Tag: Cosmology

Contributor Post Created with Sketch. Saturday Night Science: Fashion, Faith, and Fantasy

 

“Fashion, Faith, and Fantasy” by Roger PenroseSir Roger Penrose is one of the most distinguished theoretical physicists and mathematicians working today. He is known for his work on general relativity, including the Penrose-Hawking Singularity Theorems, which were a central part of the renaissance of general relativity and the acceptance of the physical reality of black holes in the 1960s and 1970s. Penrose has contributed to cosmology, argued that consciousness is not a computational process, speculated that quantum mechanical processes are involved in consciousness, proposed experimental tests to determine whether gravitation is involved in the apparent mysteries of quantum mechanics, explored the extraordinarily special conditions which appear to have obtained at the time of the Big Bang and suggested a model which might explain them, and, in mathematics, discovered Penrose tiling, a non-periodic tessellation of the plane which exhibits five-fold symmetry, which was used (without his permission) in the design of toilet paper.

“Fashion, Faith, and Fantasy” seems an odd title for a book about the fundamental physics of the universe by one of the most eminent researchers in the field. But, as the author describes in mathematical detail (which some readers may find forbidding), these all-too-human characteristics play a part in what researchers may present to the public as a dispassionate, entirely rational, search for truth, unsullied by such enthusiasms. While researchers in fundamental physics are rarely blinded to experimental evidence by fashion, faith, and fantasy, their choice of areas to explore, willingness to pursue intellectual topics far from any mooring in experiment, tendency to indulge in flights of theoretical fancy (for which there is no direct evidence whatsoever and which may not be possible to test, even in principle) do, the author contends, affect the direction of research, to its detriment.

To illustrate the power of fashion, Penrose discusses string theory, which has occupied the attentions of theorists for four decades and been described by some of its practitioners as “the only game in town”. (This is a piñata which has been whacked by others, including Peter Woit in Not Even Wrong [Saturday Night Science, 2014-11-15] and Lee Smolin in The Trouble with Physics [2014-09-13].) Unlike other critiques, which concentrate mostly on the failure of string theory to produce a single testable prediction, and the failure of experimentalists to find any evidence supporting its claims (for example, the existence of supersymmetric particles), Penrose concentrates on what he argues is a mathematical flaw in the foundations of string theory, which those pursuing it sweep under the rug, assuming that when a final theory is formulated (when?), its solution will be evident. Central to Penrose’s argument is that string theories are formulated in a space with more dimensions than the three we perceive ourselves to inhabit. Depending upon the version of string theory, it may invoke 10, 11, or 26 dimensions. Why don’t we observe these extra dimensions? Well, the string theorists argue that they’re all rolled up into a size so tiny that none of our experiments can detect any of their effects. To which Penrose responds, “not so fast”: these extra dimensions, however many, will vastly increase the functional freedom of the theory and lead to a mathematical instability which will cause the theory to blow up much like the ultraviolet catastrophe which was a key motivation for the creation of the original version of quantum theory. String theorists put forward arguments why quantum effects may similarly avoid the catastrophe Penrose describes, but he dismisses them as no more than arm waving. If you want to understand the functional freedom argument in detail, you’re just going to have to read the book. Explaining it here would require a ten kiloword review, so I shall not attempt it.

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I’m traveling down to Phoenix today to attend the 2016 Electric Universe Conference there. This is a fairly controversial topic among scientists and the theories that are put forward are mind boggling. Generally, this is considered a dissident faction of cosmology. In its early days it was affected by Velikovsky’s theories and books, Ages in […]

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Contributor Post Created with Sketch. Saturday Night Science: The Cosmic Web

 

“The Cosmic Web” by J. Richard GottSome works of popular science, trying to impress the reader with the scale of the universe and the insignificance of humans on the cosmic scale, argue that there’s nothing special about our place in the universe: “an ordinary planet orbiting an ordinary star, in a typical orbit within an ordinary galaxy,” or something like that. But this is wrong! Surfaces of planets make up a vanishingly small fraction of the volume of the universe, and habitable planets, where beings like ourselves are neither frozen nor fried by extremes of temperature, nor suffocated or poisoned by a toxic atmosphere, are rarer still. The Sun is far from an ordinary star: it is brighter than 85% of the stars in the galaxy, and only 7.8% of stars in the Milky Way share its spectral class. Fully 76% of stars are dim red dwarves, the heavens’ own 25 watt bulbs.

What does a typical place in the universe look like? What would you see if you were there? Well, first of all, you’d need a space suit and air supply, since the universe is mostly empty. And you’d see nothing. Most of the volume of the universe consists of great voids with few galaxies. If you were at a typical place in the universe, you’d be in one of these voids, probably far enough from the nearest galaxy that it wouldn’t be visible to the unaided eye. There would be no stars in the sky, since stars are only formed within galaxies. There would only be darkness. Now look out the window: you are in a pretty special place after all.

One of the great intellectual adventures of the last century is learning our place in the universe and coming to understand its large scale structure. The Cosmic Web written by J. Richard Gott, an astrophysicist who has played an important role in discovering that structure, explains how we pieced together the evidence and came to learn the details of the universe we inhabit. It provides an insider’s look at how astronomers tease insight out of the messy and often confusing data obtained from observation.

Jim Baggott is an influential science writer. A scientist himself by training, he has turned toward a career in the commercial world as a successful author who popularizes complex scientific theories by making them, well, understandable.

His latest, Origins: The Scientific Story of Creation, is a concise history of how we got here, how life has evolved on this planet, and where life may be heading next. Baggott joins us here for an hour. We only wish that we’d had more time.

Contributor Post Created with Sketch. Member Post

 

In his 2013 book Time Reborn, Lee Smolin argued that, despite its extraordinary effectiveness in understanding the behaviour of isolated systems, what he calls the “Newtonian paradigm” is inadequate to discuss cosmology: the history and evolution of the universe as a whole. In this book, Smolin and philosopher Roberto Mangabeira Unger expand upon that observation […]

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Contributor Post Created with Sketch. Saturday Night Science: Many Worlds In One

 

“Many Worlds In One” by Alexander VilenkinFrom the dawn of the human species until a time within the memory of many people younger than I, the origin of the universe was the subject of myth and a topic, if discussed at all within the academy, among doctors of divinity, not professors of physics. The advent of precision cosmology has changed that: the ultimate questions of origin are not only legitimate areas of research, but something probed by satellites in space, balloons circling the South Pole, and mega-projects of Big Science. The results of these experiments have, in the last few decades, converged upon a consensus from which few professional cosmologists would dissent:

  1. At the largest scale, the geometry of the universe is indistinguishable from Euclidean (flat), and the distribution of matter and energy within it is homogeneous and isotropic.
  2. The universe evolved from an extremely hot, dense, phase starting about 13.7 billion years ago from our point of observation, which resulted in the abundances of light elements observed today.
  3. The evidence of this event is imprinted on the cosmic background radiation which can presently be observed in the microwave frequency band. All large-scale structures in the universe grew from gravitational amplification of scale-independent quantum fluctuations in density.
  4. The flatness, homogeneity, and isotropy of the universe are best explained by a period of inflation shortly after the origin of the universe, which expanded a tiny region of space, smaller than a subatomic particle, to a volume much greater than the presently observable universe.
  5. Consequently, the universe we can observe today is bounded by a horizon, about forty billion light years away in every direction (greater than the 13.7 billion light years you might expect since the universe has been expanding since its origin), but the universe is much, much larger than what we can see; every year another light year comes into view in every direction.

Now, this may seem mind-boggling enough, but from these premises, which it must be understood are accepted by most experts who study the origin of the universe, one can deduce some disturbing consequences which seem to be logically unavoidable.

Let me walk you through it here. We assume the universe is infinite and unbounded, which is the best estimate from precision cosmology. Then, within that universe, there will be an infinite number of observable regions, which we’ll call O-regions, each defined by the volume from which an observer at the centre can have received light since the origin of the universe. Now, each O-region has a finite volume, and quantum mechanics tells us that within a finite volume there are a finite number of possible quantum states. This number, although huge (on the order of 10^10^123 for a region the size of the one we presently inhabit), is not infinite, so consequently, with an infinite number of O-regions, even if quantum mechanics specifies the initial conditions of every O-region completely at random and they evolve randomly with every quantum event thereafter, there are only a finite number of histories they can experience (around 10^10^150). Which means that, at this moment, in this universe (albeit not within our current observational horizon), invoking nothing as fuzzy, weird, or speculative as the multiple world interpretation of quantum mechanics, there are an infinite number of you reading these words scribbled by an infinite number of me. In the vast majority of our shared universes things continue much the same, but from time to time they d1v3r93 r4ndtx#e~—….

Contributor Post Created with Sketch. Science Confirms Judeo-Christian Worldview, Or, Dalai Lama, Call Your Office

 

One of the most basic observations of comparative religion is that the difference between Judeo-Christian religion and Asian religious systems, such as Buddhism, resembles the difference between a line and a circle.

In Judaism and Christianity, reality has a beginning and an end. It’s linear. It’s going somewhere. Both beginning and end are mysterious, the former rendered, mythically, in the creation story, the latter represented, at least in Christianity, in the thrilling if baffling formulation that “time shall be no more.” The beginning is believed really to have happened and the end is believed to really be coming.