. The spheres were "crystalline" rather than translucent or opaque because the fixed stars had to be visible to observers on Earth through the other rotating spheres.

The ancient Greeks knew that the Earth was a sphere, but most astronomers pictured it as a static object, immovable at the center of the universe. This view stemmed from "common sense": In our everyday experience, barring earthquakes, we do not sense any motion of the Earth. Also, if the Earth moved through the heavens, the Greeks argued, we would observe stellar parallax. Parallax can easily be demonstrated by holding a finger up in front of one's face and closing first one eye and then the other; the finger appears to be moving from side to side relative to objects in the background. Similarly, if the Earth moved through the heavens, then the stars nearest to Earth in the stellar sphere would move relative to those more distant. Since this did not happen, Aristotle concluded that the Earth stayed still at the center of the universe.

Aristotle and his contemporaries did not conceive of the vast distances that actually separate objects in the universe, and believed that the "fixed stars" were thousands of times closer to Earth than they are. In fact, we can detect parallax in the nearer stars today, as the Earth moves around the sun, and more dramatically as the solar system moves around the Milky Way galaxy. Powerful telescopes take photographs of the same stars at different points in the Earth's or solar system's orbit, and differences in the stars' positions relative to background stars can be seen when comparing those photographs.

One prominent Greek astronomer, Aristarchus of Samos (310-230 bc), did propose a heliocentric universe. He had figured out that the sun was a great deal larger than the Earth, and it made more sense to him that a smaller object would orbit a larger one. Aristarchus concluded that the universe was much larger than most people believed, that the sun was at its center, and that neither the sun nor the sphere of fixed stars moved. Aristarchus correctly placed the moon in orbit around the Earth, and all the planets, including Earth, orbiting the sun. He also concluded that we do not observe parallax because the stars are almost infinitely far away from the sun.

But Aristarchus was clearly ahead of his time. Most mathematicians and astronomers in ancient Greece considered the geocentric model of the universe to be a far simpler and more logical explanation of the movements of planets than the heliocentric universe of Aristarchus. Aristarchus was actually charged with impiety for removing the Earth and human beings from the center of the universe.

Reinventing Gravity
A Physicist Goes Beyond Einstein
. Copyright © by John Moffat. Reprinted by permission of HarperCollins Publishers, Inc. All rights reserved. Available now wherever books are sold.

Meet the Author

John W. Moffat is professor emeritus of physics at the University of Toronto and an adjunct professor of physics at the University of Waterloo, as well as a resident affiliate member of the Perimeter Institute for Theoretical Physics in Ontario, Canada. He earned a doctorate in physics at Trinity College at the University of Cambridge.

Customer Reviews

Average Review:

Post to your social network


Most Helpful Customer Reviews

See all customer reviews