In Theory for Every Fundamental Particle, the Theory of Supersymmetry Proposes a Supersymmetric Partner, a “Sparticle” in SUSY Jargon

Total Page:16

File Type:pdf, Size:1020Kb

In Theory for Every Fundamental Particle, the Theory of Supersymmetry Proposes a Supersymmetric Partner, a “Sparticle” in SUSY Jargon Volume 21 Friday, June 5, 1998 Number 11 ~ In Theory For every fundamental particle, the theory of supersymmetry proposes a supersymmetric partner, a “sparticle” in SUSY jargon. The electron, e, for example, has a SUSY spartner, the selectron e.˜ Would every Fermilab theorist have a SUSY “stheorist”? Probably not, but theorists worldwide will be watching Tevatron Run II for the first experimental evidence for SUSY. The Fermilab Stheory Group INSIDE f 2 Supersymmetry 7 Supersymmetry Workshop 8 MiniBooNE 10 Fishing 12 Paperless Papers 14 CDF Party The Fermilab Theory Group supersymmetry …and the physics of Run II by Meher Antia Without resorting to tricky mathematics or exotic physics, anyone can see that much of the stuff the world is made of has mass. Things can STANDARD be touched and felt; they have some bulk, unlike, say, light which is intangible and MODEL immaterial. But why? Why are some things in the universe, like quarks and leptons, chunky and massive and others, like photons and Mass = ~ 3 MeV ~ 1.2 GeV 175 (6) GeV gluons, ethereal and massless? up charm top photon ~ 4 MeV 95 (15) MeV ~ 4.8 GeV Answers to questions like these are usually bottom gluon provided by the Standard Model, to date the down strange 91.186 (2) GeV best framework to < 15 eV < 100 KeV < 35 MeV describe the patchwork of elementary particles electron neutrino muon neutrino tau neutrino Z boson and forces of nature. .511 MeV 106.76 MeV 1.784 GeV 80.36 (13) GeV However, in its simplest form, the Standard Model disappoints. It electron muon tau W boson clearly states that all particles should be I II III massless, just like the Three Generations of Matter photon. How, you might ask, can the Standard Model retain its reputation as the best In its simplest form, the description of nature if Standard Model fails to it makes a prediction account for different that so blatantly flies in particle masses. To solve the face of even the least this problem, theorists perceptive observer? have invoked The Standard supersymmetry, a Model retains its theory that provides a position because there supersymmetric particle is a fix to the mass partner, or “spartner” problem. A particle for each of the known fundamental particles. called the Higgs boson, yet to be observed, is conjured as part of a mechanism to bestow mass upon particles in a way that is consistent with experimental results. Still, the fix of the 2 FermiNews June 5, 1998 Supersymmetry could manifest itself in many different ways. Theorists, including Fermilab’s Joe Lykken, left, are still on the fence about exactly what form it might take. “That’s why we need our experimental colleagues,” says Lykken, shown here with theorist Xerxes Tata, of the University of Hawaii, attending CDF’s 20th birthday party on May 20. Photo by Jenny Mullins Higgs comes burdened with difficulties of its symmetry; these symmetries are restrictions on own. Happily, though, even those difficulties how they behave and interact with each other. may be resolved by a theory known as Unfortunately, the Higgs boson has no such supersymmetry. symmetry to slim it down, and it gets heavier The problem of introducing the Higgs into and heavier as the Standard Model is called the Standard Model is symptomatic of a more upon to explain physics at smaller and smaller general deficiency in an otherwise stunningly length scales. successful model. The Standard Model was The easiest way for theorists to stop the designed to describe particle interactions at out-of-control growth of the Higgs was to length scales of particles like the electron or the introduce a symmetry, and supersymmetry was quarks. These, less than billionths of millimeters the one they chose to cure the Higgs’s weight in size, are undoubtedly tiny, but are still far problem. Developed about 20 years ago, from zero. The problem with the Standard supersymmetry proposed giving the Higgs a Model occurs when physicists try to understand partner—a supersymmetric partner called the particle interactions at length scales close to Higgsino—identical to it in every way except zero. At that point, infinite quantities pop up in for its spin. The Higgsino could then act as a the energies and masses of particles. Infinities sort of personal trainer to the Higgs, not are meaningless not only to physics, but also to allowing it to do things that made it too common sense; it is impossible to have a massive, and keeping it nice and lean to be particle with an infinite mass, for example. of service to the Standard Model. Sometimes, the Standard Model can take But supersymmetry and the Higgsino came care of these infinities by a process called along with much excess baggage. Not only was renormalization: getting the infinite quantity to there a supersymmetric partner for the Higgs, cancel out with some other infinite quantity there had to be supersymmetric partners for all with an opposite sign. Most of the Standard other particles. All these new supersymmetric Model particles are prevented from being partners would have exactly the same properties infinitely massive by having some sort of as their twins, again with the exception of spin. FermiNews June 5, 1998 3 Theorists have invented particle partners before. In the 1930s, to reconcile quantum mechanics with relativity, Paul Dirac proposed siblings for all known particles, identical to the existing particles in every way but with opposite charges. The mysterious siblings— antimatter—are now as commonplace as they were once exotic. …Any particles with the same mass and charge of everyday electrons and Fermilab Archives quarks would Spartners for all The spartners, however, have been much already have Physicists have had their share of fun in more elusive. It was clear from the very naming the supersymmetric particles. Some get beginning that any particles with the same mass been found. an “s” put in front of their ordinary names, the and charge of everyday electrons and quarks sypersymmetric partner (or spartner) of the would already have been found. As no such As no such electron is the selectron, that of the quark is particles have turned up, supersymmetry is the squark. Other particles, like the Higgs, said to be a broken symmetry. Something has particles have get suffixed by an “ino”: the spartner of the caused the masses of the spartners to be very photon is the photino, that of the gluon is the different from the regular particles. In fact, turned up, gluino, and so on. In essence, supersymmetry such a symmetry breaking happens quite claims, we have only seen half the particles that naturally in the theory at extremely high supersymmetry exist. The rest are lurking in the wings, waiting energies, energies beyond the realm of even the to be discovered. most powerful particle accelerator imaginable. is said to be a Stupendous as this may sound, there has But even though the pairs of particles are split been a precedent, points out Fermilab physicist apart and given different masses at high broken symmetry. Joe Lykken. In the 1930s, when trying to energies, they must have a way of reconcile quantum mechanics with relativity, communicating that information down to the Paul Dirac found that, for his theory to make more earthly scales that are accessible to us. sense, all known particles had to have siblings. How exactly this communication might take These siblings were identical to the existing place is not well understood. One possibility is particles in every way, except that they had gravity. Another is that the interaction might opposite charges. The mysterious siblings— occur through some new particle, one similar antimatter—were soon found. They are now to the photon or the gauge bosons that fly back as commonplace as they were once exotic and and forth to carry the weak force. have been snugly accommodated into particle physics. 4 FermiNews June 5, 1998 They can’t hide forever However supersymmetry breaking transmits itself to our world, the result is that if the spartners were to be hunted down in particle accelerators they would be quite heavy. Supersymmetry does not predict exact masses for the various squarks and sleptons. Thus, there is no need to panic and abandon the theory because none of the spartners have yet been found. If they do exist, though, they cannot keep hiding forever. Although there is theoretically no limit on how heavy the spartners can get, after a certain point they no longer perform the function for which they were originally invoked. After all, the supersymmetric particles were supposed to prevent the Higgs from getting too hefty, but if they themselves are not trim enough, their existence serves no purpose. There is a sort of natural mass range within which they are expected to be found. Tantalizingly, the current generation of particle accelerators is just at the edge of that expected range. At Fermilab, the hunt for sparticles is already on. There are dozens of different ways in which these sparticles can make their presence known to experimenters, depending on exactly how supersymmetry theory is formulated. All sparticles, except perhaps the lightest one, are unstable; they decay either into other sparticles or into the regular quarks and leptons that we already know. If they decay into particles of the ordinary kind, it could be extremely difficult to Photo by Jenny Mullins confirm that they were indeed produced from supersymmetry and not from some known the missing energy; only then can it be Harvard graduate Standard Model process. Some signatures — attributed to the LSP. Like all particle searches, student and CDF the presence of lots of electrons and muons this one requires combing through staggering collaborator Maria in the detector, for example — would be clear amounts of data.
Recommended publications
  • Galaxy Cross-Corr
    Astro2020 Science White Paper Synergies Between Galaxy Surveys and Reionization Measurements Thematic Areas: ☐ Planetary Systems ☐ Star and Planet Formation ☐Formation and Evolution of Compact Objects ☒ Cosmology and Fundamental Physics ☐Stars and Stellar Evolution ☐Resolved Stellar Populations and their Environments ☒Galaxy Evolution ☐Multi-Messenger Astronomy and Astrophysics Principal Author: Name: Steven Furlanetto Institution: University of California, Los Angeles Email: [email protected] Phone: (310) 206-4127 Co-authors: Adam Beardsley (Arizona State University), Chris L. Carilli (Cavendish Laboratory, NRAO), Jordan Mirocha (McGill University), James Aguirre (University of Pennsylvania), Yacine Ali- Haimoud (New York University), Marcelo Alvarez (University of California Berkeley), George Becker (University of California Riverside), Judd D. Bowman (Arizona State University), Patrick Breysse (CITA), Volker Bromm (University of Texas at Austin), Philip Bull (Queen Mary University of London), Jack Burns (University of Colorado Boulder), Isabella P. Carucci (University College London), Tzu-Ching Chang (JPL), Hsin Chiang (McGill University), Joanne Cohn (University of California Berkeley), Frederick Davies (University of California Santa Barbara), David DeBoer (University of California Berkeley), Mark Dickinson (NOAO), Joshua Dillon (University of California Berkeley), Olivier Doré (JPL, California Institute of Technology), Cora Dvorkin (Harvard University), Anastasia Fialkov (University of Sussex), Steven Finkelstein (University
    [Show full text]
  • Maria Spiropulu; Other Dimensions? She's in Pursuit - New York Times 10/07/2007 01:26 AM
    SCIENTIST AT WORK -- Maria Spiropulu; Other Dimensions? She's in Pursuit - New York Times 10/07/2007 01:26 AM September 30, 2003 SCIENTIST AT WORK -- Maria Spiropulu; Other Dimensions? She's in Pursuit By DENNIS OVERBYE Flap harder, urged the little girl with the stopwatch. One by one, the children stepped up and launched themselves off the garden wall, flapping homemade wings with their arms. Always with the same result. Crash. Only the girl herself, 7 years old, an aspiring dancer, astronaut, wing maker and free spirit, could not jump -- not out of fear or lack of confidence in the wings she had made, but because she could not time her own flight. ''And I didn't trust anybody to time it for me,'' she recalled. She already had the soul of a scientist, as well as a knack for leadership. Crash. Just before midnight on a recent summer night, the girl, Dr. Maria Spiropulu, now 33 and a physicist affiliated with the University of California at Santa Barbara, stepped outside a South Side Chicago jazz club and climbed into a cluttered Honda Civic. She was wearing black jeans, a black sleeveless top, Nikes and three rings on her left hand. Spewing noise from a leaky muffler, she drove into the Illinois prairie, through the gates of the Fermi National Accelerator Laboratory, or Fermilab, and past scattered farmhouses too white and neat to be real farmhouses anymore. Mars' bloody stare was high in a hazy sky by the time she parked outside a hulking shedlike building. Inside the shed, the ground floor rimmed a huge pit three stories deep and wide as a basketball court, littered with the toys of industrial strength science -- cranes, racks of electronics, tool chests, cables, long magnets stacked like redwood logs.
    [Show full text]
  • High Energy Physics Quantum Information Science Awards Abstracts
    High Energy Physics Quantum Information Science Awards Abstracts Towards Directional Detection of WIMP Dark Matter using Spectroscopy of Quantum Defects in Diamond Ronald Walsworth, David Phillips, and Alexander Sushkov Challenges and Opportunities in Noise‐Aware Implementations of Quantum Field Theories on Near‐Term Quantum Computing Hardware Raphael Pooser, Patrick Dreher, and Lex Kemper Quantum Sensors for Wide Band Axion Dark Matter Detection Peter S Barry, Andrew Sonnenschein, Clarence Chang, Jiansong Gao, Steve Kuhlmann, Noah Kurinsky, and Joel Ullom The Dark Matter Radio‐: A Quantum‐Enhanced Dark Matter Search Kent Irwin and Peter Graham Quantum Sensors for Light-field Dark Matter Searches Kent Irwin, Peter Graham, Alexander Sushkov, Dmitry Budke, and Derek Kimball The Geometry and Flow of Quantum Information: From Quantum Gravity to Quantum Technology Raphael Bousso1, Ehud Altman1, Ning Bao1, Patrick Hayden, Christopher Monroe, Yasunori Nomura1, Xiao‐Liang Qi, Monika Schleier‐Smith, Brian Swingle3, Norman Yao1, and Michael Zaletel Algebraic Approach Towards Quantum Information in Quantum Field Theory and Holography Daniel Harlow, Aram Harrow and Hong Liu Interplay of Quantum Information, Thermodynamics, and Gravity in the Early Universe Nishant Agarwal, Adolfo del Campo, Archana Kamal, and Sarah Shandera Quantum Computing for Neutrino‐nucleus Dynamics Joseph Carlson, Rajan Gupta, Andy C.N. Li, Gabriel Perdue, and Alessandro Roggero Quantum‐Enhanced Metrology with Trapped Ions for Fundamental Physics Salman Habib, Kaifeng Cui1,
    [Show full text]
  • Astro2020 Science White Paper Cosmology with the Highly Redshifted 21 Cm Line
    Astro2020 Science White Paper Cosmology with the Highly Redshifted 21 cm Line Thematic Areas: Planetary Systems Star and Planet Formation Formation and Evolution of Compact Objects 3Cosmology and Fundamental Physics Stars and Stellar Evolution Resolved Stellar Populations and their Environments Galaxy Evolution Multi-Messenger Astronomy and Astrophysics Principal Author: Name: Adrian Liu Institution: McGill University Email: [email protected] Phone: (514) 716-0194 Co-authors: (names and institutions) James Aguirre (University of Pennsylvania), Joshua S. Dillon (UC Berkeley), Steven R. Furlanetto (UCLA), Chris Carilli (National Radio Astronomy Observatory), Yacine Ali-Haimoud (New York University), Marcelo Alvarez (University of California, Berkeley), Adam Beardsley (Arizona State University), George Becker (University of California, Riverside), Judd Bowman (Arizona State University), Patrick Breysse (Canadian Institute for Theoretical Astrophysics), Volker Bromm (University of Texas at Austin), Philip Bull (Queen Mary University of London), Jack Burns (University of Colorado Boulder), Isabella P. Carucci (University College London), Tzu-Ching Chang (Jet Propulsion Laboratory), Hsin Chiang (McGill University), Joanne Cohn (University of California, Berkeley), David DeBoer (University of California, Berkeley), Cora Dvorkin (Harvard University), Anastasia Fialkov (Sussex University), Nick Gnedin (Fermilab), Bryna Hazelton (University of Washington), Daniel Jacobs (Arizona State University), Marc Klein Wolt (Radboud University
    [Show full text]
  • A NSF Physics Frontier Center Annual Report 2005-2006
    A NSF Physics Frontier Center Annual Report 2005-2006 June 29, 2006 i Table of Contents 1 Executive Summary 1 2 Research Accomplishments and Plans 4 2.a Major Research Accomplishments . 4 2.a.1 Research Highlights . 4 2.a.2 Detailed Research Activities: MRC I- Theory . 5 2.a.3 Detailed Research Activities: MRC II- Structures in the Uni- verse ..................................... 20 2.a.4 Detailed Research Activities: MRC III - Cosmic Radiation Backgrounds ................................ 24 2.a.5 Detailed Research Activities: MRC IV - Particles from Space . 28 2.a.6 References . 32 2.b Research Organizational Details . 33 2.c Plans for the Coming Year . 33 3 Publications, Awards and Technology Transfers 40 3.a List of Publications in Peer Reviewed Journals . 40 3.b List of Publications in Peer Reviewed Conference Proceedings . 48 3.c Invited Talks by Institute Members . 52 3.d Honors and Awards . 56 3.e Technology Transfer . 57 4 Education and Human Resources 58 4.a Graduate and Postdoctoral Training . 58 4.a.1 Research Training . 58 4.a.2 Curriculum Development: . 62 4.b Undergraduate Education . 63 4.b.1 Undergraduate Research Experiences: . 63 4.b.2 Undergraduate Curriculum Development: . 64 4.c Educational Outreach . 65 4.c.1 K-12 Programs: Space Explorers . 66 4.c.2 Web-Based Educational Activities: . 69 4.c.3 Other: . 69 4.d Enhancing Diversity . 72 5 Community Outreach and Knowledge Transfer 74 5.a Visitor Participation in Center . 74 5.a.1 Long term visitors . 74 5.a.2 Short term and seminar visitors . 75 5.b Workshops and Symposia .
    [Show full text]
  • Upcoming Events: Science@Cal Monthly Lectures 3Rd Saturday of Each Month 11:00 A.M
    University of California, Berkeley Department of Astronomy B E R K E L E Y A S T R O N O M Y Hearst Field Annex MC 3411 Berkeley, CA 94720-3411 Upcoming Events: Science@Cal Monthly Lectures 3rd Saturday of each month 11:00 a.m. UC Berkeley Campus location changes each month Consult website for details http://scienceatcal. berkeley.edu/lectures UniversityUNIVERSITY of California OF CALIFORNIA | 2014 2014 Evening with the Stars TBA Fall 2014 From the Chair’s Desk… co-PI on the founding grant for the Berkeley the Friends of Astrophysics Postdoctoral Please see the Astronomy website for more Institute for Data Science (BIDS) to bring Fellowship and many other coveted prize information together scientists with diverse backgrounds, fellowships. http://astro.berkeley.edu The Astronomy Department is a yet all dealing with “Big Data” (see page In addition to the rigorous research they vibrant, evolving 2). He is also on the management council pursue, our students and postdocs also find 2015 Raymond and Beverly Sackler community. It’s hard that oversees the Large Synoptic Survey time to get involved in other interesting Distinguished Lecture in Astronomy to fully capture all Telescope. This past summer Bloom again career-building and public outreach activities. Carolyn Porco, Space Science Institute that is happening organized the annual Python Language Matt George, Adam Morgan, and Chris Klein Public lecture: Wednesday, Jan 28 here in a few brief Bootcamp, an immensely popular three-day joined the Insight Data Science Fellows Joint Astronomy/Earth Planetary Sciences paragraphs, but I’ll summer workshop with >200 attendees.
    [Show full text]
  • Fall 2015 Newsletter the American Physical Society
    APS Forum on International Physics Fall 2015 Newsletter page 1 The American Physical Society website: http://www.aps.org/units/fip Fall 2015 Newsletter Ernie Malamud, Editor Message from the Chair, Edmond Berger 2 Report from the APS International Affairs Office (INTAF), Amy Flatten 4 From the Editor, Ernie Malamud 7 APS SPRING MEETINGS Invited talks in FIP sponsored or co-sponsored sessions: 8 March 2 – 6, 2015, San Antonio April 11 – 14, 2015, Baltimore Photos FIP co-sponsored reception at the San Antonio meeting, from Ercan Esen Alp 9 FIP Executive Committee meeting at the Baltimore meeting, from Ercan Esen Alp 10 SAVE THE DATES ! March 14 – 18, 2016 April 16 - 19, 2016 Baltimore Salt Lake City ARTICLES SESAME Moves towards Commissioning, Chris Llewellyn-Smith 11 The São Paulo School of Advanced Sciences (ESPCA) on Recent Developments in Synchrotron Radiation, Harry Westfahl, Helio Tolentino and Esen Ercan Alp 14 Industrial Use of Japanese Synchrotron Radiation (SR) and the X-ray Free Electgron Laser (XFEL) Facilites, Tetsuya Ishikawa 15 Momentum gathers towards a Mexican Light Source, Armando Antillón, José Jimenéz and Matías Moreno 17 The Gulf Nuclear Energy Infrastructure Institute (GNEII), Amir Mohagheghi, Adam Williams, Phil Beeley, and Alex Solodov 20 The Radiation Measurements Cross Calibration (RMCC) Project, Amir Mohagheghi Al-Sharif Nasser Bin Nasser, and Matthew Sternat 22 Improvement in Education and Research through Recognition, a report from Bangladesh, Sultana Nahar 25 APS International Research Travel Award Program, IRTAP: Providing Support to International Collaborators, Michele Irwin 28 International Linear Collider Collaboration Status, Maria Spiropulu 30 NEW Distinguished Student Seminar Program 31 FIP Committees-2015 32 Disclaimer—The articles and opinion pieces found in this issue of the APS Forum on International Physics Newsletter are not peer refereed and represent solely the views of the authors and not necessarily the views of the APS.
    [Show full text]
  • Aspen Physics Turns 50 Michael S
    COMMENT AWARDS Passion and punch-ups ECOLOGY A paean to decay EXHIBITION London show OBITUARY Akira Tonomura, in a chronicle of two contested charts the life that death celebrates Alan Turing’s imaging pioneer, Nobel prizes p.318 provides p.320 life and legacy p.321 remembered p.324 S. MAXWELL/ASPEN CENTER FOR PHYSICS S. MAXWELL/ASPEN CENTER FOR Summer workshops at the Aspen Center for Physics give researchers respite from their academic duties. Aspen physics turns 50 Michael S. Turner reflects on how mountain serenity has bred big breakthroughs at the Aspen Center for Physics in Colorado. heoretical physicists are an odd lot: 10,000 theoretical physicists, including 53 Victorian buildings and wonderful skiing. She bad communicators (Niels Bohr Nobel laureates, from 65 countries. The centre persuaded her husband, a devotee of German and Werner Heisenberg); brilliant can lay claim to the string-theory revolution, writer Johann Wolfgang von Goethe, to visit Tshowmen (Richard Feynman and George the birth of the arXiv preprint archive and in 1945. Seeing it as the ideal place to bring Gamow); the ‘strangest man’ (Paul Dirac); to setting the agenda for condensed-matter together the three aspects of life — economic, lots of Hungarians (Leó Szilárd, Edward physics. Its history is tied to the revival of a sil- cultural and physical — he invested millions Teller and Eugene Wigner); bad hair (Albert ver-mining town and the American entrepre- of dollars in rebuilding it. In 1946, he formed Einstein); and too few women. They don’t neurial spirit, and features a fascinating cast of the Aspen Skiing Corporation, which remains need fancy equipment — a pencil and paper characters, from philosopher Mortimer Adler the financial engine of the valley.
    [Show full text]
  • Dark Matter Halo Mergers and Quasars
    University of Pennsylvania ScholarlyCommons Publicly Accessible Penn Dissertations Spring 2010 Dark Matter Halo Mergers and Quasars Jorge Moreno University of Pennsylvania, [email protected] Follow this and additional works at: https://repository.upenn.edu/edissertations Part of the Cosmology, Relativity, and Gravity Commons, and the External Galaxies Commons Recommended Citation Moreno, Jorge, "Dark Matter Halo Mergers and Quasars" (2010). Publicly Accessible Penn Dissertations. 177. https://repository.upenn.edu/edissertations/177 This paper is posted at ScholarlyCommons. https://repository.upenn.edu/edissertations/177 For more information, please contact [email protected]. Dark Matter Halo Mergers and Quasars Abstract The formation and evolution of galaxies and the supermassive black holes they harbor at their nuclei depends strongly on the merger history of their surrounding dark matter haloes. First we developed a semi-analytic algorithm that describes the merger history tree of a halo. The following tests were performed: the conditional mass function, the time and mass distributions at formation, and the time distribution of the last major merger. We provide a model for the creation rate of dark matter haloes, informed by both coagulation theory and the modified excursion set approach with moving barriers. A comparison with N-body simulations shows that our square-root barrier merger rate is significantly better than the standard extended Press-Schechter rate used in the literature. The last chapter is dedicated to a simple model of quasar activation by major mergers of dark matter haloes. The model consists of two main ingredients: the halo merger rate describing triggering, and a quasar light curve, which tracks the evolution of individual quasars.
    [Show full text]
  • David I. Kaiser
    David I. Kaiser Program in Science, Technology, and Society, and Department of Physics Massachusetts Institute of Technology Tel. 617 452-3173. Email. [email protected] http://web.mit.edu/dikaiser/www Academic Positions 2019 –. Associate Dean, Social and Ethical Responsibilities of Computing, Schwarzman College of Computing, MIT 2015 –. Professor, Department of Physics, MIT. 2011 –. Germeshausen Professor of the History of Science, Program in Science, Technology, and Society, MIT. 2011 –. Affiliated Faculty, Department of the History of Science, Harvard University. 2000 – 2011. Assistant Professor (2000-2004) and Associate Professor (2004-2011), Program in Science, Technology, and Society, MIT. 2000 – 2015. Lecturer (2000-2010) and Senior Lecturer (2010-2015), Department of Physics, MIT. Spring 1999. Visiting Lecturer. Department of Physics and Astronomy, Dartmouth College. Education 2000. Ph.D. in Physics and in History of Science, Harvard University History of Science Dissertation: “Making Theory: Producing Physics and Physicists in Postwar America.” May 2000. Physics Dissertation: “Post-Inflation Reheating in an Expanding Universe.” December 1997. 1993. A.B. in Physics, Dartmouth College. Summa cum Laude Academic Honors and Awards 2020. Physics World “Best of Physics in Books, TV, and Film in 2020” for Quantum Legacies: Dispatches from an Uncertain World. 2016. George Sarton Memorial Lecturer, plenary address sponsored by the History of Science Society, delivered at the American Association for the Advancement of Science annual meeting. 2013. History of Science Society, Davis Prize for best book aimed at a general audience, awarded for How the Hippies Saved Physics: Science, Counterculture, and the Quantum Revival. 2012. Physics World “Book of the Year” award for How the Hippies Saved Physics: Science, Counterculture, and the Quantum Revival.
    [Show full text]
  • University of Groningen Fundamental Cosmology in the Dark Ages With
    University of Groningen Fundamental Cosmology in the Dark Ages with 21-cm Line Fluctuations Furlanetto, Steven; Bowman, Judd D.; Mirocha, Jordan; Pober, Jonathan; Burns, Jack; Carilli, Chris L.; Munoz, Julian; Aguirre, James; Ali-Haimoud, Yacine; Alvarez, Marcelo Published in: Bulletin of the American Astronomical Society IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Final author's version (accepted by publisher, after peer review) Publication date: 2019 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Furlanetto, S., Bowman, J. D., Mirocha, J., Pober, J., Burns, J., Carilli, C. L., Munoz, J., Aguirre, J., Ali- Haimoud, Y., Alvarez, M., Beardsley, A., Becker, G., Breysse, P., Bromm, V., Bull, P., Chang, T-C., Chen, X., Chiang, H., Cohn, J., ... Zaldarriaga, M. (2019). Fundamental Cosmology in the Dark Ages with 21-cm Line Fluctuations. Bulletin of the American Astronomical Society, 51(3), [ID 144 (2019)]. https://ui.adsabs.harvard.edu/abs/2019BAAS...51c.144F Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal.
    [Show full text]
  • @Xxx.Lanl.Gov
    @xxx.lanl.gov first steps toward electronic research communication Paul H. Ginsparg [email protected] is the e-mail short period the primary means of com- The archiving software has been ex- address for the first of a series of municating ongoing research informa- panded to serve a number of other re- hautomated archives for electronic tion in formal areas of high energy par- search disciplines (see Figure 1). The communication of research information. ticle theory. Its rapid acceptance within extended, automatically maintained This “e-print archive” went on-line in this community depended critically on database and distribution system cur- August, 1991. It began as an experi- both recent technological advances and rently serves over 20,000 users from mental means of circumventing recog- particular behavioral aspects of the more than 60 countries and processes nized inadequacies of research journals, community. There are now more than over 30,000 messages per day. It is al- but unexpectedly became within a very 3600 regular users of hep-th worldwide. ready one of the largest and most active 156 Los Alamos Science Number 22 1994 @xxx.lanl.gov databases on the internet. This system may be a paradigm for worldwide, dis- cipline-wide scientific-information ex- change when the next generation of “electronic-data highways” begins to provide more universal access to high- speed computer networks. Background The rapid acceptance of electronic communication of research information in my own community of high-energy theoretical physics was facilitated by a pre-existing “preprint culture,” in which the irrelevance of refereed journals to ongoing research has long been recog- nized.
    [Show full text]