Yonatan F. Kahn, Ph.D
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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 -
Arxiv:1912.08821V2 [Hep-Ph] 27 Jul 2020
MIT-CTP/5157 FERMILAB-PUB-19-628-A A Systematic Study of Hidden Sector Dark Matter: Application to the Gamma-Ray and Antiproton Excesses Dan Hooper,1, 2, 3, ∗ Rebecca K. Leane,4, y Yu-Dai Tsai,1, z Shalma Wegsman,5, x and Samuel J. Witte6, { 1Fermilab, Fermi National Accelerator Laboratory, Batavia, IL 60510, USA 2University of Chicago, Kavli Institute for Cosmological Physics, Chicago, IL 60637, USA 3University of Chicago, Department of Astronomy and Astrophysics, Chicago, IL 60637, USA 4Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 5University of Chicago, Department of Physics, Chicago, IL 60637, USA 6Instituto de Fisica Corpuscular (IFIC), CSIC-Universitat de Valencia, Spain (Dated: July 29, 2020) Abstract In hidden sector models, dark matter does not directly couple to the particle content of the Standard Model, strongly suppressing rates at direct detection experiments, while still allowing for large signals from annihilation. In this paper, we conduct an extensive study of hidden sector dark matter, covering a wide range of dark matter spins, mediator spins, interaction diagrams, and annihilation final states, in each case determining whether the annihilations are s-wave (thus enabling efficient annihilation in the universe today). We then go on to consider a variety of portal interactions that allow the hidden sector annihilation products to decay into the Standard Model. We broadly classify constraints from relic density requirements and dwarf spheroidal galaxy observations. In the scenario that the hidden sector was in equilibrium with the Standard Model in the early universe, we place a lower bound on the portal coupling, as well as on the dark matter’s elastic scattering cross section with nuclei. -
Exact Null Tachyons from Renormalization Group Flows
Exact null tachyons from renormalization group flows The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Adams, Allan , Albion Lawrence, and Ian Swanson. “Exact null tachyons from renormalization group flows.” Physical Review D 80.10 (2009): 106005. © 2009 The American Physical Society As Published http://dx.doi.org/10.1103/PhysRevD.80.106005 Publisher American Physical Society Version Final published version Citable link http://hdl.handle.net/1721.1/52507 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. PHYSICAL REVIEW D 80, 106005 (2009) Exact null tachyons from renormalization group flows Allan Adams,1 Albion Lawrence,2 and Ian Swanson1 1Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA 2Theory Group, Martin Fisher School of Physics, Brandeis University, MS057, 415 South Street, Waltham, Massachusetts 02454, USA (Received 11 August 2009; published 20 November 2009) We construct exact two-dimensional conformal field theories, corresponding to closed string tachyon and metric profiles invariant under shifts in a null coordinate, which can be constructed from any two- dimensional renormalization group flow. These solutions satisfy first order equations of motion in the conjugate null coordinate. The direction along which the tachyon varies is identified precisely with the world sheet scale, and the tachyon equations of motion are the renormalization group flow equations. DOI: 10.1103/PhysRevD.80.106005 PACS numbers: 11.25.Àw, 11.10.Hi I. -
Dynamical Spacetimes from Numerical Hydrodynamics
MIT-CTP-4607 Dynamical Spacetimes from Numerical Hydrodynamics Allan Adams,1 Nathan Benjamin,1, 2 Arvin Moghaddam,1, 3 and Wojciech Musial1, 3 1Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, MA 02139 2Stanford Institute for Theoretical Physics, Stanford University, Stanford, CA 94305 3Center for Theoretical Physics, University of California, Berkeley, Berkeley, CA 94720 We numerically construct dynamical asymptotically-AdS4 metrics by evaluating the fluid/gravity metric on numerical solutions of dissipative hydrodynamics in (2+1) dimensions. The resulting numerical metrics satisfy Einstein's equations in (3+1) dimensions to high accuracy. Holography provides a precise relationship between Review of Fluid/Gravity black holes in AdSd+1 and QFTs in d-dimensions at fi- nite density and temperature. When the QFT state lies We begin by recalling the essential features of the in a hydrodynamic regime (i.e. when d-dimensional gra- fluid/gravity correspondence for a (2+1) fluid as given dients are sufficiently small that the stress-tensor may in [1{4]. At equilibrium, a fluid moving with constant 3- µ be expanded as a power-series in derivatives), the dual velocity u at temperature T is dual to an asymptotically spacetime metric may also be so expanded, leading to an AdS4 black brane described by the metric [10] analytic “fluid/gravity" map between solutions of hydro- ds2 = −2u dxµdr−r2f(br) u u dxµdxν +r2P dxµdxν ; dynamics in d dimensions and dynamical asymptotically- µ µ ν µν AdSd+1 solutions of the Einstein equations. 3 where b = 4πT is the rescaled inverse temperature, This suggests a simple strategy for constructing nu- P µν =ηµν +uµuν projects onto directions transverse to merical solutions of the Einstein equations in asymptot- µ 1 u , and f(ρ) = 1 − ρ3 is the emblackening factor. -
High Energy Physics Quantum Computing
High Energy Physics Quantum Computing Quantum Information Science in High Energy Physics at the Large Hadron Collider PI: O.K. Baker, Yale University Unraveling the quantum structure of QCD in parton shower Monte Carlo generators PI: Christian Bauer, Lawrence Berkeley National Laboratory Co-PIs: Wibe de Jong and Ben Nachman (LBNL) The HEP.QPR Project: Quantum Pattern Recognition for Charged Particle Tracking PI: Heather Gray, Lawrence Berkeley National Laboratory Co-PIs: Wahid Bhimji, Paolo Calafiura, Steve Farrell, Wim Lavrijsen, Lucy Linder, Illya Shapoval (LBNL) Neutrino-Nucleus Scattering on a Quantum Computer PI: Rajan Gupta, Los Alamos National Laboratory Co-PIs: Joseph Carlson (LANL); Alessandro Roggero (UW), Gabriel Purdue (FNAL) Particle Track Pattern Recognition via Content-Addressable Memory and Adiabatic Quantum Optimization PI: Lauren Ice, Johns Hopkins University Co-PIs: Gregory Quiroz (Johns Hopkins); Travis Humble (Oak Ridge National Laboratory) Towards practical quantum simulation for High Energy Physics PI: Peter Love, Tufts University Co-PIs: Gary Goldstein, Hugo Beauchemin (Tufts) High Energy Physics (HEP) ML and Optimization Go Quantum PI: Gabriel Perdue, Fermilab Co-PIs: Jim Kowalkowski, Stephen Mrenna, Brian Nord, Aris Tsaris (Fermilab); Travis Humble, Alex McCaskey (Oak Ridge National Lab) Quantum Machine Learning and Quantum Computation Frameworks for HEP (QMLQCF) PI: M. Spiropulu, California Institute of Technology Co-PIs: Panagiotis Spentzouris (Fermilab), Daniel Lidar (USC), Seth Lloyd (MIT) Quantum Algorithms for Collider Physics PI: Jesse Thaler, Massachusetts Institute of Technology Co-PI: Aram Harrow, Massachusetts Institute of Technology Quantum Machine Learning for Lattice QCD PI: Boram Yoon, Los Alamos National Laboratory Co-PIs: Nga T. T. Nguyen, Garrett Kenyon, Tanmoy Bhattacharya and Rajan Gupta (LANL) Quantum Information Science in High Energy Physics at the Large Hadron Collider O.K. -
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. -
Mariangela Lisanti
Mariangela Lisanti Academic Appointments Princeton University 2013–present Assistant Professor Princeton Center for Theoretical Science (PCTS) 2010–2013 Simons Foundation Postdoctoral Fellow Education Stanford University, Ph.D. 2005–2010 Thesis: “The Search for Dark Matter: From Colliders to Direct Detection Experiments” Advisor: Jay G. Wacker Harvard University, B.A. summa cum laude 2001–2005 Project: Casimir Force in Microelectromechanical Systems Advisor: Federico Capasso Awards and Honors 2017 Cottrell Scholar Award 2016 Sloan Research Fellowship 2013 Blavatnik Award for Young Scientists, Postdoctoral Finalist 2012 Aspen Center for Physics Block Award 2010 LHC Theory Initiative Travel and Computing Award 2009 Phi Beta Kappa Scholarship 2008 Paul Kirkpatrick Award (excellence in teaching undergraduate physics) US representative to Lindau Nobel Laureates Meeting 2007 Paul & Daisy Soros Fellowship for New Americans 2005 Phi Beta Kappa National Science Foundation Graduate Research Fellowship National Defense Science and Engineering Graduate Research Fellowship Stanford Humanities and Sciences Fellowship 2004 Barry L. Goldwater Scholar Bossert Book Award (outstanding scientific achievement at Harvard) Harvard College Scholarship 2003 John Harvard Scholar 2002 TR100 Award (world’s top innovators under the age of 35) Harvard College Scholarship 2001 First Prize National Winner of the Intel Science Talent Search Glenn T. Seaborg Nobel Prize Visit Award (first place award at Intel ISEF) Attended Nobel Prize Ceremony, December 2001 Presidential Scholar Academy of Achievement Golden Eagle Award 1 IEEE President’s Scholarship Award Academy of Achievement Salute to Excellence Program, San Antonio, TX National Merit Scholarship Honorary citation from Connecticut governor 2000 First Prize National Winner of the Siemens Westinghouse Science & Technology Competition Siemens Award for Advanced Placement Governor’s Scholar Teaching Physics 529: Introduction to High Energy Physics (graduate) Spring: 2015, 2016 Physics 406: Modern Physics II—Nuclear & Elem. -
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, -
The 19Th Particles and Nuclei International Conference (PANIC11)
The 19th Particles and Nuclei International Conference (PANIC11) Monday 25 July Tuesday 26 July Wednesday 27 July Thursday 28 July Friday 29 July 8:30 Opening Remarks Plenary 2 Plenary 3 Plenary 4 Plenary 5 Kresge Auditorium Kresge Auditorium Kresge Auditorium Kresge Auditorium Kresge Auditorium Chair: Richard Milner (08:30-10:15) (08:30-10:15) (08:30-10:15) (08:30-10:15) (MIT) Chair: Johanna Stachel Chair: Frithjof Karsch Chair: Jean-Paul Blaizot Chair: Giorgio Gratta Dr. Susan Hockfield, (University of (Brookhaven National (CEA, France) (Stanford University) President of MIT Heidelberg) Laboratory) Prof. Edmund Bertschinger, Head of MIT Dept. of Physics Plenary 1 8:30 P2-1 Glimpsing the Fly 8:30 P3-1 Recent Progress in 8:30 P4-1 Collective 8:30 P5-1 Latest Results in Kresge Auditorium in the Cathedral: Applying Gauge/ Gravity Behavior in Heavy Ion Heavy Flavour Physics (08:55-10:05) Marking the Centennial Duality to Quark-Gluon Collisions Guy WILKINSON Chair: Susan Seestrom of the First Description Plasma and Nuclear Constantin LOIZIDES (University of Oxford) (LANL) of the Atomic Nucleus Physics (LBNL) Brian CATHCART Andreas KARCH (Univ. of (Kingston University) Washington) 8:55 P1-1 Dark matter: new 9:05 P2-2 New Physics 9:05 P3-2 Light Baryon 9:05 P4-2 Hard Probes of 9:05 P5-2 Seeking the origin results from direct Discoveries at the Spectroscopy Quark-Gluon Plasma in of mass: Higgs searches detection Quark and Lepton Volker CREDE (Florida Heavy Ion Collisions at Colliders Laura BAUDIS Luminosity Frontiers or State University) Carlos -
Springer Proceedings in Physics
Springer Proceedings in Physics Volume 148 For further volumes: http://www.springer.com/series/361 David Cline Editor Sources and Detection of Dark Matter and Dark Energy in the Universe Proceedings of the 10th UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe, February 22-24, 2012, Marina del Rey, California Editor David Cline UCLA Physics & Astronomy Los Angeles , USA ISSN 0930-8989 ISSN 1867-4941 (electronic) ISBN 978-94-007-7240-3 ISBN 978-94-007-7241-0 (eBook) DOI 10.1007/978-94-007-7241-0 Springer Dordrecht Heidelberg New York London Library of Congress Control Number: 2013955385 © Springer Science+Business Media Dordrecht 2013 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifi cally the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfi lms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. Exempted from this legal reservation are brief excerpts in connection with reviews or scholarly analysis or material supplied specifi cally for the purpose of being entered and executed on a computer system, for exclusive use by the purchaser of the work. Duplication of this publication or parts thereof is permitted only under the provisions of the Copyright Law of the Publisher’s location, in its current version, and permission for use must always be obtained from Springer. Permissions for use may be obtained through RightsLink at the Copyright Clearance Center. -
By Lindley Winslow and Jesse Thaler
Listening for Dark Matter by Lindley Winslow and Jesse Thaler 34 ) winslow | thaler mit physics annual 2019 ooking out into the night sky, it is humbling to contemplate the vast- L ness of the universe. Yet the twinkling of those stars—both in our Milky Way and in distant galaxies—represent only a small fraction of the universe’s mass. Even including plumes of interstellar gas, ordinary matter can only account for around 15% of the matter in the universe. The other 85% is dark matter, completely invisible to our eyes but firmly established scientifically through its gravitational influence. WHAT IS DARK MATTER? Fundamentally, we simply do not know. We can infer its existence from the dynamics of galaxies, from its fingerprint on cosmic radiation, and from the way it bends light from ancient objects. We know how much dark matter there is now, how much there was in the early universe, and even roughly how fast it moves. We also know that dark from the Basement of Bldg. 24 mit physics annual 2019 winslow | thaler ( 35 matter formed a kind of gravitational scaffolding that allowed galaxies like our Milky Way to take shape. In that sense, we owe our very existence to this strange invisible substance. But we do not yet know what it is. This uncertainty surrounding dark matter—along with null results from previous searches—has led to an explosion of new detec- tion proposals in recent years, some more realistic than others. It has also led to an equally large explosion of new theories for dark matter, some more well-motivated than others. -
Mathematical Physics and String Theory
TIFR Annual Report 2002-03 THEORETICAL PHYSICS String Theory and Mathematical Physics Closed String Tachyon Potential Calculation The closed string 4-Tachyon amplitude in C/ZN orbifold was calculated. In an appropriate large N limit, this will throw some light on the behaviour of closed string tachyon potential in target space. [Allan Adams, Atish Dabholkar, Ashik Iqubal, Joris Raeymaekers] Compactification by Duality Twists The Scherk-Schwarz potential generated by string theory compactifications was investigated in the case of twists belonging to the duality group. For some twists, such twisted compactifications are equivalent to introducing internal fluxes. [Atish Dabholkar, Ashik Iqubal, Prasanta Tripathy, Sandip Trivedi] Duality twists, Fluxes, and Orbifolds An important problem in string theory is to generate a potential for the unwanted massless moduli fields. With this motivation, compactifications with duality twists and their relation to orbifolds and compactifications with fluxes were investigated. Inequivalent compactifications were classified by conjugacy classes of the U-duality group and resulted in gauged supergravities in lower dimensions with nontrivial potential on the moduli space. It was shown that the potential has a stable minima precisely at the fixed points of the twist group and that the theory at the minimum has an exact CFT description as an orbifold. The implications of these results for moduli stablization is under investigation. [Atish Dabholkar with Chris Hull] Tachyon Condensation in String Theory Usually F-theory duals of string theory are considered for supersymmetric backgrounds. F- theory duals of certain nonsupersymmetric backgrounds were considered that have localized tachyons. Some speculations about the endpoint of the tachyon condensation were presented based on this duality.