Report for the Academic Year 2010-2011
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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. -
Parallel Sessions
Identification of Dark Matter July 23-27, 2012 9th International Conference Chicago, IL http://kicp-workshops.uchicago.edu/IDM2012/ PARALLEL SESSIONS http://kicp.uchicago.edu/ http://www.nsf.gov/ http://www.uchicago.edu/ http://www.fnal.gov/ International Advisory Committee Daniel Akerib Elena Aprile Rita Bernabei Case Western Reserve University, Columbia University, USA Universita degli Studi di Roma, Italy Cleveland, USA Gianfranco Bertone Joakim Edsjo Katherine Freese University of Amsterdam Oskar Klein Centre / Stockholm University of Michigan, USA University Richard Gaitskell Gilles Gerbier Anne Green Brown University, USA IRFU/ CEA Saclay, France University of Nottingham, UK Karsten Jedamzik Xiangdong Ji Lawrence Krauss Universite de Montpellier, France University of Maryland, USA Arizona State University, USA Vitaly Kudryavtsev Reina Maruyama Leszek Roszkowski University of Sheffield University of Wisconsin-Madison University of Sheffield, UK Bernard Sadoulet Pierre Salati Daniel Santos University of California, Berkeley, USA University of California, Berkeley, USA LPSC/UJF/CNRS Pierre Sikivie Daniel Snowden-Ifft Neil Spooner University of Florida, USA Occidental College University of Sheffield, UK Max Tegmark Karl van Bibber Kavli Institute for Astrophysics & Space Naval Postgraduate School Monterey, Research at MIT, USA USA Local Organizing Committee Daniel Bauer Matthew Buckley Juan Collar Fermi National Accelerator Laboratory Fermi National Accelerator Laboratory Kavli Institute for Cosmological Physics Scott Dodelson Aimee -
Report for the Academic Year 1995
Institute /or ADVANCED STUDY REPORT FOR THE ACADEMIC YEAR 1994 - 95 PRINCETON NEW JERSEY Institute /or ADVANCED STUDY REPORT FOR THE ACADEMIC YEAR 1 994 - 95 OLDEN LANE PRINCETON • NEW JERSEY 08540-0631 609-734-8000 609-924-8399 (Fax) Extract from the letter addressed by the Founders to the Institute's Trustees, dated June 6, 1930. Newark, New jersey. It is fundamental in our purpose, and our express desire, that in the appointments to the staff and faculty, as well as in the admission of workers and students, no account shall be taken, directly or indirectly, of race, religion, or sex. We feel strongly that the spirit characteristic of America at its noblest, above all the pursuit of higher learning, cannot admit of any conditions as to personnel other than those designed to promote the objects for which this institution is established, and particularly with no regard whatever to accidents of race, creed, or sex. TABLE OF CONTENTS 4 BACKGROUND AND PURPOSE 5 • FOUNDERS, TRUSTEES AND OFFICERS OF THE BOARD AND OF THE CORPORATION 8 • ADMINISTRATION 11 REPORT OF THE CHAIRMAN 15 REPORT OF THE DIRECTOR 23 • ACKNOWLEDGMENTS 27 • REPORT OF THE SCHOOL OF HISTORICAL STUDIES ACADEMIC ACTIVITIES MEMBERS, VISITORS AND RESEARCH STAFF 36 • REPORT OF THE SCHOOL OF MATHEMATICS ACADEMIC ACTIVITIES MEMBERS AND VISITORS 42 • REPORT OF THE SCHOOL OF NATURAL SCIENCES ACADEMIC ACTIVITIES MEMBERS AND VISITORS 50 • REPORT OF THE SCHOOL OF SOCIAL SCIENCE ACADEMIC ACTIVITIES MEMBERS, VISITORS AND RESEARCH STAFF 55 • REPORT OF THE INSTITUTE LIBRARIES 57 • RECORD OF INSTITUTE EVENTS IN THE ACADEMIC YEAR 1994-95 85 • INDEPENDENT AUDITORS' REPORT INSTITUTE FOR ADVANCED STUDY: BACKGROUND AND PURPOSE The Institute for Advanced Study is an independent, nonprofit institution devoted to the encouragement of learning and scholarship. -
New Beginnings
NEW BEGINNINGS A three-year report of Eklavya Foundation 2001-2004 NEW BEGINNINGS A three vi'ar report of the Ikb\\a I ouruiatinn fJQOl Jun/j i We gratffulli a. k now ledpc tor Design. IOVLM illu-itMtion & le<if motif: Urijii Moh.mly. IDC. NT F'OVM^I, Murnbai Sketches Mrm.r.wmi 1 ^td Ravnuird & AntdM HjzanK.i Murnhni ic This honor, uy piojoU Inciu'.ti i.il D ,icjn C^ntif, MF P'j\\-ii. Mun.h.ii Eklavya Foundation H(Hji'.U>u>rJ Vu itMy No S l *n I ) H U--H .-/> 1 lh.' 1 ' 1 -- Mi'qiM(M(KlUtfic" H .' i. .VKM!. W.M U..lhi , O'uj ' ' ".." i " ' AM (l(.jt|.|ir In | U.'.-v.i i" 't!|i l-i, mi*, i.j, ,M.-t ,"H.'I.. :i ] J,)I)M 1- * ' 1 >' ' l I ; v'lil- '-! i i- ' .. ii i'. .i J /()(.)/ [ '! .'11" ',-,* ? ;i' ! \ i i i I)' .'. )! _>f [ ^h Jciiuuirv <?Ol)S '.'Jon uj l ontnhutoiy put i <-, sn Published In Eklavya L / Hir,-1',^ Arer.u olony Phone 0755 246 3380, 246 4824 - Fax: 0755 246 1 703 Email eklavyampfj'mantrdfteenet corn Printed at ' Bhanclan Otis*.". Pnnti-rs Arfj v.n!c>nv Bliou.u P ( iont- /-it; i Contents The dismantling oKwiMon People's voices Report of cK-tiviLies(;OOl Foreword In this report we share with you a truly momentous leg of our long journey Two events impacted significantly on the structure and work of Eklavya. One was the closure of our collaborative middle school educational programmes by the Madhya Pradesh government in July 2002 The second was the bifurcation of Eklavya into two autonomous units - a 'school education and publication' group and a'rural development'group.The latter was registered as a new society on August 1 1, 2003 as the Samavesh Society for Development and Governance. -
Explorations of Non-Supersymmetric Black Holes in Supergravity
Explorations of Non-Supersymmetric Black Holes in Supergravity by Anthony M. Charles A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy (Physics) in the University of Michigan 2018 Doctoral Committee: Professor Finn Larsen, Chair Associate Professor Lydia Bieri Professor Henriette Elvang Professor James Liu Associate Professor Jeff McMahon Anthony M. Charles [email protected] ORCID iD: 0000-0003-1851-458X c Anthony M. Charles 2018 Dedication To my wife, my love, and my everything, Emily. ii Acknowledgments I would like to thank my advisor, Finn Larsen, for his incredibly thoughtful guidance and collaboration throughout the course of my graduate career. I am also grateful to the wonder- ful faculty at the University of Michigan. In particular, I would like to thank Ratindranath Akhoury, Henriette Elvang, and Jim Liu for their unending support and advice over the last five years. I owe a lot to the incredibly talented students and postdocs in the high energy theory group at the University of Michigan. Special thanks goes to Sebastian Ellis, John Golden, Gino Knodel, Pedro Lisbao, Daniel Mayerson, Tim Olson, and Vimal Rathee for being some of the most brilliant and engaging people I've ever known. I would be remiss if I didn't thank all of my wonderful friends for making my time in Michigan an absolute joy. In particular, I would like to thank Alec, Ansel, Emily Y., Glenn, Hannah, Jessie, Joe, John, Meryl, Midhat, Natasha, and Peter. You are the best friends I've ever had, and I wouldn't be where I am today without you. -
16 February 2016 Prof. M. Jagadesh Kumar Vice Chancellor
16 February 2016 Prof. M. Jagadesh Kumar Vice Chancellor Jawaharlal Nehru University New Delhi-110 067, India Dear Prof. Kumar, We are writing, as a group of academics, to express our deep disappointment with your actions in the event leading up to the arrest of several students last week. We understand that last Tuesday, a student group organized a rally to commemorate the death anniversary of Afzal Guru. The police alleges that some of the students voiced controversial opinions. The police then proceeded to arrest the president of the JNU Students Union, Kanhaiya Kumar, and charged him with sedition. This has been followed by a number of further arrests. What is most disturbing is that the JNU administration appears to have defended and aided these repressive actions by the police, rather than defending the students who were involved in a non-violent activity. The arrest of the president of the JNUSU is especially troublesome since he was not even an organizer of the rally but merely present to express his solidarity. However, even as far the organizers and the speakers at the event are concerned, we hope that you recognize that expressing controversial views in a peaceful forum cannot be equated with sedition. For example, many people believe that Afzal Guru was let down by a lack of appropriate legal representation in his trial, and that his execution was therefore a grave miscarriage of justice. One may agree or disagree with this viewpoint — and, indeed, signatories to this letter hold different positions — but we are unanimous that students should have the right to freely discuss this issue. -
Asian Nobel Prize' for Mapping the Universe 27 May 2010
Scientists win 'Asian Nobel Prize' for mapping the universe 27 May 2010 Three US scientists whose work helped map the category. universe are among the recipients of the one- million-US-dollar Shaw Prize, known as the "Asian (c) 2010 AFP Nobel," the competition's organisers said Thursday. Princeton University professors Lyman Page and David Spergel and Charles Bennett of Johns Hopkins University, won the award for an experiment that helped to determine the "geometry, age and composition of the universe to unprecedented precision." The trio will share the Shaw Prize's award for astronomy, with one-million-US-dollar prizes also awarded in the categories for mathematical sciences and life sciences and medicine. The University of California's David Julius won the award for life sciences and medicine for his "seminal discoveries" of how the skin senses pain and temperature, the organisers' statement said. "(Julius's) work has provided insights into fundamental mechanisms underlying the sense of touch as well as knowledge that opens the door to rational drug design for the treatment of chronic pain," the statement said. Princeton's Jean Bourgain won an award for his "profound work" in mathematical sciences, it said. The Shaw Prize, funded by Hong Kong film producer and philanthropist Run Run Shaw and first awarded in 2004, honours exceptional contributions "to the advancement of civilization and the well-being of humankind." The awards will be presented at a ceremony in Hong Kong on September 28. Last year, two scientists whose work challenged the assumption that obesity is caused by a lack of will power won the life sciences and medicine 1 / 2 APA citation: Scientists win 'Asian Nobel Prize' for mapping the universe (2010, May 27) retrieved 27 September 2021 from https://phys.org/news/2010-05-scientists-asian-nobel-prize-universe.html This document is subject to copyright. -
Professor Peter Goldreich Member of the Board of Adjudicators Chairman of the Selection Committee for the Prize in Astronomy
The Shaw Prize The Shaw Prize is an international award to honour individuals who are currently active in their respective fields and who have recently achieved distinguished and significant advances, who have made outstanding contributions in academic and scientific research or applications, or who in other domains have achieved excellence. The award is dedicated to furthering societal progress, enhancing quality of life, and enriching humanity’s spiritual civilization. Preference is to be given to individuals whose significant work was recently achieved and who are currently active in their respective fields. Founder's Biographical Note The Shaw Prize was established under the auspices of Mr Run Run Shaw. Mr Shaw, born in China in 1907, was a native of Ningbo County, Zhejiang Province. He joined his brother’s film company in China in the 1920s. During the 1950s he founded the film company Shaw Brothers (HK) Limited in Hong Kong. He was one of the founding members of Television Broadcasts Limited launched in Hong Kong in 1967. Mr Shaw also founded two charities, The Shaw Foundation Hong Kong and The Sir Run Run Shaw Charitable Trust, both dedicated to the promotion of education, scientific and technological research, medical and welfare services, and culture and the arts. ~ 1 ~ Message from the Chief Executive I warmly congratulate the six Shaw Laureates of 2014. Established in 2002 under the auspices of Mr Run Run Shaw, the Shaw Prize is a highly prestigious recognition of the role that scientists play in shaping the development of a modern world. Since the first award in 2004, 54 leading international scientists have been honoured for their ground-breaking discoveries which have expanded the frontiers of human knowledge and made significant contributions to humankind. -
David Spergel Is the Director of the Center for Computational Astrophysics and the Charles Young Professor of Astronomy at Princeton University
David Spergel is the director of the Center for Computational Astrophysics and the Charles Young Professor of Astronomy at Princeton University. He is the former chair of the Space Studies Board. Using microwave background observations from the Wilkinson Microwave Anisotropy Probe (WMAP) and the Atacama Cosmology Telescope, Spergel has measured the age, shape and composition of the universe. These observations have played a significant role in establishing the standard model of cosmology. He is one of the leaders of the Simons Observatory, which will include a planned millimeter-wave telescope that will allow us to take the next step in studying the microwave sky and probing the history of the universe. Spergel is currently co-chair of the Wide Field Infrared Survey Telescope (WFIRST) science team. WFIRST will study the nature of dark energy, complete the demographic survey of extrasolar planets, characterize the atmospheres of nearby planets and survey the universe with more than 100 times the field of view of the Hubble Space Telescope. Spergel has played a significant role in designing the coronagraph and in shaping the overall mission. Since completing my Ph.D. work, Spergel has been interested in using laboratory experiments and astronomical observations to probe the nature of dark matter and look for new physics. Recently, Spergel has been active in the exploration of data from the Gaia satellite and observations made by Subaru’s Hyper Suprime-Cam. Spergel serves as co-chair of the Global Coordination of Ground and Space Astrophysics working group of the International Astronomical Union. At Princeton, Spergel was department chair for a decade. -
Academic Report 2009–10
Academic Report 2009–10 Harish-Chandra Research Institute Chhatnag Road, Jhunsi, Allahabad 211019 Contents About the Institute 2 Director’s Report 4 Governing Council 8 Academic Staff 10 Administrative Staff 14 Academic Report: Mathematics 16 Academic Report: Physics 47 Workshops and Conferences 150 Recent Graduates 151 Publications 152 Preprints 163 About the Computer Section 173 Library 174 Construction Work 176 1 About the Institute Early Years The Harish-Chandra Research Institute is one of the premier research institute in the country. It is an autonomous institute fully funded by the Department of Atomic Energy, Government of India. Till October 10, 2000 the Institute was known as Mehta Research Institute of Mathematics and Mathematical Physics (MRI) after which it was renamed as Harish-Chandra Research Institute (HRI) after the internationally acclaimed mathematician, late Prof Harish-Chandra. The Institute started with efforts of Dr. B. N. Prasad, a mathematician at the University of Allahabad with initial support from the B. S. Mehta Trust, Kolkata. Dr. Prasad was succeeded in January 1966 by Dr. S. R. Sinha, also of Allahabad University. He was followed by Prof. P. L. Bhatnagar as the first formal Director. After an interim period in January 1983, Prof. S. S. Shrikhande joined as the next Director of the Institute. During his tenure the dialogue with the Department of Atomic Energy (DAE) entered into decisive stage and a review committee was constituted by the DAE to examine the Institutes fu- ture. In 1985 N. D. Tiwari, the then Chief Minister of Uttar Pradesh, agreed to provide sufficient land for the Institute and the DAE promised financial sup- port for meeting both the recurring and non-recurring expenditure. -
Dissertation Siska De Baerdemaeker
Cosmology: The Impossible Integration? by Siska De Baerdemaeker B.A., Philosophy, KU Leuven, 2012 M.A. Philosophy, KU Leuven, 2013 B.Sc. Physics, KU Leuven, 2014 Submitted to the Graduate Faculty of the Dietrich School of Arts and Sciences in partial fulfillment of the requirements for the degree of Doctor of Philosophy University of Pittsburgh 2020 UNIVERSITY OF PITTSBURGH DIETRICH SCHOOL OF ARTS AND SCIENCES This dissertation was presented by Siska De Baerdemaeker It was defended on March 31st 2020 and approved by John Norton, History and Philosophy of Science, University of Pittsburgh Arthur Kosowsky, Physics and Astronomy, University of Pittsburgh Sandra Mitchell, History and Philosophy of Science, University of Pittsburgh James Woodward, History and Philosophy of Science, University of Pittsburgh Dissertation Director: John Norton, History and Philosophy of Science, University of Pittsburgh ii Copyright c by Siska De Baerdemaeker 2020 iii Cosmology: The Impossible Integration? Siska De Baerdemaeker, PhD University of Pittsburgh, 2020 My dissertation introduces a new account of how empirical methods and lines of evidence can come to bear on cosmological model-building. Through a careful study of the recent history of cosmology and dark matter research, I explicate a new type of justification for ex- periments, a `method-driven logic'. This structure of justification underlies terrestrial exper- iments researching dark matter and dark energy, but it is more generally prevalent in cases of an underdescribed target. Using a method-driven logic comes with a cost, however. Specif- ically, interpreting the empirical results of experiments justified through a method-driven logic is non-trivial: negative results warrant secure constraints on the space of possibilities for the target, whereas significant positive results remain ambivalent. -
Glossary of Terms Absorption Line a Dark Line at a Particular Wavelength Superimposed Upon a Bright, Continuous Spectrum
Glossary of terms absorption line A dark line at a particular wavelength superimposed upon a bright, continuous spectrum. Such a spectral line can be formed when electromag- netic radiation, while travelling on its way to an observer, meets a substance; if that substance can absorb energy at that particular wavelength then the observer sees an absorption line. Compare with emission line. accretion disk A disk of gas or dust orbiting a massive object such as a star, a stellar-mass black hole or an active galactic nucleus. An accretion disk plays an important role in the formation of a planetary system around a young star. An accretion disk around a supermassive black hole is thought to be the key mecha- nism powering an active galactic nucleus. active galactic nucleus (agn) A compact region at the center of a galaxy that emits vast amounts of electromagnetic radiation and fast-moving jets of particles; an agn can outshine the rest of the galaxy despite being hardly larger in volume than the Solar System. Various classes of agn exist, including quasars and Seyfert galaxies, but in each case the energy is believed to be generated as matter accretes onto a supermassive black hole. adaptive optics A technique used by large ground-based optical telescopes to remove the blurring affects caused by Earth’s atmosphere. Light from a guide star is used as a calibration source; a complicated system of software and hardware then deforms a small mirror to correct for atmospheric distortions. The mirror shape changes more quickly than the atmosphere itself fluctuates.