Georges Lemaître - Wikipedia, the Free Encyclopedia Page 1 of 5

Total Page:16

File Type:pdf, Size:1020Kb

Georges Lemaître - Wikipedia, the Free Encyclopedia Page 1 of 5 Georges Lemaître - Wikipedia, the free encyclopedia Page 1 of 5 Georges Lemaître From Wikipedia, the free encyclopedia Monsignor Georges Henri Joseph Édouard Georges Lemaître Lemaître ( lemaitre.ogg 17 July 1894 – 20 June 1966) was a Belgian priest, astronomer and professor of physics at the Catholic University of Louvain. He sometimes used the title Abbé or Monseigneur . Lemaître proposed what became known as the Big Bang theory of the origin of the Universe, which he called his 'hypothesis of the primeval atom'. [1][2] Contents 1 Biography 2 Work 3 Namesakes 4 Bibliography 5 See also 6 References 7 Further reading 8 External links Biography Monseigneur Georges Lemaître, priest and scientist Born 17 July 1894 After a Charleroi, Belgium classical education at Died 20 June 1966 (aged 71) a Jesuit Leuven, Belgium secondary Nationality Belgian school (Collège du Fields Cosmology, Astrophysics Sacré-Coeur, Institutions Catholic University of Louvain Charleroi), Lemaître began studying civil engineering at the Catholic University of Louvain at the age of 17. In 1914, he interrupted his studies to serve as an artillery officer in the Belgian army for the duration of World War I. At the end of hostilities, he received the Military Cross with palms. According to the Big Bang theory, the After the war, he studied physics and mathematics, and began universe emerged from an extremely to prepare for priesthood. He obtained his doctorate in 1920 dense and hot state (singularity). Space with a thesis entitled l'Approximation des fonctions de itself has been expanding ever since, plusieurs variables réelles ( Approximation of functions of carrying galaxies with it, like raisins in a several real variables ), written under the direction of Charles rising loaf of bread. The graphic scheme de la Vallée-Poussin. He was ordained a priest in 1923. above is an artist's conception illustrating In 1923, he became a graduate student in astronomy at the the expansion of a portion of a flat http://en.wikipedia.org/wiki/Georges_Lema%C3%AEtre 5/23/2011 Georges Lemaître - Wikipedia, the free encyclopedia Page 2 of 5 University of Cambridge, spending a year at St Edmund's universe. House (now St Edmund's College, Cambridge). He worked with Arthur Eddington who initiated him into modern cosmology, stellar astronomy, and numerical analysis. He spent the following year at Harvard College Observatory in Cambridge, Massachusetts with Harlow Shapley, who had just gained a name for his work on nebulae, and at the Massachusetts Institute of Technology, where he registered for the doctorate in sciences. In 1925, on his return to Belgium, he became a part-time lecturer at the Catholic University of Louvain. He then began the report which would bring him international fame, published in 1927 in the Annales de la Société Scientifique de Bruxelles ( Annals of the Scientific Society of Brussels ), under the title "Un Univers homogène de masse constante et de rayon croissant rendant compte de la vitesse radiale des nébuleuses extragalactiques" ("A homogeneous Universe of constant mass and growing radius accounting for the radial velocity of extragalactic nebulae"). [3] In this report, he presented his new idea of an expanding Universe (he also derived Hubble's law and provided the first observational estimation of the Hubble constant) but not yet that of the primeval atom. Instead, the initial state was taken as Einstein's own finite-size static universe model. Unfortunately, the paper had little impact because the journal in which it was published was not widely read by astronomers outside of Belgium. At this time, Einstein, while not taking exception to the mathematics of Lemaître's theory, refused to accept the idea of an expanding universe; Lemaître recalled him commenting "Vos calculs sont corrects, mais votre physique est abominable"[4] ("Your math is correct, but your physics is abominable.") The same year, Lemaître returned to MIT to present his doctoral thesis on The gravitational field in a fluid sphere of uniform invariant density according to the theory of relativity . Upon obtaining the PhD, he was named Ordinary Professor at the Catholic University of Louvain. In 1930, Eddington published in the Monthly Notices of the Royal Astronomical Society a long commentary on Lemaître's 1927 article, in which he described the latter as a "brilliant solution" to the outstanding problems of cosmology. [5] The original paper was published in an abbreviated English translation in 1931, along with a sequel by Lemaître responding to Eddington's comments. [6] Lemaître was then invited to London in order to take part in a meeting of the British Association on the relation between the physical Universe and spirituality. There he proposed that the Universe expanded from an initial point, which he called the "Primeval Atom" and developed in a report published in Nature .[7] Lemaître himself also described his theory as "the Cosmic Egg exploding at the moment of the creation"; it became better known as the "Big Bang theory," a term coined by Fred Hoyle. This proposal met skepticism from his fellow scientists at the time. Eddington found Lemaître's notion unpleasant. Einstein found it suspect because he deemed it unjustifiable from a physical point of view. On the other hand, Einstein encouraged Lemaître to look into the possibility of models of non-isotropic expansion, so it's clear he was not altogether dismissive of the concept. He also appreciated Lemaître's argument that a static-Einstein model of the universe could not be sustained indefinitely into the past. In January 1933, Lemaître and Einstein, who had met on several occasions - in 1927 in Brussels, at the time of a Solvay Conference, in 1932 in Belgium, at the time of a cycle of conferences in Brussels and lastly in 1935 at Princeton - traveled together to California for a series of seminars. After the Belgian detailed his theory, Einstein stood up, applauded, and is supposed to have said, "This is the most beautiful and satisfactory explanation of creation to which I have ever listened." [citation needed ] However there is disagreement over the reporting of this quote in the newspapers of the time, and it may be that Einstein was not actually referring to the theory as a whole but to Lemaître's proposal that cosmic rays may in fact be the left over artifacts of the initial "explosion." Later research on cosmic rays by Robert Millikan would undercut this proposal, however. http://en.wikipedia.org/wiki/Georges_Lema%C3%AEtre 5/23/2011 Georges Lemaître - Wikipedia, the free encyclopedia Page 3 of 5 In 1933, when he resumed his theory of the expanding Universe and published a more detailed version in the Annals of the Scientific Society of Brussels , Lemaître would achieve his greatest glory. Newspapers around the world called him a famous Belgian scientist and described him as the leader of the new cosmological physics. On 17 March 1934, Lemaître received the Francqui Prize, the highest Belgian scientific distinction, from King Léopold III. His proposers were Albert Einstein, Charles de la Vallée-Poussin and Alexandre de Hemptinne. The members of the international jury were Eddington, Langevin and Théophile de Donder. Another distinction that the Belgian government reserves for exceptional scientists was allotted to him in 1950: the decennial prize for applied sciences for the period 1933-1942. [citation needed ] In 1936, he was elected member of the Pontifical Academy of Sciences. He took an active role there, becoming its president in March 1960 and remaining so until his death. During Vatican II he was asked to serve on the first special commission to examine the question of contraception. However, as he could not travel to Rome because of his health (he had suffered a heart attack in December 1964), Lemaître demurred, expressing his surprise that he was even chosen, at the time telling a Dominican colleague, P. Henri de Riedmatten, that he thought it was dangerous for a mathematician to venture outside of his specialty. [8] He was also named prelate ( Monsignor ) in 1960 by Pope John XXIII. In 1941, he was elected member of the Royal Academy of Sciences and Arts of Belgium.[citation needed ] In 1946, he published his book on L'Hypothèse de l'Atome Primitif ( The Primeval Atom Hypothesis ). It would be translated into Spanish in the same year and into English in 1950. [citation needed ] In 1953, he was given the very first Eddington Medal awarded by the Royal Astronomical Society.[9][10] During the 1950s, he gradually gave up part of his teaching workload, ending it completely with his éméritat in 1964. At the end of his life, he was devoted more and more to numerical calculation. He was in fact a remarkable algebraicist and arithmetical calculator. Since 1930, he used the most powerful calculating machines of the time like the Mercedes. In 1958, he introduced at the University a Burroughs E 101, the University's first electronic computer. Lemaître kept a strong interest in the development of computers and, even more, in the problems of language and programming. This interest grew with age until it absorbed him almost completely. He died on 20 June 1966, shortly after having learned of the discovery of cosmic microwave background radiation, which provided further evidence for his intuitions about the birth of the Universe. In 2005, Lemaître was voted to the 61st place of De Grootste Belg (Dutch for "The Greatest Belgian"), a Flemish television program on the VRT. In the same year he was voted to the 78th place by the audience of the Le plus grand belge (French for "The Greatest Belgian"), a television show of the RTBF. Work Lemaître was a pioneer in applying Albert Einstein's theory of general relativity to cosmology.
Recommended publications
  • Frame Covariance and Fine Tuning in Inflationary Cosmology
    FRAME COVARIANCE AND FINE TUNING IN INFLATIONARY COSMOLOGY A thesis submitted to the University of Manchester for the degree of Doctor of Philosophy in the Faculty of Science and Engineering 2019 By Sotirios Karamitsos School of Physics and Astronomy Contents Abstract 8 Declaration 9 Copyright Statement 10 Acknowledgements 11 1 Introduction 13 1.1 Frames in Cosmology: A Historical Overview . 13 1.2 Modern Cosmology: Frames and Fine Tuning . 15 1.3 Outline . 17 2 Standard Cosmology and the Inflationary Paradigm 20 2.1 General Relativity . 20 2.2 The Hot Big Bang Model . 25 2.2.1 The Expanding Universe . 26 2.2.2 The Friedmann Equations . 29 2.2.3 Horizons and Distances in Cosmology . 33 2.3 Problems in Standard Cosmology . 34 2.3.1 The Flatness Problem . 35 2.3.2 The Horizon Problem . 36 2 2.4 An Accelerating Universe . 37 2.5 Inflation: More Questions Than Answers? . 40 2.5.1 The Frame Problem . 41 2.5.2 Fine Tuning and Initial Conditions . 45 3 Classical Frame Covariance 48 3.1 Conformal and Weyl Transformations . 48 3.2 Conformal Transformations and Unit Changes . 51 3.3 Frames in Multifield Scalar-Tensor Theories . 55 3.4 Dynamics of Multifield Inflation . 63 4 Quantum Perturbations in Field Space 70 4.1 Gauge Invariant Perturbations . 71 4.2 The Field Space in Multifield Inflation . 74 4.3 Frame-Covariant Observable Quantities . 78 4.3.1 The Potential Slow-Roll Hierarchy . 81 4.3.2 Isocurvature Effects in Two-Field Models . 83 5 Fine Tuning in Inflation 88 5.1 Initial Conditions Fine Tuning .
    [Show full text]
  • PDF Solutions
    Solutions to exercises Solutions to exercises Exercise 1.1 A‘stationary’ particle in anylaboratory on theEarth is actually subject to gravitationalforcesdue to theEarth andthe Sun. Thesehelp to ensure that theparticle moveswith thelaboratory.Ifstepsweretaken to counterbalance theseforcessothatthe particle wasreally not subject to anynet force, then the rotation of theEarth andthe Earth’sorbital motionaround theSun would carry thelaboratory away from theparticle, causing theforce-free particle to followacurving path through thelaboratory.Thiswouldclearly show that the particle didnot have constantvelocity in the laboratory (i.e.constantspeed in a fixed direction) andhence that aframe fixed in the laboratory is not an inertial frame.More realistically,anexperimentperformed usingthe kind of long, freely suspendedpendulum known as a Foucaultpendulum couldreveal the fact that a frame fixed on theEarth is rotating andthereforecannot be an inertial frame of reference. An even more practical demonstrationisprovidedbythe winds,which do not flowdirectly from areas of high pressure to areas of lowpressure because of theEarth’srotation. - Exercise 1.2 TheLorentzfactor is γ(V )=1/ 1−V2/c2. (a) If V =0.1c,then 1 γ = - =1.01 (to 3s.f.). 1 − (0.1c)2/c2 (b) If V =0.9c,then 1 γ = - =2.29 (to 3s.f.). 1 − (0.9c)2/c2 Notethatitisoften convenient to write speedsinterms of c instead of writingthe values in ms−1,because of thecancellation between factorsofc. ? @ AB Exercise 1.3 2 × 2 M = Theinverse of a matrix CDis ? @ 1 D −B M −1 = AD − BC −CA. Taking A = γ(V ), B = −γ(V )V/c, C = −γ(V)V/c and D = γ(V ),and noting that AD − BC =[γ(V)]2(1 − V 2/c2)=1,wehave ? @ γ(V )+γ(V)V/c [Λ]−1 = .
    [Show full text]
  • Hubble's Evidence for the Big Bang
    Hubble’s Evidence for the Big Bang | Instructor Guide Students will explore data from real galaxies to assemble evidence for the expansion of the Universe. Prerequisites ● Light spectra, including graphs of intensity vs. wavelength. ● Linear (y vs x) graphs and slope. ● Basic measurement statistics, like mean and standard deviation. Resources for Review ● Doppler Shift Overview ● Students will consider what the velocity vs. distance graph should look like for 3 different types of universes - a static universe, a universe with random motion, and an expanding universe. ● In an online interactive environment, students will collect evidence by: ○ using actual spectral data to calculate the recession velocities of the galaxies ○ using a “standard ruler” approach to estimate distances to the galaxies ● After they have collected the data, students will plot the galaxy velocities and distances to determine what type of model Universe is supported by their data. Grade Level: 9-12 Suggested Time One or two 50-minute class periods Multimedia Resources ● Hubble and the Big Bang WorldWide Telescope Interactive ​ Materials ● Activity sheet - Hubble’s Evidence for the Big Bang Lesson Plan The following represents one manner in which the materials could be organized into a lesson: Focus Question: ● How does characterizing how galaxies move today tell us about the history of our Universe? Learning Objective: ● SWBAT collect and graph velocity and distance data for a set of galaxies, and argue that their data set provides evidence for the Big Bang theory of an expanding Universe. Activity Outline: 1. Engage a. Invite students to share their ideas about these questions: i. Where did the Universe come from? ii.
    [Show full text]
  • The Big-Bang Theory AST-101, Ast-117, AST-602
    AST-101, Ast-117, AST-602 The Big-Bang theory Luis Anchordoqui Thursday, November 21, 19 1 17.1 The Expanding Universe! Last class.... Thursday, November 21, 19 2 Hubbles Law v = Ho × d Velocity of Hubbles Recession Distance Constant (Mpc) (Doppler Shift) (km/sec/Mpc) (km/sec) velocity Implies the Expansion of the Universe! distance Thursday, November 21, 19 3 The redshift of a Galaxy is: A. The rate at which a Galaxy is expanding in size B. How much reader the galaxy appears when observed at large distances C. the speed at which a galaxy is orbiting around the Milky Way D. the relative speed of the redder stars in the galaxy with respect to the blues stars E. The recessional velocity of a galaxy, expressed as a fraction of the speed of light Thursday, November 21, 19 4 The redshift of a Galaxy is: A. The rate at which a Galaxy is expanding in size B. How much reader the galaxy appears when observed at large distances C. the speed at which a galaxy is orbiting around the Milky Way D. the relative speed of the redder stars in the galaxy with respect to the blues stars E. The recessional velocity of a galaxy, expressed as a fraction of the speed of light Thursday, November 21, 19 5 To a first approximation, a rough maximum age of the Universe can be estimated using which of the following? A. the age of the oldest open clusters B. 1/H0 the Hubble time C. the age of the Sun D.
    [Show full text]
  • The Discovery of the Expansion of the Universe
    galaxies Review The Discovery of the Expansion of the Universe Øyvind Grøn Faculty of Technology, Art and Design, Oslo Metropolitan University, PO Box 4 St. Olavs Plass, NO-0130 Oslo, Norway; [email protected]; Tel.: +047-90-94-64-60 Received: 2 November 2018; Accepted: 29 November 2018; Published: 3 December 2018 Abstract: Alexander Friedmann, Carl Wilhelm Wirtz, Vesto Slipher, Knut E. Lundmark, Willem de Sitter, Georges H. Lemaître, and Edwin Hubble all contributed to the discovery of the expansion of the universe. If only two persons are to be ranked as the most important ones for the general acceptance of the expansion of the universe, the historical evidence points at Lemaître and Hubble, and the proper answer to the question, “Who discovered the expansion of the universe?”, is Georges H. Lemaître. Keywords: cosmology history; expansion of the universe; Lemaitre; Hubble 1. Introduction The history of the discovery of the expansion of the universe is fascinating, and it has been thoroughly studied by several historians of science. (See, among others, the contributions to the conference Origins of the expanding universe [1]: 1912–1932). Here, I will present the main points of this important part of the history of the evolution of the modern picture of our world. 2. Einstein’s Static Universe Albert Einstein completed the general theory of relativity in December 1915, and the theory was presented in an impressive article [2] in May 1916. He applied [3] the theory to the construction of a relativistic model of the universe in 1917. At that time, it was commonly thought that the universe was static, since one had not observed any large scale motions of the stars.
    [Show full text]
  • Cosmology and Religion — an Outsider's Study
    Cosmology and Religion — An Outsider’s Study (Big Bang and Creation) Dezs˝oHorváth [email protected] KFKI Research Institute for Particle and Nuclear Physics (RMKI), Budapest and Institute of Nuclear Research (ATOMKI), Debrecen Dezs˝oHorváth: Cosmology and religion Wien, 10.03.2010 – p. 1/46 Outline Big Bang, Inflation. Lemaître and Einstein. Evolution and Religion. Big Bang and Hinduism, Islam, Christianity. Saint Augustine on Creation. Saint Augustine on Time. John Paul II and Stephen Hawking. Dezs˝oHorváth: Cosmology and religion Wien, 10.03.2010 – p. 2/46 Warning Physics is an exact science (collection of formulae) It is based on precise mathematical formalism. A theory is valid if quantities calculated with it agree with experiment. Real physical terms are measurable quantities, words are just words. Behind the words there are precise mathematics and experimental evidence What and how: Physics Why: philosopy? And theology? Dezs˝oHorváth: Cosmology and religion Wien, 10.03.2010 – p. 3/46 What is Cosmology? Its subject is the Universe as a whole. How did it form? (Not why?) Static, expanding or shrinking? Open or closed? Its substance, composition? Its past and future? Dezs˝oHorváth: Cosmology and religion Wien, 10.03.2010 – p. 4/46 The Story of the Big Bang Theory Red Shift of Distant Galaxies Henrietta S. Leavitt Vesto Slipher Distances to galaxies Red shift of galaxies 1908–1912 1912 Dezs˝oHorváth: Cosmology and religion Wien, 10.03.2010 – p. 5/46 Expanding Universe Cosmological principle: if the expansion linear A. Friedmann v(B/A) = v(C/B) ⇒ v(C/A)=2v(B/A) the Universe is homogeneous, it has no special point.
    [Show full text]
  • Dark Universe: Science & Literacy Activity for Grades 9-12
    Dark Universe Science & Literacy Activity GRADES 9-12 OVERVIEW Common Core State Standards: This activity, which is aligned to the Common Core State Standards (CCSS) WHST.9-12.2, WHST.9-12.8, WHST.9-12.9, for English Language Arts, introduces students to scientific knowledge and RST.9-12.1, RST.9-12.2, RST.9-12.4, RST.9-12.7, language related to the study of cosmology. Students will read content-rich RST.9-12.10 texts, view the Dark Universe space show, and use what they have learned New York State Science Core Curriculum: to complete a CCSS-aligned writing task, creating an illustrated text about PS 1.2a how scientists study the history of the universe. Next Generation Science Standards: Materials in this activity include: PE HS-ESS1-2 • Teacher instructions for: DCI ESS1.A: The Universe and Its Stars o Pre-visit student reading The Big Bang theory is supported by o Viewing the Dark Universe space show observations of distant galaxies receding o Post-visit writing task from our own, of the measured composition • Text for student reading: “Case Study: The Cosmic Microwave Background ” of stars and non-stellar gases, and of the • Student Writing Guidelines maps of spectra of the primordial radiation (cosmic microwave background) that still • Teacher rubric for writing assessment fills the universe. SUPPORTS FOR DIVERSE LEARNERS: An Overview This resource has been designed to engage all learners with the principles of Universal Design for Learning in mind. It represents information in multiple ways and offers multiple ways for your students to engage with content as they read about, discuss, view, and write about scientific concepts.
    [Show full text]
  • A the Highland Park Enews August 1, 2016 221 S
    , A The Highland Park eNews August 1, 2016 www.hpboro.com 221 S. Fifth Avenue, Highland Park, NJ, 08904 732-572-3400 Events & Meetings Tuesday, August 2 Book Break 3-5 yr. old Story Time 11:30 a.m., Public Library Tuesday, August 2 Teen Sidewalk Chalk Graffiti and Games 3:00 p.m., Public Library Tuesday, August 2 National Night Out rd 5:00 p.m., North 3 /Raritan Ave Tuesday, August 2 The NJ Youth Corps of Middlesex County was on-hand Wednesday, July 27th working the International Film Festival – Second Mother 1st stage of our Senior/Youth Center beautification project. Weeds were pulled, shrubs trimmed, and beds mulched. We can't wait to see how the project progresses. Thank 6:30 p.m., Public Library you to all involved. Wednesday, August 3 Borough Council Meeting Re: Buck Woods Having a Blast at the Highland Park Recreation Summer Camp 7:00 p.m., Borough Council Wednesday, August 3 Community Food Pantry 7:00 p.m., Senior/Youth Center Tuesday, August 9 Book Break 3-5 yr. old Story Time 11:30 a.m., Public Library Tuesday, August 9 Summer Afternoon Film Series –Rudy (PG) 3:00 p.m., Public Library Summer in Highland Park is always fun, especially for the many kids who attend our Tuesday, August 9 Recreation Summer Camp. This year we are averaging 175 campers per week in our day International Film Series – Coming Home camp, sports camp, teen camp, and new special needs camp. This week’s sports camp is 6:30 p.m., Public Library soccer, and next week will be tennis or wrestling.
    [Show full text]
  • Georges Lemaître & the Big Bang
    Monsignor Georges Lemaître & Albert Einstein, 1933 In the winter of 1998, two separate teams of astronomers in Berkeley, California, made a similar, startling discovery. They were both observing supernovae – exploding stars visible over great distances – to see how fast the universe is expanding. In accordance with prevailing scientific wisdom, the astronomers expected to find the rate of expansion to be decreasing, Instead they found it to be increasing – a discovery which has since "shaken astronomy to its core" (Astronomy, October 1999). This discovery would have come as no surprise to Georges Lemaitre (1894-1966), a Belgian mathematician and Catholic priest who developed the theory of the Big Bang. Lemaitre described the beginning of the universe as a burst of fireworks, comparing galaxies to the burning embers spreading out in a growing sphere from the center of the burst. He believed this burst of fireworks was the beginning of time, taking place on "a day without yesterday." After decades of struggle, other scientists came to accept the Big Bang as fact. But while most scientists – including the mathematician Stephen Hawking -- predicted that gravity would eventually slow down the expansion of the universe and make the universe fall back toward its center, Lemaitre believed that the universe would keep expanding. He argued that the Big Bang was a unique event, while other scientists believed that the universe would shrink to the point of another Big Bang, and so on. The observations made in Berkeley supported Lemaitre's contention that the Big Bang was in fact "a day without yesterday." When Georges Lemaitre was born in Charleroi, Belgium, most scientists thought that the universe was infinite in age and constant in its general appearance.
    [Show full text]
  • 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.
    [Show full text]
  • The Universe of General Relativity, Springer 2005.Pdf
    Einstein Studies Editors: Don Howard John Stachel Published under the sponsorship of the Center for Einstein Studies, Boston University Volume 1: Einstein and the History of General Relativity Don Howard and John Stachel, editors Volume 2: Conceptual Problems of Quantum Gravity Abhay Ashtekar and John Stachel, editors Volume 3: Studies in the History of General Relativity Jean Eisenstaedt and A.J. Kox, editors Volume 4: Recent Advances in General Relativity Allen I. Janis and John R. Porter, editors Volume 5: The Attraction of Gravitation: New Studies in the History of General Relativity John Earman, Michel Janssen and John D. Norton, editors Volume 6: Mach’s Principle: From Newton’s Bucket to Quantum Gravity Julian B. Barbour and Herbert Pfister, editors Volume 7: The Expanding Worlds of General Relativity Hubert Goenner, Jürgen Renn, Jim Ritter, and Tilman Sauer, editors Volume 8: Einstein: The Formative Years, 1879–1909 Don Howard and John Stachel, editors Volume 9: Einstein from ‘B’ to ‘Z’ John Stachel Volume 10: Einstein Studies in Russia Yuri Balashov and Vladimir Vizgin, editors Volume 11: The Universe of General Relativity A.J. Kox and Jean Eisenstaedt, editors A.J. Kox Jean Eisenstaedt Editors The Universe of General Relativity Birkhauser¨ Boston • Basel • Berlin A.J. Kox Jean Eisenstaedt Universiteit van Amsterdam Observatoire de Paris Instituut voor Theoretische Fysica SYRTE/UMR8630–CNRS Valckenierstraat 65 F-75014 Paris Cedex 1018 XE Amsterdam France The Netherlands AMS Subject Classification (2000): 01A60, 83-03, 83-06 Library of Congress Cataloging-in-Publication Data The universe of general relativity / A.J. Kox, editors, Jean Eisenstaedt. p.
    [Show full text]
  • 22. Big-Bang Cosmology
    1 22. Big-Bang Cosmology 22. Big-Bang Cosmology Revised August 2019 by K.A. Olive (Minnesota U.) and J.A. Peacock (Edinburgh U.). 22.1 Introduction to Standard Big-Bang Model The observed expansion of the Universe [1–3] is a natural (almost inevitable) result of any homogeneous and isotropic cosmological model based on general relativity. However, by itself, the Hubble expansion does not provide sufficient evidence for what we generally refer to as the Big-Bang model of cosmology. While general relativity is in principle capable of describing the cosmology of any given distribution of matter, it is extremely fortunate that our Universe appears to be homogeneous and isotropic on large scales. Together, homogeneity and isotropy allow us to extend the Copernican Principle to the Cosmological Principle, stating that all spatial positions in the Universe are essentially equivalent. The formulation of the Big-Bang model began in the 1940s with the work of George Gamow and his collaborators, Ralph Alpher and Robert Herman. In order to account for the possibility that the abundances of the elements had a cosmological origin, they proposed that the early Universe was once very hot and dense (enough so as to allow for the nucleosynthetic processing of hydrogen), and has subsequently expanded and cooled to its present state [4,5]. In 1948, Alpher and Herman predicted that a direct consequence of this model is the presence of a relic background radiation with a temperature of order a few K [6,7]. Of course this radiation was observed 16 years later as the Cosmic Microwave Background (CMB) [8].
    [Show full text]