The Anthropic Principle and Multiple Universe Hypotheses Oren Kreps
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Cosmic Questions, Answers Pending
special section | cosmic questions, Answers pending Cosmic questions, answers pending throughout human history, great missions of mission reveal the exploration have been inspired by curiosity, : the desire to find out about unknown realms. secrets of the universe such missions have taken explorers across wide oceans and far below their surfaces, THE OBJECTIVE deep into jungles, high onto mountain peaks For millennia, people have turned to the heavens in search of clues to nature’s mysteries. truth seekers from ages past to the present day and over vast stretches of ice to the earth’s have found that the earth is not the center of the universe, that polar extremities. countless galaxies dot the abyss of space, that an unknown form of today’s greatest exploratory mission is no matter and dark forces are at work in shaping the cosmos. Yet despite longer earthbound. it’s the scientific quest to these heroic efforts, big cosmological questions remain unresolved: explain the cosmos, to answer the grandest What happened before the Big Bang? ............................... Page 22 questions about the universe as a whole. What is the universe made of? ......................................... Page 24 what is the identity, for example, of the Is there a theory of everything? ....................................... Page 26 Are space and time fundamental? .................................... Page 28 “dark” ingredients in the cosmic recipe, com- What is the fate of the universe? ..................................... Page 30 posing 95 percent of the -
Inflation and the Theory of Cosmological Perturbations
Inflation and the Theory of Cosmological Perturbations A. Riotto INFN, Sezione di Padova, via Marzolo 8, I-35131, Padova, Italy. Abstract These lectures provide a pedagogical introduction to inflation and the theory of cosmological per- turbations generated during inflation which are thought to be the origin of structure in the universe. Lectures given at the: Summer School on arXiv:hep-ph/0210162v2 30 Jan 2017 Astroparticle Physics and Cosmology Trieste, 17 June - 5 July 2002 1 Notation A few words on the metric notation. We will be using the convention (−; +; +; +), even though we might switch time to time to the other option (+; −; −; −). This might happen for our convenience, but also for pedagogical reasons. Students should not be shielded too much against the phenomenon of changes of convention and notation in books and articles. Units We will adopt natural, or high energy physics, units. There is only one fundamental dimension, energy, after setting ~ = c = kb = 1, [Energy] = [Mass] = [Temperature] = [Length]−1 = [Time]−1 : The most common conversion factors and quantities we will make use of are 1 GeV−1 = 1:97 × 10−14 cm=6:59 × 10−25 sec, 1 Mpc= 3.08×1024 cm=1.56×1038 GeV−1, 19 MPl = 1:22 × 10 GeV, −1 −1 −42 H0= 100 h Km sec Mpc =2.1 h × 10 GeV, 2 −29 −3 2 4 −3 2 −47 4 ρc = 1:87h · 10 g cm = 1:05h · 10 eV cm = 8:1h × 10 GeV , −13 T0 = 2:75 K=2.3×10 GeV, 2 Teq = 5:5(Ω0h ) eV, Tls = 0:26 (T0=2:75 K) eV. -
THE ANTHROPIC PRINCIPLE - IS the UNIVERSE SPECIALLY DESIGNED to SUPPORT LIFE? by William Reville, University College, Cork
THE ANTHROPIC PRINCIPLE - IS THE UNIVERSE SPECIALLY DESIGNED TO SUPPORT LIFE? By William Reville, University College, Cork. Scientists are often impressed by how finely-tuned the world is for the existence of life. If any of a large number of fundamental physical properties of the world were slightly different, biological life would be impossible. The observation that we inhabit a world which is uniquely suited to us has led to the development of a scientific principle called the anthropic principle. This principle asserts that we see the universe the way it is because we exist. There are two forms of the anthropic principle, a weak form and a strong form. Most scientists find the weak anthrophic principle to be a useful methodological principle, but few scientists believe in the strong form of the principle. Others claim that the anthropic principle is not a scientific principle at all, but is just an irritating tautology. The principle is lucidly described in Theories of Everything by J.D. Barrow (Clarendon Press, 1991). The weak anthropic principle recognises that the fact of human existence requires certain conditions to be met regarding the past and the present structure of the universe. In other words, the conditions we observe in the universe must be such that allowed carbon-based observers like ourselves to arise and evolve within a certain time-frame. This time-frame must reside in a window of opportunity bounded at the late end by the death of the sun and, at the early end, by the requirement that the elements that compose our bodies must be present. -
Vilenkin's Cosmic Vision a Review Essay of Emmany Worlds in One
Vilenkin's Cosmic Vision A Review Essay of emMany Worlds in One The Search for Other Universesem, by Alex Vilenkin William Lane Craig Used by permission of Philosophia Christi 11 (2009): 231-8. SUMMARY Vilenkin's recent book is a wonderful popular introduction to contemporary cosmology. It contains provocative discussions of both the beginning of the universe and of the fine-tuning of the universe for intelligent life. Vilenkin is a prominent exponent of the multiverse hypothesis, which features in the book's title. His defense of this hypothesis depends in a crucial and interesting way on conflating time and space. His claim that his theory of the quantum creation of the universe explains the origin of the universe from nothing trades on a misunderstanding of "nothing." VILENKIN'S COSMIC VISION A REVIEW ESSAY OF EMMANY WORLDS IN ONE THE SEARCH FOR OTHER UNIVERSESEM, BY ALEX VILENKIN The task of scientific popularization is a difficult one. Too many authors think that it is to be accomplished by frequent resort to explanatorily vacuous and obfuscating metaphors which leave the reader puzzling over what exactly a particular theory asserts. One of the great merits of Alexander Vilenkin's book is that he shuns this route in favor of straightforward, simple explanations of key terms and ideas. Couple that with a writing style that is marvelously lucid, and you have one of the best popularizations of current physical cosmology available from one of its foremost practitioners. Vilenkin vigorously champions the idea that we live in a multiverse, that is to say, the causally connected universe is but one domain in a much vaster cosmos which comprises an infinite number of such domains. -
The Age of the Universe Transcript
The Age of the Universe Transcript Date: Wednesday, 6 February 2013 - 1:00PM Location: Museum of London 6 February 2013 The Age of The Universe Professor Carolin Crawford Introduction The idea that the Universe might have an age is a relatively new concept, one that became recognised only during the past century. Even as it became understood that individual objects, such as stars, have finite lives surrounded by a birth and an end, the encompassing cosmos was always regarded as a static and eternal framework. The change in our thinking has underpinned cosmology, the science concerned with the structure and the evolution of the Universe as a whole. Before we turn to the whole cosmos then, let us start our story nearer to home, with the difficulty of solving what might appear a simpler problem, determining the age of the Earth. Age of the Earth The fact that our planet has evolved at all arose predominantly from the work of 19th century geologists, and in particular, the understanding of how sedimentary rocks had been set down as an accumulation of layers over extraordinarily long periods of time. The remains of creatures trapped in these layers as fossils clearly did not resemble any currently living, but there was disagreement about how long a time had passed since they had died. The cooling earth The first attempt to age the Earth based on physics rather than geology came from Lord Kelvin at the end of the 19th Century. Assuming that the whole planet would have started from a completely molten state, he then calculated how long it would take for the surface layers of Earth to cool to their present temperature. -
Eternal Inflation and Its Implications
IOP PUBLISHING JOURNAL OF PHYSICS A: MATHEMATICAL AND THEORETICAL J. Phys. A: Math. Theor. 40 (2007) 6811–6826 doi:10.1088/1751-8113/40/25/S25 Eternal inflation and its implications Alan H Guth Center for Theoretical Physics, Laboratory for Nuclear Science, and Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA E-mail: [email protected] Received 8 February 2006 Published 6 June 2007 Online at stacks.iop.org/JPhysA/40/6811 Abstract Isummarizetheargumentsthatstronglysuggestthatouruniverseisthe product of inflation. The mechanisms that lead to eternal inflation in both new and chaotic models are described. Although the infinity of pocket universes produced by eternal inflation are unobservable, it is argued that eternal inflation has real consequences in terms of the way that predictions are extracted from theoretical models. The ambiguities in defining probabilities in eternally inflating spacetimes are reviewed, with emphasis on the youngness paradox that results from a synchronous gauge regularization technique. Although inflation is generically eternal into the future, it is not eternal into the past: it can be proven under reasonable assumptions that the inflating region must be incomplete in past directions, so some physics other than inflation is needed to describe the past boundary of the inflating region. PACS numbers: 98.80.cQ, 98.80.Bp, 98.80.Es 1. Introduction: the successes of inflation Since the proposal of the inflationary model some 25 years ago [1–4], inflation has been remarkably successful in explaining many important qualitative and quantitative properties of the universe. In this paper, I will summarize the key successes, and then discuss a number of issues associated with the eternal nature of inflation. -
Editorial Note To: Brandon Carter, Large Number Coincidences and the Anthropic Principle in Cosmology
Gen Relativ Gravit (2011) 43:3213–3223 DOI 10.1007/s10714-011-1257-8 GOLDEN OLDIE EDITORIAL Editorial note to: Brandon Carter, Large number coincidences and the anthropic principle in cosmology George F. R. Ellis Published online: 27 September 2011 © Springer Science+Business Media, LLC 2011 Keywords Cosmology · Confrontation of cosmological theories with observational data · Anthropic principle · World ensemble · Golden Oldie Editorial The anthropic principle is one of the most controversial proposals in cosmology. It relates to why the universe is of such a nature as to allow the existence of life. This inevitably engages with the foundations of cosmology, and has philosophical as well as technical aspects. The literature on the topic is vast—the Carter paper reprinted here [10] has 226 listed citations, and the Barrow and Tipler book [3] has 1,740. Obviously I can only pick up on a few of these papers in this brief review of the impact of the paper. While there were numerous previous philosophical treatises on the topic, stretching back to speculations about the origin of the universe in ancient times (see [3]fora magisterial survey), scientific studies are more recent. A well known early one was by biologist Alfred Russell Wallace, who wrote in 1904: “Such a vast and complex uni- verse as that which we know exists around us, may have been absolutely required … in order to produce a world that should be precisely adapted in every detail for the orderly development of life culminating in man” [50]. But that was before modern cosmology was established: the idea of the expanding and evolving universe was yet to come. -
Hubble's Law and the Expanding Universe
COMMENTARY COMMENTARY Hubble’s Law and the expanding universe Neta A. Bahcall1 the expansion rate is constant in all direc- Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 tions at any given time, this rate changes with time throughout the life of the uni- verse. When expressed as a function of cos- In one of the most famous classic papers presented the observational evidence for one H t in the annals of science, Edwin Hubble’s of science’s greatest discoveries—the expand- mic time, ( ), it is known as the Hubble 1929 PNAS article on the observed relation inguniverse.Hubbleshowedthatgalaxiesare Parameter. The expansion rate at the pres- between distance and recession velocity of receding away from us with a velocity that is ent time, Ho, is about 70 km/s/Mpc (where 1 Mpc = 106 parsec = 3.26 × 106 light-y). galaxies—the Hubble Law—unveiled the proportional to their distance from us: more The inverse of the Hubble Constant is the expanding universe and forever changed our distant galaxies recede faster than nearby gal- Hubble Time, tH = d/v = 1/H ; it reflects understanding of the cosmos. It inaugurated axies. Hubble’s classic graph of the observed o the time since a linear cosmic expansion has the field of observational cosmology that has velocity vs. distance for nearby galaxies is begun (extrapolating a linear Hubble Law uncovered an amazingly vast universe that presented in Fig. 1; this graph has become back to time t = 0); it is thus related to has been expanding and evolving for 14 bil- a scientific landmark that is regularly repro- the age of the Universe from the Big-Bang lion years and contains dark matter, dark duced in astronomy textbooks. -
Analysis of Big Bounce in Einstein--Cartan Cosmology
Analysis of big bounce in Einstein{Cartan cosmology Jordan L. Cubero∗ and Nikodem J. Poplawski y Department of Mathematics and Physics, University of New Haven, 300 Boston Post Road, West Haven, CT 06516, USA We analyze the dynamics of a homogeneous and isotropic universe in the Einstein{Cartan theory of gravity. The spin of fermions produces spacetime torsion that prevents gravitational singularities and replaces the big bang with a nonsingular big bounce. We show that a closed universe exists only when a particular function of its scale factor and temperature is higher than some threshold value, whereas an open and a flat universes do not have such a restriction. We also show that a bounce of the scale factor is double: as the temperature increases and then decreases, the scale factor decreases, increases, decreases, and then increases. Introduction. The Einstein{Cartan (EC) theory of a size where the cosmological constant starts cosmic ac- gravity provides the simplest mechanism generating a celeration. This expansion also predicts the cosmic mi- nonsingular big bounce, without unknown parameters crowave background radiation parameters that are con- or hypothetical fields [1]. EC is the simplest and most sistent with the Planck 2015 observations [11], as was natural theory of gravity with torsion, in which the La- shown in [12]. grangian density for the gravitational field is proportional The spin-fluid description of matter is the particle ap- to the Ricci scalar, as in general relativity [2, 3]. The con- proximation of the multipole expansion of the integrated sistency of the conservation law for the total (orbital plus conservation laws in EC. -
The Reionization of Cosmic Hydrogen by the First Galaxies Abstract 1
David Goodstein’s Cosmology Book The Reionization of Cosmic Hydrogen by the First Galaxies Abraham Loeb Department of Astronomy, Harvard University, 60 Garden St., Cambridge MA, 02138 Abstract Cosmology is by now a mature experimental science. We are privileged to live at a time when the story of genesis (how the Universe started and developed) can be critically explored by direct observations. Looking deep into the Universe through powerful telescopes, we can see images of the Universe when it was younger because of the finite time it takes light to travel to us from distant sources. Existing data sets include an image of the Universe when it was 0.4 million years old (in the form of the cosmic microwave background), as well as images of individual galaxies when the Universe was older than a billion years. But there is a serious challenge: in between these two epochs was a period when the Universe was dark, stars had not yet formed, and the cosmic microwave background no longer traced the distribution of matter. And this is precisely the most interesting period, when the primordial soup evolved into the rich zoo of objects we now see. The observers are moving ahead along several fronts. The first involves the construction of large infrared telescopes on the ground and in space, that will provide us with new photos of the first galaxies. Current plans include ground-based telescopes which are 24-42 meter in diameter, and NASA’s successor to the Hubble Space Telescope, called the James Webb Space Telescope. In addition, several observational groups around the globe are constructing radio arrays that will be capable of mapping the three-dimensional distribution of cosmic hydrogen in the infant Universe. -
Exploring Cosmic Strings: Observable Effects and Cosmological Constraints
EXPLORING COSMIC STRINGS: OBSERVABLE EFFECTS AND COSMOLOGICAL CONSTRAINTS A dissertation submitted by Eray Sabancilar In partial fulfilment of the requirements for the degree of Doctor of Philosophy in Physics TUFTS UNIVERSITY May 2011 ADVISOR: Prof. Alexander Vilenkin To my parents Afife and Erdal, and to the memory of my grandmother Fadime ii Abstract Observation of cosmic (super)strings can serve as a useful hint to understand the fundamental theories of physics, such as grand unified theories (GUTs) and/or superstring theory. In this regard, I present new mechanisms to pro- duce particles from cosmic (super)strings, and discuss their cosmological and observational effects in this dissertation. The first chapter is devoted to a review of the standard cosmology, cosmic (super)strings and cosmic rays. The second chapter discusses the cosmological effects of moduli. Moduli are relatively light, weakly coupled scalar fields, predicted in supersymmetric particle theories including string theory. They can be emitted from cosmic (super)string loops in the early universe. Abundance of such moduli is con- strained by diffuse gamma ray background, dark matter, and primordial ele- ment abundances. These constraints put an upper bound on the string tension 28 as strong as Gµ . 10− for a wide range of modulus mass m. If the modulus coupling constant is stronger than gravitational strength, modulus radiation can be the dominant energy loss mechanism for the loops. Furthermore, mod- ulus lifetimes become shorter for stronger coupling. Hence, the constraints on string tension Gµ and modulus mass m are significantly relaxed for strongly coupled moduli predicted in superstring theory. Thermal production of these particles and their possible effects are also considered. -
Anthropic Explanations in Cosmology
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by PhilSci Archive 1 Jesús Mosterín ANTHROPIC EXPLANATIONS IN COSMOLOGY In the last century cosmology has ceased to be a dormant branch of speculative philosophy and has become a vibrant part of physics, constantly invigorated by new empirical inputs from a legion of new terrestrial and outer space detectors. Nevertheless cosmology continues to be relevant to our philosophical world view, and some conceptual and methodological issues arising in cosmology are in need of epistemological analysis. In particular, in the last decades extraordinary claims have been repeatedly voiced for an alleged new type of scientific reasoning and explanation, based on a so-called “anthropic principle”. “The anthropic principle is a remarkable device. It eschews the normal methods of science as they have been practiced for centuries, and instead elevates humanity's existence to the status of a principle of understanding” [Greenstein 1988, p. 47]. Steven Weinberg has taken it seriously at some stage, while many physicists and philosophers of science dismiss it out of hand. The whole issue deserves a detailed critical analysis. Let us begin with a historical survey. History of the anthropic principle After Herman Weyl’s remark of 1919 on the dimensionless numbers in physics, several eminent British physicists engaged in numerological or aprioristic speculations in the 1920's and 1930's (see Barrow 1990). Arthur Eddington (1923) calculated the number of protons and electrons in the universe (Eddington's number, N) and found it to be around 10 79 . He noticed the coincidence between N 1/2 and the ratio of the electromagnetic to gravitational 2 1/2 39 forces between a proton and an electron: e /Gm emp ≈ N ≈ 10 .