COSMOLOGY K U Research Briefing
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Finding the Radiation from the Big Bang
Finding The Radiation from the Big Bang P. J. E. Peebles and R. B. Partridge January 9, 2007 4. Preface 6. Chapter 1. Introduction 13. Chapter 2. A guide to cosmology 14. The expanding universe 19. The thermal cosmic microwave background radiation 21. What is the universe made of? 26. Chapter 3. Origins of the Cosmology of 1960 27. Nucleosynthesis in a hot big bang 32. Nucleosynthesis in alternative cosmologies 36. Thermal radiation from a bouncing universe 37. Detecting the cosmic microwave background radiation 44. Cosmology in 1960 52. Chapter 4. Cosmology in the 1960s 53. David Hogg: Early Low-Noise and Related Studies at Bell Lab- oratories, Holmdel, N.J. 57. Nick Woolf: Conversations with Dicke 59. George Field: Cyanogen and the CMBR 62. Pat Thaddeus 63. Don Osterbrock: The Helium Content of the Universe 70. Igor Novikov: Cosmology in the Soviet Union in the 1960s 78. Andrei Doroshkevich: Cosmology in the Sixties 1 80. Rashid Sunyaev 81. Arno Penzias: Encountering Cosmology 95. Bob Wilson: Two Astronomical Discoveries 114. Bernard F. Burke: Radio astronomy from first contacts to the CMBR 122. Kenneth C. Turner: Spreading the Word — or How the News Went From Princeton to Holmdel 123. Jim Peebles: How I Learned Physical Cosmology 136. David T. Wilkinson: Measuring the Cosmic Microwave Back- ground Radiation 144. Peter Roll: Recollections of the Second Measurement of the CMBR at Princeton University in 1965 153. Bob Wagoner: An Initial Impact of the CMBR on Nucleosyn- thesis in Big and Little Bangs 157. Martin Rees: Advances in Cosmology and Relativistic Astro- physics 163. -
The Philosophy of Cosmology Edited by Khalil Chamcham , Joseph Silk , John D
Cambridge University Press 978-1-107-14539-9 — The Philosophy of Cosmology Edited by Khalil Chamcham , Joseph Silk , John D. Barrow , Simon Saunders Frontmatter More Information THE PHILOSOPHY OF COSMOLOGY Following a long-term international collaboration between leaders in cosmology and the philosophy of science, this volume addresses foundational questions at the limits of sci- ence across these disciplines, questions raised by observational and theoretical progress in modern cosmology. Space missions have mapped the Universe up to its early instants, opening up questions on what came before the Big Bang, the nature of space and time, and the quantum origin of the Universe. As the foundational volume of an emerging academic discipline, experts from relevant fields lay out the fundamental problems of contemporary cosmology and explore the routes toward possible solutions. Written for physicists and philosophers, the emphasis is on con- ceptual questions, and on ways of framing them that are accessible to each community and to a still wider readership: those who wish to understand our modern vision of the Universe, its unavoidable philosophical questions, and its ramifications for scientific methodology. KHALIL CHAMCHAM is a researcher at the University of Oxford. He acted as the exec- utive director of the UK collaboration on the ‘Philosophy of Cosmology’ programme. His main research interests are in the chemical evolution of galaxies, nucleosynthesis, dark matter, and the concept of time. He has co-authored four books and co-edited ten, includ- ing From Quantum Fluctuations to Cosmological Structures and Science and Search for Meaning. JOSEPH SILK FRS is Homewood Professor at the Johns Hopkins University, Research Scientist at the Institut d’Astrophysique de Paris, CNRS and Sorbonne Universities, and Senior Fellow at the Beecroft Institute for Particle Astrophysics at the University of Oxford. -
Religion in an Age of Science by Ian Barbour
Religion in an Age of Science return to religion-online 47 Religion in an Age of Science by Ian Barbour Ian G. Barbour is Professor of Science, Technology, and Society at Carleton College, Northefiled, Minnesota. He is the author of Myths, Models and Paradigms (a National Book Award), Issues in Science and Religion, and Science and Secularity, all published by HarperSanFrancisco. Published by Harper San Francisco, 1990. This material was prepared for Religion Online by Ted and Winnie Brock. (ENTIRE BOOK) An excellent and readable summary of the role of religion in an age of science. Barbour's Gifford Lectures -- the expression of a lifetime of scholarship and deep personal conviction and insight -- including a clear and helpful analysis of process theology. Preface What is the place of religion in an age of science? How can one believe in God today? What view of God is consistent with the scientific understanding of the world? My goals are to explore the place of religion in an age of science and to present an interpretation of Christianity that is responsive to both the historical tradition and contemporary science. Part 1: Religion and the Methods of Science Chapter 1: Ways of Relating Science and Religion A broad description of contemporary views of the relationship between the methods of science and those of religion: Conflict, Independence, Dialogue, and Integration. Chapter 2: Models and Paradigms This chapter examines some parallels between the methods of science and those of religion: the interaction of data and theory (or experience and interpretation); the historical character of the interpretive community; the use of models; and the influence of paradigms or programs. -
Publications John N
Publications John N. Bahcall I. BOOKS AUTHORED 1. The Redshift Controversy, G. B. Field, ed.; H. C. Arp and J. N. Bahcall, auths., Addison-Wesley (1973). Redshifts as Distance Indicators, J. N. Bahcall, pp. 61–121. 2. Neutrino Astrophysics (Cambridge: Cambridge University Press) (1989 April). II. BOOKS EDITED 1. The Galaxy and the Solar System, R. Smoluchowski, J. N. Bahcall, and M. S. Matthews, eds., University of Arizona Press (1986). 2. Dark Matter in the Universe, J. N. Bahcall, T. Piran, and S. Weinberg, eds., World Scientific Publications (1988). 3. The Decade of Discovery in Astronomy and Astrophysics, J. N. Bahcall, Chairman, ed., National Academy Press (1991). 4. Solar Neutrinos, The First Thirty Years, John N. Bahcall, Raymond Davis, Jr., Peter Parker, Alexei Smirnov, and Roger Ulrich, eds., first paperback edition (Westview Press, 2002). 5. Unsolved Problems in Astrophysics, John N. Bahcall and Jeremiah P. Ostriker, eds., Princeton University Press (1997). 6. Dark Matter in the Universe, Second Edition, John Bahcall, Tsvi Piran, and Steven Weinberg, eds., World Scientific (2004). 7. Neutrino Physics, Its Impact on Particle Physics, Astrophysics and Cosmology; Proceedings of the Carolina Sym- posium on Neutrino Physics, J. Bahcall, W. Haxton, K. Kubodera, and C. Poole, eds., World Scientific (2001). III. TECHNICAL PAPERS 1. The Mass of the Muon’s Neutrino (J. N. Bahcall and R. B. Curtis), Il Nuovo Cimento 21, pp. 422–429 (1961 August). 2. Theory of Bound-State Beta Decay, Phys. Rev. 124, pp. 495–499 (1961 October 15). 3. Virial Theorem for Many-Electron Dirac Systems, Phys. Rev. 124, No. 3, pp. -
Index to JRASC Volumes 61-90 (PDF)
THE ROYAL ASTRONOMICAL SOCIETY OF CANADA GENERAL INDEX to the JOURNAL 1967–1996 Volumes 61 to 90 inclusive (including the NATIONAL NEWSLETTER, NATIONAL NEWSLETTER/BULLETIN, and BULLETIN) Compiled by Beverly Miskolczi and David Turner* * Editor of the Journal 1994–2000 Layout and Production by David Lane Published by and Copyright 2002 by The Royal Astronomical Society of Canada 136 Dupont Street Toronto, Ontario, M5R 1V2 Canada www.rasc.ca — [email protected] Table of Contents Preface ....................................................................................2 Volume Number Reference ...................................................3 Subject Index Reference ........................................................4 Subject Index ..........................................................................7 Author Index ..................................................................... 121 Abstracts of Papers Presented at Annual Meetings of the National Committee for Canada of the I.A.U. (1967–1970) and Canadian Astronomical Society (1971–1996) .......................................................................168 Abstracts of Papers Presented at the Annual General Assembly of the Royal Astronomical Society of Canada (1969–1996) ...........................................................207 JRASC Index (1967-1996) Page 1 PREFACE The last cumulative Index to the Journal, published in 1971, was compiled by Ruth J. Northcott and assembled for publication by Helen Sawyer Hogg. It included all articles published in the Journal during the interval 1932–1966, Volumes 26–60. In the intervening years the Journal has undergone a variety of changes. In 1970 the National Newsletter was published along with the Journal, being bound with the regular pages of the Journal. In 1978 the National Newsletter was physically separated but still included with the Journal, and in 1989 it became simply the Newsletter/Bulletin and in 1991 the Bulletin. That continued until the eventual merger of the two publications into the new Journal in 1997. -
How Special Is Our Universe? Fine-Tuning and Cosmological Natural Selection
6 DECEMBER 2017 How Special is our Universe? Fine-Tuning and Cosmological Natural Selection PROFESSOR JOSEPH SILK Fine-tuning in Nature If the fundamental constants of nature differed from their measured values, life as we know it would not have emerged. Imagine a universe in which the fine structure constant was slightly larger or smaller than the actual value that we measure. Stars like the sun are witness to a titanic battle between the forces of electromagnetism and gravity. The solar system formed from the ashes of burnt-out stars. Displace this equilibrium slightly and the very existence of nuclear-burning stars is at risk. In such a universe, stars would never have formed, or might have collapsed to black holes. Perhaps there are many other universes, most of which are uncongenial to life. Theories of the multiverse are designed to accommodate the possibility that there are only incredibly rare examples of life-containing universes. We live in one of these, whether by cosmological natural selection or by the consequences of an ultimate theory that has yet to be formulated. Simple physical arguments can account for the fundamental scaling relations of stars and galaxies. To be fair to simulators, the dispersion in these relations contains most of the relevant physics, and can only be adequately explored via state-of-the-art numerical simulations over a vast and currently inadequate dynamical range. Here however I focus here not on the scaling laws but on the actual scales: characteristic, minimum and maximum, from protostars to stars, galaxies and supermassive black holes. Unlike the scientists of antiquity, astronomers today have two significant advantages. -
Astrophysics in 1997
UC Irvine UC Irvine Previously Published Works Title Astrophysics in 1997 Permalink https://escholarship.org/uc/item/5q53b2pm Journal PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 110(745) ISSN 0004-6280 Authors Trimble, V McFadden, LA Publication Date 1998-03-01 DOI 10.1086/316143 License https://creativecommons.org/licenses/by/4.0/ 4.0 Peer reviewed eScholarship.org Powered by the California Digital Library University of California Publications of the Astronomical Society of the Pacific, 110:223–267, 1998 March ᭧ 1998. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A. Astrophysics in 1997 Virginia Trimble1,2 and Lucy-Ann McFadden1 Received 1997 December 9; accepted 1998 January 2 ABSTRACT. Martian marvels, a gamma-ray burster with a redshift, Galileo converses with Ganymede, a record galactic redshift of 4.92, and much else. Fiscal 1997 was definitely an exciting year for astronomers. We have tried hard to hit all the obvious highlights, but also to report more gradual progress on traditional problems of understanding planets, stars, galaxies, and the universe. Though the year was saddened by the loss of many valued colleagues, we nevertheless indulge in occasional soupc¸ons of frivolity. 1. INTRODUCTION ternational Astronomical Union numbered 112. Members of It is with considerable regret that we record Ap97 as the last the American astronomical community (meaning current or review we will prepare for retiring editor Howard E. Bond. former members and prizewinners of AAS and ASP Bruce The series was originally his idea (though he must have felt Medalists) who died during the reference year, or whose deaths occasionally like the parent of Rosemary’s Baby), and he has were belatedly announced, include Viktor A. -
Numerical Relativity on Cosmological Past Null Cones
Numerical Relativity on Cosmological Past Null Cones A thesis submitted in fulfilment of the requirements for the degree of Doctor of Philosophy (Science) Rhodes University Department of Mathematics (Pure & Applied) by Petrus Johannes van der Walt Supervised by: Prof. Nigel T. Bishop December 2012 Abstract The observational approach to cosmology is the endeavour to reconstruct the geometry of the Universe using only data that is theoretically verifiable within the causal boundaries of a cosmological observer. Using this approach, it was shown in [36] that given ideal cosmological observations, the only essential assumption necessary to determine the geometry of the Universe is a theory of gravity. Assuming General Relativity, the full set of Einstein field equations (EFEs) can be used to reconstruct the geometry of the Universe using direct observations on the past null cone (PNC) as initial conditions. Observationally and theoretically this is a very ambitious task and therefore, current developments have been restricted to spherically symmetric dust models while only relaxing the usual assumption of homogeneity in the radial direction. These restricted models are important for the development of theoretical foundations and also useful as verification models since they avoid the circularity of verifying what has already been assumed. The work presented in this thesis is the development of such a model where numerical relativity (NR) is used to simulate the observable universe. Similar to the work of Ellis and co-workers [36], a reference frame based on the PNC is used. The reference frame used here, however, is based on that of the characteristic formalism of NR, which was developed for calculating the propagation of gravitational waves. -
1 Katherine Freese George E. Uhlenbeck Professor of Physics
1 Katherine Freese George E. Uhlenbeck Professor of Physics Department of Physics University of Michigan Ann Arbor, MI 48109 (734) 604-1325 (cell) [email protected] Citizenship: USA Education: Sept. 1973 - June 1974: Massachusetts Institute of Technology Sept. 1974 - June 1977: Princeton University, B.A. in Physics '77 Sept. 1979 - Jan. 1982: Columbia University, M.A. in Physics '81 Feb. 1982 - Aug. 1984: University of Chicago, Ph.D. in Physics '84 Thesis Advisor: Dr. David N. Schramm Positions: 1984-85 Postdoctoral fellow at Harvard Center for Astrophysics 1985-87 Postdoctoral fellow at Institute for Theoretical Physics, Santa Barbara, California 1987-88 Presidential Fellow at UC Berkeley 1988-91 Assistant Professor of Physics, Massachusetts Institute of Technology 1991-99 Associate Professor of Physics (with tenure), University of Michigan 1999-2009 Professor of Physics, University of Michigan 2009{ George E. Uhlenbeck Professor of Physics, University of Michigan Awards, Honors and National/International Service: 2012: awarded Honorary Doctorate (Honoris Causa) at the University of Stockholm 2012: Simons Foundation Fellowship in Theoretical Physics 2011-2012: Member, Executive Board of the American Physical Society 2009{ : named George E. Uhlenbeck Professor of Physics at the Univ. of Michigan 2009{ : named Fellow, American Physical Society 2008-2113: American Physical Society General Councillor 2005-2008: Member, Astronomy and Astrophysics Advisory Committee (AAAC) mandated by Congress 2007: Visiting Professor, Perimeter Institute for Theoretical Physics 2006-2007: Visiting Miller Professor, UC Berkeley 2006: NSF Panel to evaluate Theory Proposals 2006: Reviewer, Deep Underground Science and Engineering Laboratory (DUSEL) 2006-2007: Member, Dark Matter Scientific Advisory Group (DMSAG) reporting to DOE and NSF 2005: External Review Committee, Physics Dept. -
Probes of the Early Universe
Probes of the Early Universe by Max Erik Tegmark B.A., Stockholm School of Economics, 1989 B.A., Royal Institute of Technology, Stockholm, 1990 M.A., University of California at Berkeley, 1992 A dissertation submitted in satisfaction of the final requirement for the degree of Doctor of Philosophy in Physics in the Graduate Division of the University of California at Berkeley Committee in charge: Professor Joseph Silk, Chair Professor Bernard Sadoulet Professor Hyron Spinrad April 1994 The dissertation of Max Tegmark is approved: Chair Date Date Date University of California at Berkeley April 1994 Probes of the Early Universe °c 1994 by Max Tegmark Abstract Probes of the Early Universe by Max Erik Tegmark Doctor of Philosophy in Physics University of California at Berkeley Professor Joseph Silk, Chair One of the main challenges in cosmology is to quantify how small density fluctuations at the recombination epoch z ¼ 103 evolved into the galaxies and the large-scale structure we observe in the universe today. This thesis discusses ways of probing the intermediate epoch, focusing on the thermal history. The main emphasis is on the role played by non- linear feedback, where a small fraction of matter forming luminous objects can inject enough energy into the inter-galactic medium (IGM) to radically alter subsequent events. The main conclusions are: ² Early structures corresponding to rare Gaussian peaks in a cold dark matter (CDM) model can photoionize the IGM early enough to appreciably smooth out fluctuations in the cosmic microwave background radiation (CBR), provided that these early struc- 8 tures are quite small, no more massive than about 10 M¯. -
Shaping the Future
The Royal Society 6–9 Carlton House Terrace London SW1Y 5AG tel +44 (0)20 7451 2500 fax +44 (0)20 7930 2170 email: [email protected] www.royalsoc.ac.uk The Royal Society is a Fellowship of 1,400 outstanding Invest in future scientific leaders and in innovation Influence policymaking with individuals from all areas of science, engineering and the best scientific advice Invigorate science and mathematics education Increase medicine, who form a global scientific network of the access to the best science internationally Inspire an interest in the joy, wonder highest calibre. The Fellowship is supported by a and excitement of scientific discovery Invest in future scientific leaders and in permanent staff of 124 with responsibility for the innovation Influence policymaking with the best scientific advice Invigorate science and mathematics education day-to-day management of the Society and its activities. Increase access to the best science internationally Inspire an interest in the joy, As we prepare for our 350th anniversary in 2010, we are wonder and excitement of scientific discovery Invest in future scientific leaders working to achieve five strategic priorities: and in innovation Influence policymaking with the best scientific advice Invigorate • Invest in future scientific leaders and in innovation science and mathematics education Increase access to the best science internationally SHAPING THE FUTURE • Influence policymaking with the best scientific advice Inspire an interest in the joy, wonder and excitement of scientific discovery Review of the Year 2006/07 • Invigorate science and mathematics education • Increase access to the best science internationally • Inspire an interest in the joy, wonder and excitement of scientific discovery Issued: August 2007 Founded in 1660, the Royal Society is the independent scientific academy of the UK, dedicated to promoting excellence in science Printed on stock containing 55% recycled fibre. -
National and State Banks, Saving's- Banks, and Trust Companies
1900 DIRECTORS National and State Banks, Saving's- Banks, and Trust Companies PRINCIPAL CITIES IN THE UNITED STATES. ABBANGED ALPHABETICALLY BY STATES. CITIES, AND BANKS. First National. First National. Merchants' & Plant Geo. Ptisch. ers* National. L. M. Jacobs. T. H. Molton. J. R. Stevens. S. M. Franklin. ALABAMA. T. T. Uillman. V. K. Hall. S. C.Marks. ARIZONA. W. S. Brown. A. S. Fletcher. M. P. Le Grand. W. A. Walker. R. E. Spragins. C. S. Mathews. Consolidated Nat'l. N. E. Barker. W. H. Echols. R. Goldthwaite. PHCENIX. M. P. Freeman. Robt. Jemison. O. B. Patton. S. B. Marks, Jr. K. W. ulaves. ANNISTON. F. D. Nabers. D. Coleman. W. D. Brown. Home Savings W. C. Davit*. B. F. Moore. n.h. Rnth. Bank & Trust Co. II. B. Tenny. II. M. Ilobbie. Aunlston Banking: E. M. Tutwiler. Chan. F. Ainsworth. Chas. T. Etchells. & Loan Go. ErBkine Ramsay. MOBILE. R. F. Ligon, Jr. F. M. Jackson. S. M.McCowan. J. B. Goodwin. City National. It. II. Greene. II. A. Young. Hugh II. Price. W. L. McCaa. Jefferson County E. J. Buck. Ancil Martin. A. Henderson. Savings. Jno. Carraway. OPELIKA. ARKANSAS. A. W. Bell. L. Lopez. National Bank of J. A. Downey. O. F. Cawthon. Arizona. M.B. Wellborn. Bank of Opelika. J.J.Willett. Geo. W. Harris. C. T. Hearin. C. F. Enslen. F. C. Turner. S. Lewis, FAYETTEVILLE. E- F. Enslen. E. G. Dieaper. R. M. Greene. E. Ganz. Aunlston National. Cnas. F. Enslen. J. T. Dumas. J. C. Farley. S. Ob^rfelder. B.W. Williams. John Y. T.