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Is the Universe Expanding?: an Historical and Philosophical Perspective for Cosmologists Starting Anew
Western Michigan University ScholarWorks at WMU Master's Theses Graduate College 6-1996 Is the Universe Expanding?: An Historical and Philosophical Perspective for Cosmologists Starting Anew David A. Vlosak Follow this and additional works at: https://scholarworks.wmich.edu/masters_theses Part of the Cosmology, Relativity, and Gravity Commons Recommended Citation Vlosak, David A., "Is the Universe Expanding?: An Historical and Philosophical Perspective for Cosmologists Starting Anew" (1996). Master's Theses. 3474. https://scholarworks.wmich.edu/masters_theses/3474 This Masters Thesis-Open Access is brought to you for free and open access by the Graduate College at ScholarWorks at WMU. It has been accepted for inclusion in Master's Theses by an authorized administrator of ScholarWorks at WMU. For more information, please contact [email protected]. IS THEUN IVERSE EXPANDING?: AN HISTORICAL AND PHILOSOPHICAL PERSPECTIVE FOR COSMOLOGISTS STAR TING ANEW by David A Vlasak A Thesis Submitted to the Faculty of The Graduate College in partial fulfillment of the requirements forthe Degree of Master of Arts Department of Philosophy Western Michigan University Kalamazoo, Michigan June 1996 IS THE UNIVERSE EXPANDING?: AN HISTORICAL AND PHILOSOPHICAL PERSPECTIVE FOR COSMOLOGISTS STARTING ANEW David A Vlasak, M.A. Western Michigan University, 1996 This study addresses the problem of how scientists ought to go about resolving the current crisis in big bang cosmology. Although this problem can be addressed by scientists themselves at the level of their own practice, this study addresses it at the meta level by using the resources offered by philosophy of science. There are two ways to resolve the current crisis. -
Computing ATOMIC NUCLEI
UNIVERSAL NUCLEAR ENERGY DENSITY FUNCTIONAL Computing ATOMIC NUCLEI Petascale computing helps disentangle the nuclear puzzle. The goal of the Universal Nuclear Energy Density Functional (UNEDF) collaboration is to provide a comprehensive description of all nuclei and their reactions based on the most accurate knowledge of the nuclear interaction, the most reliable theoretical approaches, and the massive use of computer power. Science of Nuclei the Hamiltonian matrix. Coupled cluster (CC) Nuclei comprise 99.9% of all baryonic matter in techniques, which were formulated by nuclear sci- the Universe and are the fuel that burns in stars. entists in the 1950s, are essential techniques in The rather complex nature of the nuclear forces chemistry today and have recently been resurgent among protons and neutrons generates a broad in nuclear structure. Quantum Monte Carlo tech- range and diversity in the nuclear phenomena that niques dominate studies of phase transitions in can be observed. As shown during the last decade, spin systems and nuclei. These methods are used developing a comprehensive description of all to understand both the nuclear and electronic nuclei and their reactions requires theoretical and equations of state in condensed systems, and they experimental investigations of rare isotopes with are used to investigate the excitation spectra in unusual neutron-to-proton ratios. These nuclei nuclei, atoms, and molecules. are labeled exotic, or rare, because they are not When applied to systems with many active par- typically found on Earth. They are difficult to pro- ticles, ab initio and configuration interaction duce experimentally because they usually have methods present computational challenges as the extremely short lifetimes. -
Conference on the History of Quantum Physics Max-Planck-Institut Für Wissenschaftsgeschichte Berlin, 2–6 July 2007 Abstract
Conference on the history of quantum physics Max-Planck-Institut für Wissenschaftsgeschichte Berlin, 2–6 July 2007 Abstract Title: Walther Nernst, Albert Einstein, Otto Stern, Adriaan Fokker, and the rotational specific heat of hydrogen Author: Clayton A. Gearhart (St. John’s University, Minnesota, USA) In 1911, the German physical chemist Walther Nernst argued that the new quantum theory promised to clear up long-standing puzzles in kinetic theory, particularly in understanding the discrepancies between the predictions of the equipartition theorem and the measured specific heats of gases. Nernst noted that hydrogen gas would be a good test case. The first measurements were published by his assistant Arnold Euken in 1912, and showed a sharp drop in the specific heat at low temperatures, corresponding to rotational degrees of freedom “freezing out.” In his 1911 paper, Nernst also developed a theory for a quantum rotator (a tiny rotating dumbbell representing a diatomic gas). Remarkably, he did not quantize rotational energies. Instead, the specific heat fell off because the gas reached equilibrium by exchanging harmonic oscillator quanta with quantized Planck resonators. Nernst’s theory was flawed. But Einstein adopted a corrected version at the 1911 Solvay Conference, and in 1913, he and Otto Stern published a detailed treatment. Following Nernst, Einstein and Stern did not quantize the rotators. But they did explore the new zero- point energy that Max Planck had introduced in his “second quantum theory” in 1911. Einstein and Stern calculated the specific heat of hydrogen for two cases, one that assumed a zero-point energy for a rotator and one that did not. -
Nathaniel Rich's Losing Earth and the Role of William Nierenberg And
Nathaniel Rich’s Losing Earth and the Role of William Nierenberg and Other Science Advisors: Why didn’t we act on climate change in the 1980s? Ed Levy The entire New York Times Magazine of August 5, 2018 was devoted to an important article by Nathaniel Rich, Losing Earth: The Decade we almost stopped climate Change. In Rich’s account from 1979 to 1989 the United States came close to “breaking our suicide pact with fossil fuels.”1 Rich shows that at the beginning of that decade a broad international consensus had developed favoring action in the form of a global treaty to curb emissions and that U.S. leadership was required and possibly forthcoming. Yet at the end of the decade it was clear that these efforts had failed. Rich sets as his primary task answering the question, “Why didn’t we act?” He does not provide a satisfactory answer. However, Rich’s informative and nuanced accounts convey well the shifting positions about climate change in the US during the decade. At the beginning it was difficult to get widespread attention, later it looked as though linking global warming to other issues such as ozone depletion and CFCs could result in action. These accounts are based on a large number of interviews and extensive research, but the story is told primarily through the eyes of two significant players, Rafe Pomerance and James Hansen, “a hyperkinetic lobbyist and a guileless atmospheric physicist who, at great personal cost, tried to warn humanity of what was coming.” Still, Rich barely addresses the central question explicitly and does not come close to providing a convincing answer. -
A General Theory of Climate Denial Peter J
A General Theory of Climate Denial Peter J. Jacques A General Theory of Climate Denial • Peter J. Jacques There is now a well-recognized right-wing counter-movement challenging the trend, attribution, impact, and civic implications of orthodox climate change science. Where do the body and spirit of this counter-movement come from? Here I will reºect on some conspicuous questions. First, why have academics, the media, and the counter-movement itself had difªculty naming the counter- movement? Second, why reject the premise of global environmental change at all? Finally, what is the result of the apparent binary choice between the ac- knowledgment of the orthodoxy and its rejection? A General Theory of Denial I will argue that climate denial is an appropriate label consistent with Lang’s “General Theory of Historical Denial.”1 Currently, there is disagreement whether climate “skeptic,” “contrarian,” and “denier” are representative terms.2 I have used the word “skeptic,” but I admit here and elsewhere that it is inappro- priate,3 because the skepticism in environmental skepticism is asymmetrical. As skeptics cast doubt on ecological science, they have an abiding faith in industrial science and technology, free enterprise, and those great institutions of Western Enlightenment.4 Further, skeptics rightfully argue that skepticism is a funda- mental sentiment of rigorous science. Ecological cynicism is then positioned as scientiªc without drawing attention to the asymmetry. Lahsen has successfully used the word “contrarian” to denote the most outspoken leaders of climate rejection, particularly credentialed physicists and climate scientists such as Frederick Seitz, Robert Jastrow, William Nierenberg, Willie Soon, and Sallie Balliunas. -
1 Census of Marine Life Participants 2000-2010
Census of Marine Life Participants 2000-2010 Raza Abidi, Dalhousie University, Canada Jo Acebes, Asia Research Center, Philippines Arturo Acero, Universidad Nacional de Colombia, Colombia Shanta Nair Achuthankutty, National Centre for Antarctic and Ocean Research, India C.T. Achuthankutty, National Institute of Oceanography, India Colleen Adam, DIVERSITAS, France Sarah Adamowicz, University of Guelph, Canada Nathan Adams, United States Helena Adão, University of Évora, Portugal Adrian Aebischer, University of Bern and Museum Fribourg, Switzerland Steven Africk, Acentech Inc, United States Vikram Agadi, National Institute Scientific Communication & Information Resources, India Yogi Agrawal, Sequoia Scientific, United States Maite Aguado, Universidad Autonóma de Madrid, Spain Anelio Aguayo-Lobo, Instituto Antarctico Chileno, Chile Paula Aguiar, University of the Azores, Portugal John Ahearn, Museum Victoria, Australia Sayyed Ahmed, Sultan Qaboos University, Sultanate of Oman Shane Ahyong, National Institute of Water & Atmospheric Research (NIWA), New Zealand Jim Aiken, Plymouth Marine Laboratory, United Kingdom Cameron Ainsworth, University of British Columbia, Canada Laura Airoldi, Università di Bologna, Italy Belinda Aker, National Oceanography Centre, Southampton, United Kingdom Dag Aksnes, University of Bergen, Norway Farid Al-Abdali, Five Oceans LLC, Sultanate of Oman Nasser Al-Azri, HMR Environmental Engineering Cunsultants, Sultanate of Oman Adnan Al-Azri, Sultan Qaboos University, Sultanate of Oman Monica Albuquerque, University Lusófona de Humanidades e Tecnologias, Portugal Jacqueline Alder, UNEP, Kenya Viviana Alder, University of Buenos Aires, Argentina Juan Luis Aleget, Universitat de Girona, Spain Yaroslava Alekseeva, Russian Academy of Sciences, Russia Vera Alexander, University of Alaska Fairbanks, United States Karen Alexander, University of New Hampshire, United States Daniel Alexandrov, European University at St. Petersburg, Russia J.R.B. -
Wolfgang Pauli Niels Bohr Paul Dirac Max Planck Richard Feynman
Wolfgang Pauli Niels Bohr Paul Dirac Max Planck Richard Feynman Louis de Broglie Norman Ramsey Willis Lamb Otto Stern Werner Heisenberg Walther Gerlach Ernest Rutherford Satyendranath Bose Max Born Erwin Schrödinger Eugene Wigner Arnold Sommerfeld Julian Schwinger David Bohm Enrico Fermi Albert Einstein Where discovery meets practice Center for Integrated Quantum Science and Technology IQ ST in Baden-Württemberg . Introduction “But I do not wish to be forced into abandoning strict These two quotes by Albert Einstein not only express his well more securely, develop new types of computer or construct highly causality without having defended it quite differently known aversion to quantum theory, they also come from two quite accurate measuring equipment. than I have so far. The idea that an electron exposed to a different periods of his life. The first is from a letter dated 19 April Thus quantum theory extends beyond the field of physics into other 1924 to Max Born regarding the latter’s statistical interpretation of areas, e.g. mathematics, engineering, chemistry, and even biology. beam freely chooses the moment and direction in which quantum mechanics. The second is from Einstein’s last lecture as Let us look at a few examples which illustrate this. The field of crypt it wants to move is unbearable to me. If that is the case, part of a series of classes by the American physicist John Archibald ography uses number theory, which constitutes a subdiscipline of then I would rather be a cobbler or a casino employee Wheeler in 1954 at Princeton. pure mathematics. Producing a quantum computer with new types than a physicist.” The realization that, in the quantum world, objects only exist when of gates on the basis of the superposition principle from quantum they are measured – and this is what is behind the moon/mouse mechanics requires the involvement of engineering. -
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The Second Lepton Family Klaus Winter, CERN The Nobel Prize for Physics for 1988 was awarded to L. Lederman, M. Schwartz and J. Steinberger for work on neutrinos in the early 1960s. In a letter [1] addressed to the "dear radioactive ladies and gentlemen", writ ten in December 1930, Wolfgang Pauli proposed, as a "desperate remedy" to save the principle of conservation of energy in beta-decay, the idea of the neutrino, a neutral particle of spin 1/2 and with a mass not larger than 0.01 proton mass. "The continuous beta-spectrum [2] would then become understandable by the assumption that in beta-decay a neutrino is emitted together with the electron, in such a way that the sum of the energies of the neutrino and electron is constant." Pauli did not specify at that time Fig. 1 — A recent photograph taken at CERN of Leon Lederman (left), whether the neutrino was to be ejected Jack Steinberger (centre) and Melvin Schwartz. or created. In his famous paper "An attempt of a theory of beta-decay" [3] the muon not decay into e + at the rate ween 1 and 2 GeV should be achievable. E. Fermi used the neutrino concept of predicted if such a non-locality exis Would these synchrotrons though, deli Pauli together with the concept of the ted ? ". On this view the muon would vir ver enough neutrinos? According to nucleon of Heisenberg. He assumed tually dissociate into W + v, the charged their specifications they should accele that in beta-decay a pair comprising an W would radiate a and W + v would rate 1011 protons per second, an unpre electron and a neutrino is created, analo recombine to an electron. -
SHELDON LEE GLASHOW Lyman Laboratory of Physics Harvard University Cambridge, Mass., USA
TOWARDS A UNIFIED THEORY - THREADS IN A TAPESTRY Nobel Lecture, 8 December, 1979 by SHELDON LEE GLASHOW Lyman Laboratory of Physics Harvard University Cambridge, Mass., USA INTRODUCTION In 1956, when I began doing theoretical physics, the study of elementary particles was like a patchwork quilt. Electrodynamics, weak interactions, and strong interactions were clearly separate disciplines, separately taught and separately studied. There was no coherent theory that described them all. Developments such as the observation of parity violation, the successes of quantum electrodynamics, the discovery of hadron resonances and the appearance of strangeness were well-defined parts of the picture, but they could not be easily fitted together. Things have changed. Today we have what has been called a “standard theory” of elementary particle physics in which strong, weak, and electro- magnetic interactions all arise from a local symmetry principle. It is, in a sense, a complete and apparently correct theory, offering a qualitative description of all particle phenomena and precise quantitative predictions in many instances. There is no experimental data that contradicts the theory. In principle, if not yet in practice, all experimental data can be expressed in terms of a small number of “fundamental” masses and cou- pling constants. The theory we now have is an integral work of art: the patchwork quilt has become a tapestry. Tapestries are made by many artisans working together. The contribu- tions of separate workers cannot be discerned in the completed work, and the loose and false threads have been covered over. So it is in our picture of particle physics. Part of the picture is the unification of weak and electromagnetic interactions and the prediction of neutral currents, now being celebrated by the award of the Nobel Prize. -
Physics Nobel Prize 1975
Physics Nobel Prize 1975 Nobel prize winners, left to right, A. Bohr, B. Mottelson and J. Rainwater. 0. Kofoed-Hansen (Photos Keystone Press, Photopress) Before 1949 every physicist knew that mooted, it was a major breakthrough from 1943-45. From December 1943 the atomic nucleus does not rotate. in thinking about the nucleus and he was actually in the USA. Back in The reasoning behind this erroneous opened a whole new field of research Denmark after the war, he obtained belief came from the following argu• in nuclear physics. This work has for his Ph. D. in 1954 for work on rota• ments. A quantum-mechanical rotator years been guided by the inspiration tional states in atomic nuclei. His with the moment of inertia J can take of Bohr and Mottelson. thesis was thus based on the work for up various energy levels with rota• An entire industry of nuclear which he has now been recognized at tional energies equal to h2(l + 1)| research thus began with Rainwater's the very highest level. He is Professor /8TC2J, where h is Planck's constant brief contribution to Physical Review at the Niels Bohr Institute of the ^nd I is the spin. As an example, I may in 1950 entitled 'Nuclear energy level University of Copenhagen and a nave values 0, 2, 4, ... etc. If the argument for a spheroidal nuclear member of the CERN Scientific Policy nucleus is considered as a rigid body, model'. Today a fair-sized library is Committee. then the moment of inertia J is very needed in order to contain all the Ben Mottelson was born in the USA large and the rotational energies papers written on deformed nuclei and in 1926 and has, for many years, become correspondingly very small. -
Date: To: September 22, 1 997 Mr Ian Johnston©
22-SEP-1997 16:36 NOBELSTIFTELSEN 4& 8 6603847 SID 01 NOBELSTIFTELSEN The Nobel Foundation TELEFAX Date: September 22, 1 997 To: Mr Ian Johnston© Company: Executive Office of the Secretary-General Fax no: 0091-2129633511 From: The Nobel Foundation Total number of pages: olO MESSAGE DearMrJohnstone, With reference to your fax and to our telephone conversation, I am enclosing the address list of all Nobel Prize laureates. Yours sincerely, Ingr BergstrSm Mailing address: Bos StU S-102 45 Stockholm. Sweden Strat itddrtSMi Suircfatan 14 Teleptelrtts: (-MB S) 663 » 20 Fsuc (*-«>!) «W Jg 47 22-SEP-1997 16:36 NOBELSTIFTELSEN 46 B S603847 SID 02 22-SEP-1997 16:35 NOBELSTIFTELSEN 46 8 6603847 SID 03 Professor Willis E, Lamb Jr Prof. Aleksandre M. Prokhorov Dr. Leo EsaJki 848 North Norris Avenue Russian Academy of Sciences University of Tsukuba TUCSON, AZ 857 19 Leninskii Prospect 14 Tsukuba USA MSOCOWV71 Ibaraki Ru s s I a 305 Japan 59* c>io Dr. Tsung Dao Lee Professor Hans A. Bethe Professor Antony Hewlsh Department of Physics Cornell University Cavendish Laboratory Columbia University ITHACA, NY 14853 University of Cambridge 538 West I20th Street USA CAMBRIDGE CB3 OHE NEW YORK, NY 10027 England USA S96 014 S ' Dr. Chen Ning Yang Professor Murray Gell-Mann ^ Professor Aage Bohr The Institute for Department of Physics Niels Bohr Institutet Theoretical Physics California Institute of Technology Blegdamsvej 17 State University of New York PASADENA, CA91125 DK-2100 KOPENHAMN 0 STONY BROOK, NY 11794 USA D anni ark USA 595 600 613 Professor Owen Chamberlain Professor Louis Neel ' Professor Ben Mottelson 6068 Margarldo Drive Membre de rinstitute Nordita OAKLAND, CA 946 IS 15 Rue Marcel-Allegot Blegdamsvej 17 USA F-92190 MEUDON-BELLEVUE DK-2100 KOPENHAMN 0 Frankrike D an m ar k 599 615 Professor Donald A. -
Press Release (PDF)
American Association of Physics Teachers FOR IMMEDIATE RELEASE Mary Beth Monroe Recognized for Creative Leadership in Physics Education College Park, Maryland, United States, October 29, 2009 —The American Associa- tion of Physics Teachers (AAPT) announced today that The Melba Newell Phillips Medal has been awarded to Mary Beth Monroe, Professor of Physics at Southwest Texas Junior College, in recognition of her creative leadership and dedicated service that have resulted in exceptional contributions within AAPT. The Medal will be presented to at a Ceremonial Session of the AAPT Winter Meeting at the Washington Marriott Wardman Park in Washington, DC, on Monday, February 15, 2010. Lila Adair, Chairman, AAPT Awards Committee, said, “Mary Beth is an amazing lady. She has dedicated her entire ca- reer to sharing her passion for physics and AAPT with her students, colleagues and fellow AAPT members. She is one of the few experts I turn to for the institutional history of AAPT, and I am so proud to be presenting the Phillips Medal to her.” As a long time AAPT member, Monroe has quietly and tenaciously served the organization at the state and national level for more than three decades. She served as AAPT Secretary and Chair of the Publications Committee from 2001-2007 and is currently serving as a member of the Committee on the Interests of Senior Physicists and as Chair of the Gover- nance Review Committee. She has played a leading role in developing networks among physicists teaching in Two Year Colleges that have led both to their increasing involvement in AAPT and to better teaching for the students who study physics in these schools “The Melba Newell Phillips Medal is AAPT’s highest recognition for member leadership and service.