The Anthropic Principle

Save this PDF as:

Size: px
Start display at page:

Transcription

1 (Also list under The Fine-Tuning argument) The Anthropic Principle Victor J. Stenger For The Encyclopedia of Nonbelief to be published by Prometheus Books. The Anthropic Coincidences In 1919, mathematician and physicist Hermann Weyl puzzled why the ratio of the electromagnetic force to the gravitational force between two electrons is such a huge number, N 1 = Weyl wondered why this should be the case, expressing his intuition (and nothing more than that) that "pure" numbers, like p, that is, numbers that do not depend any system of units, when occurring in the description of physical properties, should most naturally occur within a few orders of magnitude of unity. Why 10 39? Why not or ? Some principle, Weyl thought, must select out In 1923, astronomer Arthur Eddington agreed: "It is difficult to account for the occurrence of a pure number (of order greatly different from unity) in the scheme of things; but this difficulty would be removed if we could connect it to the number of particles in the world a number presumably decided by accident. 2 He estimated that number, now called the "Eddington number," to be N = Well, N is not too far from the square of N 1. In 1937, physicist Paul Dirac noticed that N 1 is the same order of magnitude as another pure number N 2 that gives the ratio of a typical stellar lifetime to the time for light to traverse the radius of a proton. 3 That is, he found two seemingly unconnected large numbers to be of the

2 same order of magnitude. If one number being large is unlikely, how much more unlikely is another to come along with about the same value? In 1961, astrophysicist Robert Dicke pointed out that N 2 is necessarily large in order that the lifetime of typical stars is sufficient to generate heavy chemical elements such as carbon. Furthermore, he showed that N 1 must be of the same order of N 2 in any universe with heavy elements. 4 Thus, this became the first of what are called the anthropic coincidences, connections between physical constants that seem to be necessary for the existence of life in the universe. While many examples of claimed anthropic coincidences can be found in the literature, here are the most significant: 1. The electromagnetic force is 39 orders of magnitude stronger than the gravitational force. If they were more comparable in strength, stars would have collapsed long before life had a chance to evolve. 2. The vacuum energy density of the universe is at least 120 orders of magnitude lower than some theoretical estimates. If at any time it were as large as these calculations suggest, the universe would have quickly blown apart. 3. The electron's mass is less than the difference in the masses of the neutron and proton. Thus, a free neutron can decay into a proton, electron, and anti-neutrino. If this were not the case, the neutron would be stable and most of the protons and electrons in the early universe would have combined to form neutrons, leaving little hydrogen to act as the main component and fuel of stars. 4. The neutron is heavier than the proton, but not so much heavier that neutrons cannot be bound in nuclei, where conservation of energy prevents the neutrons from

3 decaying. Without neutrons we would not have the heavier elements needed for building complex systems such as life. 5. The carbon nucleus has an excited energy level at around 7.65 million electron-volts (MeV). Without this state, insufficient carbon would be manufactured in stars to form the basis for life. Using anthropic arguments, astronomer Fred Hoyle predicted this energy level before it was confirmed experimentally. 5 The Three Anthropic Principles In 1974, astronomer Brandon Carter introduced the notion of the anthropic principle, which hypothesized that the anthropic coincidences are not the result of chance but somehow built into the structure of the universe. 6 He proposed two versions. His weak anthropic principle (WAP) states that We must be prepared to take into account the fact that our location in the universe is necessarily privileged to the extent of being compatible with our existence as observers. Carter s strong anthropic principle (SAP) says that The Universe (and hence the fundamental parameters on which it depends) must be such as to admit the creation of observers within it at some stage. Other authors have presented their own versions of anthropic principles, over thirty being available in the literature. I will just mention three more versions those proposed by mathematician John Barrow and physicist Frank Tipler in their tome on the subject. 7 The first two are rephrases of Carter s wording. The Barrow and Tipler WAP reads: The observed values of all physical and cosmological quantities are not equally probable but take on values restricted by the requirement that there exist sites

4 where carbon-based life can evolve and by the requirement that the Universe be old enough for it to have already done so. Note that Barrow and Tipler require the existence of carbon-based life while Carter simply refers to the existence of observers. This is better phasing since many of the coincidences have to do with carbon, directly or indirectly. Barrow and Tipler s SAP reads: The Universe must have those properties which allow life to develop within it at some stage in its history. Note that all three authors say that the universe must have the properties that allow for the creation of life, or, at least, observers. Thus, the SAP seems to imply some intent or purpose within the universe. Barrow and Tipler round out their various anthropic principles with the final anthropic principle (FAP): Intelligent, information processing must come into evidence in the Universe, and, once it comes into existence, it will never die out. Note that the term "anthropic principle" is a misnomer, as is "anthropic coincidence." While singling out our kind of carbon-based life, none of the coincidences require human life or demand that carbon-based life develop intelligence. Implications The WAP is considered by most physicists and cosmologists to be a simple tautology. Of course the constants of nature are suitable for our form of life. If they were not, we would not be here to talk about it. For a study of selection effects, see Bostrom. 8

5 Still, the anthropic coincidences strike most people as puzzling and they wonder what might imply about the nature of the universe. Barrow and Tipler suggest three different possible implications of the SAP: (A) There exists one possible universe "designed" with the goal of generating and sustaining "observers." (B) Observers are necessary to bring the Universe into being. (C) An ensemble of other different universes is necessary for the existence of our universe. Authors with religious agenda have interpreted (A) as evidence for a creator God, in particular, the God they happen to worship. They ask: How can the universe possibly have obtained the unique set of physical constants it has, so exquisitely fine-tuned for life as they are, except by purposeful design design with life and perhaps humanity in mind? 9,10 However, nothing in the above discussion requires that this God be the one of any particular faith. Indeed, design might be interpreted as a purely natural process, perhaps an evolutionary one akin to the design inherent in Darwinian natural selection or just some structure built into the universe that science has not yet explained. 11 Possibility (B) arises from a mystical misinterpretation of quantum mechanics. Though it has formed the basis of a large popular literature in recent years, few physicists take it very seriously. 12 Possibility (C) presents the notion that multiple universes exist and so we happen to just live in that universe which is suitable for the evolution of our kind of life. We will consider this possibility below.

6 Fine-tuning in the Eye of the Beholder The strength of the electromagnetic force is determined by the value of the unit electric charge the magnitude of the charge of an electron designated by e. The claim is that e is a constant that has been fine-tuned far from its natural value in order that we have stars sufficiently long-lived for life to evolve (coincidence 1 above). However, e is not a constant. We now know from the highly successful standard model of particles and forces that e and the strengths of the other elementary forces vary with energy and changed very rapidly in the first moments of the big bang. According to current understanding, in the very high-energy environment at the start of the big bang, the four known forces were unified as one force, just as Weyl anticipated should happen "naturally." That is, e began with its natural value. Then, as the universe cooled, the forces separated by a process called spontaneous symmetry breaking into the four basic kinds we experience at much lower energies today, with e and the other force strengths having evolved to their current stable values. Stellar formation, and thus life, had to simply wait for the forces to separate sufficiently. Actually the wait was a just tiny fraction of a second. Only four parameters are needed to specify the broad features of the universe, as it exists today: the masses of the electron and proton and the current strengths of the electromagnetic and strong interactions. 13 I have studied how the minimum lifetime of a typical star depends on the first three of these parameters. Varying them by ten orders of magnitude around their present values, I find that over half of the stars will have lifetimes exceeding a billion years. 14 Large stars need to live tens of millions of years or more to allow for the fabrication of heavy elements. Smaller stars, such as our sun, also need about a billion years to allow life to develop within its solar system of planets. Earth did not even form until nine billion years after

7 the big bang. The requirement of long-lived stars is easily met for a wide range of possible parameters. The universe is certainly not fine-tuned for this characteristic. One of the many major flaws with most studies of the anthropic coincidences is that the investigators vary a single parameter while assuming all the others remain fixed. They further compound this mistake by proceeding to calculate meaningless probabilities based on the grossly erroneous assumption that all the parameters are independent. 15 In my study I took care to allow several parameters to vary at the same time. In a very impressive paper, physicist Anthony Aguire has independently examined the universes that result when six cosmological parameters are simultaneously varied by orders of magnitude and found he could construct cosmologies in which "stars, planets, and intelligent life can plausibly arise." 16 The standard model contains about twenty parameters that are not determined by the theory but must currently be inferred from experiments. However, only four are needed to specify most properties of matter. These are the masses of the electron and the two quarks ("up" and "down") that constitute protons and neutrons, and a universal strength parameter from which the value e and the other force strengths are determined. Ultimately, it is hoped that all the basic parameters will be determined by theories that unify gravity with the standard model, for example, string theory. 17 We must wait to see if the calculated masses of the electron and neutron come out to satisfy coincidences 3 and 4 above. Another possibility, which we will consider below, is that these parameters are random. Many of the examples of anthropic coincidences found in theological literature result from simple misunderstanding of physics. For example, any reference to the fine-tuning of constants like the speed of light c, Planck's constant, h, or Newton's gravitational constant, G, are

8 irrelevant since these are all arbitrary constants whose values simply define the system of units being used. Also, some of the "remarkable" precision people talk about is highly misleading, depending on the arbitrary choice of units. For example, theologian John Jefferson Davis asserts, "If the mass of neutrinos were 5x10-34 instead of 5x10-35 kg [kilogram], because of their great abundance in the universe, the additional gravitational mass would result in a contracting rather than expanding universe." 18 This sounds like fine-tuning by one part in However, as philosopher Neil Manson points out, this is like saying that "if he had been one part in of a light-year shorter (that is, one meter shorter), Michael Jordan would not have been the world s greatest basketball player." 19 Incidentally, Davis' estimate of the neutrino mass is not accurate. In fact, the individual masses are not known, with experiments so far measuring only mass differences. Furthermore, if the mass of neutrinos were ten times greater, there likely would be ten times fewer of them in the cosmos and the gravitational effect would be the same. So this fine-tuning claim collapses on several fronts. Let us next consider coincidence 5, which asserts fine-tuning is needed to produce carbon. Nobel laureate physicist Steven Weinberg has shown that the production of carbon in stars is not very dependent on the 7.65 MeV nuclear energy level predicted by Hoyle. Rather it hinges on the radioactive state of a carbon nucleus formed out of three beryllium nuclei. This misses being too high for carbon production by 20 percent, which, as he says, "is not such a close call after all." 20 In short, much of the so-called fine-tuning of the parameters of microphysics is in the eye of the beholder, not always sufficiently versed in physics, who plays with the numbers until they seem to support a prior belief that was based on something other than objective scientific analysis.

9 The Vacuum Energy Problem Although we normally think of the vacuum as empty of matter and energy, gravitational energy can be stored in the curvature of empty space. Futhermore, quantum mechanics implies that a vacuum will contain a minimum zero-point energy. Weinberg was perhaps the first to highlight the vacuum energy problem (coincidence 2). He referred to it as the cosmological constant problem, since any vacuum energy density is equivalent to the parameter in Einstein's theory of general relativity called the cosmological constant that relates to the curvature of empty space. 21 Calculations gave a value for the vacuum energy density that is some 120 orders of magnitude greater than the maximum value possible from observations. Since this density is constant, it would seem to have been fine-tuned with this precision from the early universe, so that its value today allowed for the existence of life. Until recently, it was thought that the cosmological constant was probably exactly zero, in which case there was no need for fine-tuning. However, in 1998, two independent research groups studying distant supernovae were astonished to discover that the current expansion of the universe is accelerating. 22 More recent observations have confirmed this result. The universe is falling up! The source of this cosmic acceleration is some still-unidentified dark energy, which constitutes 70 percent of the mass of the universe. One possible explanation is gravitational repulsion by means of the cosmological constant, that is, by way of the vacuum energy field that is allowed by general relativity. If that is the case, then the cosmological constant problem resurfaces. In the meantime, we now can argue plausibly that the original calculation was incomplete and a proper calculation will give zero for the vacuum energy density. Until these newer estimates are shown to be

10 wrong, we cannot conclude that the vacuum is fine-tuned for life and have no particularly strong need to invoke a designer deity. But, then, what is responsible for cosmic acceleration? What is the nature of the dark energy? A cosmological constant is not the only possible source of gravitational repulsion. According to general relativity, any matter field will be repulsive if its pressure is sufficiently negative. Theorists have proposed that the dark energy may be a matter field, called quintessence, which requires no fine-tuning. Is Our Form of Life the Only Possible? Consider the fact that we live on Earth, rather than Mercury, Venus, Mars, or some other planet in the known solar system. Mercury and Venus are too hot and Mars is too cold. Mercury has no atmosphere, while the atmosphere of Venus is too thick for the sun s rays to penetrate to the surface and the atmosphere of Mars is too thin to provide sufficient oxygen and water. The temperature range and other properties of Earth are just right for life. For example, Earth s atmosphere is transparent to the same spectrum of light to which our eyes are sensitive. Anthropic reasoning would have it that the atmosphere was fine-tuned so that humans and other animals could see at a distance. The transparency also happens to match the spectral regions within which the electromagnetic radiation from the sun is maximal. Again, anthropic reasoning would attribute this to design with humans in mind. But, rather obviously, life evolved on Earth because conditions here were right. The type of life that evolved was suitable for those conditions. With 100 billion stars in 100 billion galaxies in the visible universe, and countless others, according to current cosmological theory, likely to lie beyond our horizon, the chances of some form of life developing on some planets seems very good. Indeed, many of the chemical

11 ingredients of life such as complex molecules have been observed in outer space. Of course, we will not know for sure until we find such life. Still, we expect any life found in our universe to be carbon-based, or at least based on heavy element chemistry. The fine-tuning argument implies that this is the only form of life that is possible, and that is a huge, unwarranted assumption. Even if all the forms of life in our universe turn out to be of this basic structure, it does not follow that life is impossible under any other arrangement of physical laws and constants. This fact alone is fatal to the fine-tuning argument. Carbon would seem to be the chemical element best suited to act as the building block for the type of complex molecular systems that develop lifelike qualities. Even today, new materials assembled from carbon atoms exhibit remarkable, unexpected properties, from superconductivity to ferromagnetism. However, we have no reason to assume that only carbon life is possible. Given the known laws of physics and chemistry, we can imagine life based on silicon or other elements chemically similar to carbon. While carbon may be optimum for the parameters of our universe, silicon might be better if the parameters were slightly different. However, whatever elements are used, they still require cooking in stars and thus a universe old enough for stellar evolution. We can only speculate what form life might take on another planet, with different conditions. It would be wonderful to have more examples of life, but we do not. And, any speculation about what form life might take in a universe with a different electron mass, electromagnetic interaction strength, or different laws of physics is even more problematical. We simply do not have the knowledge to say whether life of some sort would not occur under different circumstances.

12 Multiple Universes We have seen that cosmological parameters, such as the cosmological constant, need not have been fine-tuned for life. We also have a plausible scenario in which the strengths of the four forces evolved to their current values and that long-live stars can be expected over a large range of these and other physical parameters. The hope is that a future theory that unifies gravity and microphysics will enable the calculation of the few parameters that are needed to define the fundamental structure of matter. However, even if this hope is not realized current theories already suggest another possible answer to the anthropic coincidences. For example, our universe may be just one of a huge number other universes within some super universe called the multiverse. The fundamental parameters may be randomly distributed among universes and we live in the one where the parameters happen to be suitable for the evolution of our form of life. Theists have scoffed at the idea of multiple universes, arguing that we have no evidence for the existence of any but our own. But, we have no evidence for their God, either. At least in the case of multiple universes we have physical theories, based firmly on empirical data within our own universe, pointing to their existence. The highly successful cosmological inflation model implies that the spontaneous event that created our universe would have been repeated many times. 23 While this may still be classified as speculation, it is speculation based on good science and observational data. The speculation that a Creator God exists is based on no science and no data. Several commentators have argued that a multiverse cosmology violates Occam's razor. 24 This is wrong. The entities that Occam's law of parsimony forbids us from "multiplying beyond necessity" are theoretical hypotheses, not universes. Although the atomic theory of matter multiplied the number of bodies we must consider in solving a thermodynamic problem by 10 24

13 or so per gram, it did not violate Occam's razor. Instead, it provided for a simpler, more powerful, more economic exposition of the rules that were obeyed by thermodynamic systems. The existence of many universes is in fact consistent with all we know about physics and cosmology. No new hypotheses are needed to introduce them. It takes an added hypothesis to rule them out a super law of nature that says only one universe can exist. That would be an uneconomical hypothesis. Putting it another way, we have no basis for assuming that only a single universe exists. The theist argument requires two hypotheses that are unwarranted by data or theory: (1) only one universe exists and (2) God exists. A Life Principle? Despite the apparent uncongeniality of the universe to life, life is present and some people still insist that this is remarkable. Physicist Paul Davies suggests a life principle is "written into the laws of physics" or "built into the nature of the universe." Of course, nowhere in current physics, chemistry, or biology do we see any sign of a fundamental life principle, some élan vital that distinguishes life from non-life. Davies speculates, "a felicitous mix of law and chance might be generalised to cosmology, producing directional evolution from simple states, through complex, to life and mind." 25 Davies shares this notion with Nobel laureate biochemist Christian de Duve 26 and biologist Stuart Kauffman. 27 These authors all seem to view the life principle as some previously unrecognized, holistic, teleological law of nature. Nancey Murphy and other theologians, who admit that the traditional notion of a separate soul and body is no longer viable given the evidence from neuroscience, have termed this notion "nonreductive physicalism." They think they can find a place for God and the soul therein. 28

14 However, computer simulations indicate that complexity evolves from simplicity by familiar, purely reductive physical processes without the aid of any overarching holistic guiding principle. The life principle, if it exists, may be one of the type of so-called "emergent principles" found in chaos and complexity theory that naturally arise from the nonlinear, dissipative, but still purely local interactions of material particles. These cannot be called new laws of physics since they follow from already existing laws, if not by direct, mathematical proof, then by computer simulation. A Tiny Pocket of Complexity Perhaps any random universe, regardless of its properties, will naturally develop at least some tiny pockets of complexity within a vast sea of randomness, which is just what we see in our universe. Complexity is not so ubiquitous in our universe as most people seem to think. The photons in the Cosmic Microwave Background, a billion times more common than hydrogen atoms, are random to one part in a hundred thousand. The visible matter we see around us and in the sky, which impresses us so much by its complexity, constitutes one-half of one percent of the mass of the universe. Perhaps we do not need either a designer or multiple universes to explain such small deviation from chance behavior. I find it rather amusing that theists make two contradictory arguments for life requiring a creator. Sometimes you hear these from the same people. In the fine-tuning argument, the universe is so congenial to life that the universe must have been created. But, if it is so congenial, then we should expect life to evolve by natural processes. In the second argument, which one hears from creationists and anti-evolutionists, the universe is so uncongenial to life that life must have been created. In that case it is too unlikely for life to have evolved by natural

15 processes and so must have been produced by an intelligent designer. But, then life could very easily have been an improbable accident. The universe looks just as it would be expected to look if it were not created by God. From this we can conclude, beyond a reasonable doubt, that such a God does not exist. References 1 Weyl, H., Ann. Physik 59 (1919): Eddington, A. S., The Mathematical Theory of Relativity (London: Cambridge, 1923). 3 Dirac, P. A. M., Nature 139 (1937): Dicke, R. H., "Dirac's Cosmology and Mach's Principle," Nature 192 (1961): Hoyle, F., Dunbar D.N.F., Wensel, W.A., and Whaling, W., "A State in C12 Predicted from Astrophysical Evidence" Physical Review Letters 92 (1953): Carter, Brandon, "Large Number Coincidences and the Anthropic Principle in Cosmology," in M. S. Longair, ed., Confrontation of Cosmological Theory with Astronomical Data (Dordrecht: Reidel, 1974), pp , Reprinted in Leslie, John, ed., Physical Cosmology and Philosophy (New York: Macmillan, 1990). 7 Barrow, John D., and Frank J. Tipler, The Anthropic Cosmological Principle. Oxford: Oxford University Press, 1986), p Bostrom, Nick, Anthropic Bias: Observation Selection Effects in Science and Philosophy, New York: Routledge, Swinburne, Richard, "Argument from the Fine-Tuning of the Universe" in Leslie 1990, pp ; Ellis, George. Before the Beginning: Cosmology Explained (London, New York:

16 Boyars/Bowerdean, 1993); Ross, Hugh, The Creator and the Cosmos: How the Greatest Scientific Discoveries of the Century Reveal God. (Colorado Springs: Navpress. 1995). 10 For a philosophically precise rebuttal of the fine-tuning argument, see Drange, Theodore M., "The Fine-Tuning Argument Revisited," Philo 3, No. 2 (2000):38-49, online at (accessed December 29, 2004). 11 Smith, Quentin, "A Natural Explanation of the Existence and Laws of Our Universe" Australasian Journal of Philosophy 68, (1990): 22-43; Smolin, Lee, "Did the universe evolve?" Classical and Quantum Gravity 9 (1992): ; The Life of the Cosmos (Oxford: Oxford University Press, 1997). 12 Stenger, Victor J., The Unconscious Quantum: Metaphysics in Modern Physics and Cosmology (Amherst, NY: Prometheus Books, 1995). 13 Salpeter, E.E., "Accretion of Interstellar Matter by Massive Objects," Astrophysical Journal 140 (1964): ; Carr, B.J. and M.J. Rees. "The Anthropic Principle and the Structure of the Physical World," Nature 278 (1979): Stenger, The Unconscious Quantum (1995), pp ; "Natural Explanations for the Anthropic Coincidences," Philo 3(2): See, for example, Totten, R., "The Intelligent Design of the Cosmos: A Mathematical Proof" (2000), online at (accessed February 6, Aguire, Anthony, The Cold Big-Bang Cosmology as a Counter-example to Several Anthropic Arguments, Physical Review D64 (2001):

17 17 Kane, Gordon, The Particle Garden: Our Universe as Understood by Particle Physicists (New York: Addison-Wesley, 1995). 18 Davis, J.J., "The Design Argument, Cosmic 'Fine Tuning, and the Anthropic Principle," Philosophy of Religion 22 (1987): , pp Manson, Neil A.,"There Is No Adequate Definition of 'Fine-tuned for Life," Inquiry 43 (2000): Weinberg, Steven, A Designer Universe? New York Review of Books, 21 October Reprinted in The Skeptical Inquirer (September October 2001): Weinberg, Steven, Weinberg, Steven, "The Cosmological Constant Problem." Reviews of Modern Physics 61 (1989): Reiss, A., et al. "Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant." Astronomical Journal 116 (1998): ; Perlmutter, S. et al. "Measurements of Omega and Lambda from 42 High-Redshift Supernovae," Astrophysical Journal 517 (1999): Linde, Andre "Particle Physics and Inflationary Cosmology," Physics Today 40 (1987): 61-68; "The Self-Reproducing Inflationary Universe," Scientific American 271 (November, 1994): 48-55; Leslie, John. Universes (London and New York: Routledge, 1989); Guth, Alan, The Inflationary Universe (New York: Addison-Wesley, 1997). 24 See, typically, Ellis, George. Before the Beginning: Cosmology Explained (London, New York: Boyars/Bowerdean, 1993), p Davies, Paul, The Cosmic Blueprint (New York: Simon and Schuster, 1988), (Radnor, PA: The Templeton Foundation Press, 2004); "Multiverse or Design: Reflections on a Third Way" to appear in proceedings of Universe or Multiverse? Stanford University, March

18 2003, online at (accessed January 4, 2005). 26 De Duve, Christian. Vital Dust (New York: Basic Books, 1995). 27 Kauffman, Stuart, At Home in the Universe: The Search for the Laws of Self-Organization and Complexity (New York and Oxford, Oxford University Press, 1995). 28 Brown, Warren S., Nancey Murphy, and H. Newton Malony, eds, Whatever Happened to the Soul? Scientific and Theological Portraits of Human Nature, Minneapolis: Fortress Press, 1998.

Where is Fundamental Physics Heading? Nathan Seiberg IAS Apr. 30, 2014

Where is Fundamental Physics Heading? Nathan Seiberg IAS Apr. 30, 2014 Disclaimer We do not know what will be discovered. This is the reason we perform experiments. This is the reason scientific research

Lecture Outlines. Chapter 27. Astronomy Today 7th Edition Chaisson/McMillan. 2011 Pearson Education, Inc.

Lecture Outlines Chapter 27 Astronomy Today 7th Edition Chaisson/McMillan Chapter 27 The Early Universe Units of Chapter 27 27.1 Back to the Big Bang 27.2 The Evolution of the Universe More on Fundamental

What Are Stars? continued. What Are Stars? How are stars formed? Stars are powered by nuclear fusion reactions.

What Are Stars? How are stars formed? Stars are formed from clouds of dust and gas, or nebulas, and go through different stages as they age. star: a large celestial body that is composed of gas and emits

The Early Universe. Lecture 27-1

The Early Universe Lecture 27-1 Back to the Big Bang The total energy of the universe consists of both radiation and matter. As the Universe cooled, it went from being radiation dominated to being matter

The Big Bang Theory David Terr, Ph.D 4/10/13

The Big Bang Theory David Terr, Ph.D 4/10/13 The Big Bang theory is the currently accepted theory of the origin of the universe. According to this theory, the observable universe was formed approximately

WHAT EMERGED FROM THE BIG BANG?

2 WHAT EMERGED FROM THE BIG BANG? David Christian explains how the Big Bang theory developed during the 20th century. This three-part lecture focuses on how the evidence for the expansion of the Universe

Chapter 27: The Early Universe

Chapter 27: The Early Universe The plan: 1. A brief survey of the entire history of the big bang universe. 2. A more detailed discussion of each phase, or epoch, from the Planck era through particle production,

Lecture 15 Fundamentals of Physics Phys 120, Fall 2015 Cosmology

Lecture 15 Fundamentals of Physics Phys 120, Fall 2015 Cosmology A. J. Wagner North Dakota State University, Fargo, ND 58108 Fargo, October 20, 2015 Overview A history of our view of the universe The Big

REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe

REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe The End of Physics Albert A. Michelson, at the dedication of Ryerson Physics Lab, U. of Chicago, 1894 The Miracle Year - 1905 Relativity Quantum

3 HOW WERE STARS FORMED?

3 HOW WERE STARS FORMED? David Christian explains how the first stars were formed. This two-part lecture begins by focusing on what the Universe was like in its first 200 million years of existence, a

The Sun and Solar Energy

I The Sun and Solar Energy One of the most important forces behind global change on Earth is over 90 million miles distant from the planet. The Sun is the ultimate, original source of the energy that drives

Our UNIVERSE: where it all came from.

Our UNIVERSE: where it all came from. QUESTIONS OF THE DAY. How did the Universe start? How did the Universe evolve up to the present day? What is the fate of our Universe? The theory of general relativity

Solar Energy Production

Solar Energy Production We re now ready to address the very important question: What makes the Sun shine? Why is this such an important topic in astronomy? As humans, we see in the visible part of the

Astro 102 Test 5 Review Spring 2016. See Old Test 4 #16-23, Test 5 #1-3, Old Final #1-14

Astro 102 Test 5 Review Spring 2016 See Old Test 4 #16-23, Test 5 #1-3, Old Final #1-14 Sec 14.5 Expanding Universe Know: Doppler shift, redshift, Hubble s Law, cosmic distance ladder, standard candles,

Your years of toil Said Ryle to Hoyle Are wasted years, believe me. The Steady State Is out of date Unless my eyes deceive me.

Your years of toil Said Ryle to Hoyle Are wasted years, believe me. The Steady State Is out of date Unless my eyes deceive me. My telescope Has dashed your hope; Your tenets are refuted. Let me be terse:

The Nature of Evolution David L. Alles Western Washington University

The Nature of Evolution David L. Alles Western Washington University e-mail: alles@biol.wwu.edu Alles, D. L. (2005). The Nature of Evolution. The American Biology Teacher, Vol. 67, No. 1(Jan), 7-10. What

The Nature of Light Light and other forms of radiation carry information to us from distance astronomical objects Visible light is a subset of a huge spectrum of electromagnetic radiation Maxwell pioneered

When the Wall fell I was only eleven years old. I must admit that I did not fully appreciate the significance of the event at that age.

Breaking the Wall of the Beginning of Time. How Cosmology Will Tell Us What Happened Before the Big Bang. Jean-Luc Lehners, Max Planck Institute for Gravitational Physics, Potsdam, Germany. When the Wall

Stellar Evolution: a Journey through the H-R Diagram

Stellar Evolution: a Journey through the H-R Diagram Mike Montgomery 21 Apr, 2001 0-0 The Herztsprung-Russell Diagram (HRD) was independently invented by Herztsprung (1911) and Russell (1913) They plotted

Cosmology - The Story of our Universe. Raghu Rangarajan Physical Research Laboratory Ahmedabad

Cosmology - The Story of our Universe Raghu Rangarajan Physical Research Laboratory Ahmedabad What is Cosmology? Study of our Universe today galaxies, clusters, superclusters Understanding the past history

A Critique of Cosmological Natural Selection

A Critique of Cosmological Natural Selection Gordon McCabe March 7, 2004 Abstract Mathematical physicist Lee Smolin has proposed a theory of Cosmological natural selection which, he argues, explains the

Chapter 15 Cosmology: Will the universe end?

Cosmology: Will the universe end? 1. Who first showed that the Milky Way is not the only galaxy in the universe? a. Kepler b. Copernicus c. Newton d. Hubble e. Galileo Ans: d 2. The big bang theory and

Pretest Ch 20: Origins of the Universe

Name: _Answer key Pretest: _2_/ 58 Posttest: _58_/ 58 Pretest Ch 20: Origins of the Universe Vocab/Matching: Match the definition on the left with the term on the right by placing the letter of the term

TIME, SYMMETRY OF. Although everyday experience leads us to believe that time "flows" in one direction, the

TIME, SYMMETRY OF Although everyday experience leads us to believe that time "flows" in one direction, the equations of both classical and modern physics work equally well in either time direction. Since

Transcript 22 - Universe

Transcript 22 - Universe A few introductory words of explanation about this transcript: This transcript includes the words sent to the narrator for inclusion in the latest version of the associated video.

MODULE P7: FURTHER PHYSICS OBSERVING THE UNIVERSE OVERVIEW

OVERVIEW More than ever before, Physics in the Twenty First Century has become an example of international cooperation, particularly in the areas of astronomy and cosmology. Astronomers work in a number

Astro 102 Practice Test 3

Class: Date: Astro 102 Practice Test 3 Multiple Choice Identify the choice that best completes the statement or answers the question. 1. Interstellar gas clouds may collapse to form stars if they a. have

The Origin, Evolution, and Fate of the Universe

The Origin, Evolution, and Fate of the Universe Announcements n Homework # 8 is available as of this morning in OWL. Due date for is Friday Dec 9th n Exam # 3 will take place on Tuesday, December 6 th

Lecture 19 Big Bang Cosmology

The Nature of the Physical World Lecture 19 Big Bang Cosmology Arán García-Bellido 1 News Exam 2: you can do better! Presentations April 14: Great Physicist life, Controlled fusion April 19: Nuclear power,

Exampro GCSE Physics. P2 Fission, Fusion and life cycle of a star self study questions - Higher tier. Name: Class: Author: Date: Time: 68.

Exampro GCSE Physics P2 Fission, Fusion and life cycle of a star self study questions - Higher tier Name: Class: Author: Date: Time: 68 Marks: 68 Comments: Page of 26 Q. Describe briefly how stars such

The Birth of the Universe Newcomer Academy High School Visualization One

The Birth of the Universe Newcomer Academy High School Visualization One Chapter Topic Key Points of Discussion Notes & Vocabulary 1 Birth of The Big Bang Theory Activity 4A the How and when did the universe

What Energy Drives the Universe? Andrei Linde

What Energy Drives the Universe? Andrei Linde Two major cosmological discoveries:! The new-born universe experienced rapid acceleration (inflation)! A new (slow) stage of acceleration started 5 billion

Lecture 17: Dark Energy & The Big Bang

Lecture 17: Dark Energy & The Big Bang As with all course material (including homework, exams), these lecture notes are not be reproduced, redistributed, or sold in any form. Solution? ~1998 astronomers

Build Your Own Universe You will need: At least 10,000,000,000,000,00 0,000,000,000,000,000,000,00 0,000,000,000,000,000,000,00 0,000,000,000,000,000,000,00 0,000 x Down quarks At least 10,000,000,000,000,000,

WHERE DID ALL THE ELEMENTS COME FROM??

WHERE DID ALL THE ELEMENTS COME FROM?? In the very beginning, both space and time were created in the Big Bang. It happened 13.7 billion years ago. Afterwards, the universe was a very hot, expanding soup

8. Newton's Law of Gravitation

2 8. Newton's Law Gravitation Rev.nb 8. Newton's Law of Gravitation Introduction and Summary There is one other major law due to Newton that will be used in this course and this is his famous Law of Universal

How do we describe motion?

Lecture 3: The Laws of Motion and Universal Gravitation Astronomy 2020, Prof. Tom Megeath To be ignorant of motion is to be ignorant of nature -Aristotle Overview of Today s Lecture 1. Newton s three laws

Modern Ways of Dating the Universe. Martha P. Haynes Goldwin Smith Professor of Astronomy Cornell University. CAU Study Tour June 2014

Modern Ways of Dating the Universe Martha P. Haynes Goldwin Smith Professor of Astronomy Cornell University CAU Study Tour June 2014 What does the night sky look like? The disk of the Milky Way, our galaxy

How Our View of the Universe Can Change David Hedin Department of Physics -- NIU

How Our View of the Universe Can Change David Hedin Department of Physics -- NIU New Ideas in History and Science: Galileo Conference February 6, 2009 1 Introduction 1609 Galileo was the first person to

Origins of the Cosmos Summer 2016. Pre-course assessment

Origins of the Cosmos Summer 2016 Pre-course assessment In order to grant two graduate credits for the workshop, we do require you to spend some hours before arriving at Penn State. We encourage all of

The Birth of Our Universe Today s Lecture:

The Birth of Our Universe Today s Lecture: (Chapter 19, pages 454-481) Cosmic Microwave Background (CMB) The first few minutes of the Universe Inflation! Cosmic Microwave Background (CMB) A. Penzias and

Is the Universe hostile to life? Loukas Vlahos Department of Physics, Aristotle University of Thessaloniki, Greece

Is the Universe hostile to life? Loukas Vlahos Department of Physics, Aristotle University of Thessaloniki, Greece Astrophysics and Biology Last century was declared the century of Physics This century

II The Nature of Electromagnetic Radiation The Sun s energy has traveled across space as electromagnetic radiation, and that is the form in which it arrives on Earth. It is this radiation that determines

Evolution of the Universe from 13 to 4 Billion Years Ago

Evolution of the Universe from 13 to 4 Billion Years Ago Prof. Dr. Harold Geller hgeller@gmu.edu http://physics.gmu.edu/~hgeller/ Department of Physics and Astronomy George Mason University Unity in the

Thursday, 14 March, 13

The Hot Big Bang http://www.bayho.com/info/vote universe @ the big bang was dense at the Planck time (t ~ 10-43 sec) our visible universe was ~ 0.01 cm across (10 30 smaller) but any observer only sees

The Sun s Source of Energy. E= m c 2 AND STARS!

The Sun s Source of Energy E= m c 2 AND STARS! Announcements q Homework # 5 starts on Thursday, Nov 3 th. It is due on Tue, Nov 15 th q Exam # 2 will take place on Tuesday, November 8 th : q Please remember

Topic 3. Evidence for the Big Bang

Topic 3 Primordial nucleosynthesis Evidence for the Big Bang! Back in the 1920s it was generally thought that the Universe was infinite! However a number of experimental observations started to question

thermal history of the universe and big bang nucleosynthesis

thermal history of the universe and big bang nucleosynthesis Kosmologie für Nichtphysiker Markus Pössel (vertreten durch Björn Malte Schäfer) Fakultät für Physik und Astronomie, Universität Heidelberg

Our Galaxy, the Milky Way

Our Galaxy, the Milky Way In the night sky, the Milky Way appears as a faint band of light. Dusty gas clouds obscure our view because they absorb visible light. This is the interstellar medium that makes

Science Standard 4 Earth in Space Grade Level Expectations

Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal

What was before the Big Bang?

1 / 68 Std. What was before the Big Bang? of the Very Robert Brandenberger McGill University February 21, 2013 2 / 68 Outline Std. 1 What is? 2 Standard Big Bang 3 ary 4 String 5 3 / 68 Plan Std. 1 What

i>clicker Questions A scientific law is something that has been proven to be true. A. True B. False C. Only in experimental sciences.

A scientific law is something that has been proven to be true. A. True B. False C. Only in experimental sciences. i>clicker Questions The fifth planet from the sun, the sixth planet and the seventh planet

Page 1 of 12. Version 1 - published August 2016 View Creative Commons Attribution 3.0 Unported License at

High School Conceptual Progressions Model Course II Bundle 1 Matter and Energy in the Universe This is the first bundle of the High School Conceptual Progressions Model Course II. Each bundle has connections

The Crafoord Prize 2005

I N F O R M A T I O N F O R T H E P U B L I C The Royal Swedish Academy of Sciences has decided to award the Crafoord Prize in Astronomy 2005 to James Gunn, Princeton University, USA, James Peebles, Princeton

Federation of Galaxy Explorers Space Science

Federation of Galaxy Explorers Space Science Once Upon A Big Bang Learning Objectives: 1. Explain how the universe was created using the Big Bang theory. 2. Understand how the existence of Cosmic Background

Introduction to the Solar System

Introduction to the Solar System Lesson Objectives Describe some early ideas about our solar system. Name the planets, and describe their motion around the Sun. Explain how the solar system formed. Introduction

A Quantum Theory of Consciousness May Require a Paradigm Shift in Biology

A Quantum Theory of Consciousness May Require a Paradigm Shift in Biology Maurice Goodman * 1 Article School of Physics, Dublin Institute of Technology, Ireland Abstract It is often assumed that the known

Astronomy 100 Exam 2

1 Prof. Mo Exam Version A Astronomy 100 Exam 2 INSTRUCTIONS: Write your name and ID number on BOTH this sheet and the computer grading form. Use a #2 Pencil on the computer grading form. Be careful to

Astrophysics Syllabus

Astrophysics Syllabus Center for Talented Youth Johns Hopkins University Text: Astronomy Today: Stars and Galaxies, Volume II Author: Chaisson and McMillan Course Objective: The purpose of this course

ASTRONOMY/SPACE SCIENCE TEST

ASTRONOMY/SPACE SCIENCE TEST For some questions, there may be more than one correct answer. However, each question has only one best answer. Choose the single best answer from the five choices for each

How Fundamental is the Curvature of Spacetime? A Solar System Test. Abstract

Submitted to the Gravity Research Foundation s 2006 Essay Contest How Fundamental is the Curvature of Spacetime? A Solar System Test Robert J. Nemiroff Abstract Are some paths and interactions immune to

The Big Questions Spring 2008

MIT OpenCourseWare http://ocw.mit.edu The Big Questions Spring 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. Lecture Notes 1: Was There a Beginning

outline Einstein Vs Newton Deflection of light May, 29th 1919 the challenging Universe Sir Isaac Albert

the challenging Universe outline Einstein vs Newton and the solar eclipse of 1919 The missing mass problem Seeing the invisible: gravitational lensing Dark matter hunting Dr Roberto Trotta The challenging

10. Our violent origin Cosmology and the nuclear processes in the Big Bang

10. Our violent origin Cosmology and the nuclear processes in the Big Bang Our Universe is getting larger. The space between the galaxies is expanding so that we see distant galaxies in all directions

Avogadro s Number, the Mole and the Kilogram

Avogadro s Number, the Mole and the Kilogram The American Chemical Society Committee on Nomenclature, Terminology and Symbols met August 23, 2010 to discuss the definition of the mole. This was in anticipation

Basic Nuclear Concepts

Section 7: In this section, we present a basic description of atomic nuclei, the stored energy contained within them, their occurrence and stability Basic Nuclear Concepts EARLY DISCOVERIES [see also Section

The Universe. The Solar system, Stars and Galaxies

The Universe The Universe is everything. All us, the room, the U.S. the earth, the solar system, all the other stars in the Milky way galaxy, all the other galaxies... everything. How big and how old is

4 Formation of the Universe

CHAPTER 2 4 Formation of the Universe SECTION Stars, Galaxies, and the Universe BEFORE YOU READ After you read this section, you should be able to answer these questions: What is the big bang theory? How

Origin of Our Universe

Origin of Our Universe Before the Big Bang? As cosmologists begin to understand what happened just after the Big Bang, many are questioning what led up to the Big Bang (4 possibilities) 1. No previous

7. In which part of the electromagnetic spectrum are molecules most easily detected? A. visible light B. radio waves C. X rays D.

1. Most interstellar matter is too cold to be observed optically. Its radiation can be detected in which part of the electromagnetic spectrum? A. gamma ray B. ultraviolet C. infrared D. X ray 2. The space

A Century of Paradigm Shifts in our Thinking About the Universe George R. Blumenthal Chancellor, UC Santa Cruz Professor of Astronomy and Astrophysics Why start 100 years ago? Before 1910 there was no

Indiana's Academic Standards 2010 ICP Indiana's Academic Standards 2016 ICP. map) that describe the relationship acceleration, velocity and distance.

.1.1 Measure the motion of objects to understand.1.1 Develop graphical, the relationships among distance, velocity and mathematical, and pictorial acceleration. Develop deeper understanding through representations

Void Cosmology-Better Explains What Happens First, Background Radiation, Voids in Space, Hydrogen Concentrations

From the SelectedWorks of James T Struck 2015 Void Cosmology-Better Explains What Happens First, Background Radiation, Voids in Space, Hydrogen Concentrations James T Struck Available at: http://works.bepress.com/james_struck/63/

Interesting note: When the Big Bang theory came out, many Christians embraced it. Why?

Cosmology Interesting note: When the Big Bang theory came out, many Christians embraced it. Why? Because the prevailing scientific view about the Universe in the early 1900 s was: The Universe is infinite

DO PHYSICS ONLINE FROM QUANTA TO QUARKS QUANTUM (WAVE) MECHANICS

DO PHYSICS ONLINE FROM QUANTA TO QUARKS QUANTUM (WAVE) MECHANICS Quantum Mechanics or wave mechanics is the best mathematical theory used today to describe and predict the behaviour of particles and waves.

1 A Solar System Is Born

CHAPTER 3 1 A Solar System Is Born SECTION Formation of the Solar System BEFORE YOU READ After you read this section, you should be able to answer these questions: What is a nebula? How did our solar system

Elaborated by Helmut Söllinger April 2005 and February About the Nature of Dark Energy.

About the Nature of Dark Energy. Abstract The concept of dark energy has been integrated in the cosmology in order to explain some phenomena of the universe, such as the flatness of its geometry or its

165 points. Name Date Period. Column B a. Cepheid variables b. luminosity c. RR Lyrae variables d. Sagittarius e. variable stars

Name Date Period 30 GALAXIES AND THE UNIVERSE SECTION 30.1 The Milky Way Galaxy In your textbook, read about discovering the Milky Way. (20 points) For each item in Column A, write the letter of the matching

Fundamental Particles, Fundamental Questions. Elizabeth H. Simmons Dean and Professor, Lyman Briggs College

Fundamental Particles, Fundamental Questions Elizabeth H. Simmons Dean and Professor, Lyman Briggs College The smallest pieces of matter Nuclear physics and particle physics study the smallest known building

Grade 8 FCAT 2.0 Science Achievement Level Descriptions

Grade 8 FCAT 2.0 Science Achievement Level Descriptions Florida Department of Education/Office of Assessment December 2012 Grade 8 FCAT 2.0 Science Reporting Category Nature of Science Students performing

Pre-lab The Origin of the Elements

name Pre-lab The Origin of the Elements Introduction Have you ever wondered where all the matter around us comes from? It must have been created somewhere in this universe. In this exercise you will learn

Carol and Charles see their pencils fall exactly straight down.

Section 24-1 1. Carol is in a railroad car on a train moving west along a straight stretch of track at a constant speed of 120 km/h, and Charles is in a railroad car on a train at rest on a siding along

WELCOME to Aurorae In the Solar System. J.E. Klemaszewski

WELCOME to Aurorae In the Solar System Aurorae in the Solar System Sponsoring Projects Galileo Europa Mission Jupiter System Data Analysis Program ACRIMSAT Supporting Projects Ulysses Project Outer Planets

Einstein s cosmological legacy: From the big bang to black holes

School of Mathematical and Computing Sciences Te Kura Pangarau, Rorohiko Einstein s cosmological legacy: From the big bang to black holes Matt Visser Overview: 2005 marks 100 years since Einstein discovered

In January 2010, Verlinde caused a worldwide stir with the publication of On the

Erik Verlinde interview Physics has led to an astonishing range of developments in the last century from transistors, computers, the Internet, atomic bombs and space travel to the recent search for the

9 th Grade Physical Science Springfield Local Schools Common Course Syllabi. Course Description

9 th Grade Physical Science Springfield Local Schools Common Course Syllabi Course Description The purpose of the Physical Science course is to satisfy the Ohio Core science graduation requirement. The

1 Introduction. 1 There may, of course, in principle, exist other universes, but they are not accessible to our

1 1 Introduction Cosmology is the study of the universe as a whole, its structure, its origin, and its evolution. Cosmology is soundly based on observations, mostly astronomical, and laws of physics. These

Generally Covariant Quantum Mechanics

Chapter 15 Generally Covariant Quantum Mechanics by Myron W. Evans, Alpha Foundation s Institutute for Advance Study (AIAS). (emyrone@oal.com, www.aias.us, www.atomicprecision.com) Dedicated to the Late

1.3 Radioactivity and the age of the solar system

1.3. RADIOACTIVITY AND THE AGE OF THE SOLAR SYSTEM 57 1.3 Radioactivity and the age of the solar system Most of you are familiar with the phenomenon of radioactive decay: Certain elements have isotopes

Modeling Galaxy Formation

Galaxy Evolution is the study of how galaxies form and how they change over time. As was the case with we can not observe an individual galaxy evolve but we can observe different galaxies at various stages

Basics of Nuclear Physics and Fission

Basics of Nuclear Physics and Fission A basic background in nuclear physics for those who want to start at the beginning. Some of the terms used in this factsheet can be found in IEER s on-line glossary.

The Expanding Universe

Stars, Galaxies, Guided Reading and Study This section explains how astronomers think the universe and the solar system formed. Use Target Reading Skills As you read about the evidence that supports the

FIRST GRADE UNIVERSE 1 WEEK LESSON PLANS AND ACTIVITIES UNIVERSE CYCLE OVERVIEW OF FIRST GRADE UNIVERSE WEEK 1. PRE: Describing the Universe. LAB: Comparing and contrasting bodies that reflect light. POST:

THE MEANING OF THE FINE STRUCTURE CONSTANT

THE MEANING OF THE FINE STRUCTURE CONSTANT Robert L. Oldershaw Amherst College Amherst, MA 01002 USA rloldershaw@amherst.edu Abstract: A possible explanation is offered for the longstanding mystery surrounding

Chapter 22 Review Clickers. The Cosmic Perspective Seventh Edition. The Birth of the Universe Pearson Education, Inc.

Review Clickers The Cosmic Perspective Seventh Edition The Birth of the Universe What do we know about the beginning of the universe? a) It was about 6000 years ago. b) It was billions of years ago. c)

Big Bang Cosmology. Big Bang vs. Steady State

Big Bang vs. Steady State Big Bang Cosmology Perfect cosmological principle: universe is unchanging in space and time => Steady-State universe - Bondi, Hoyle, Gold. True? No! Hubble s Law => expansion

Theory of electrons and positrons

P AUL A. M. DIRAC Theory of electrons and positrons Nobel Lecture, December 12, 1933 Matter has been found by experimental physicists to be made up of small particles of various kinds, the particles of