Three Duality Symmetries Between Photons and Cosmic String Loops, and Macro and Micro Black Holes
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M2-Branes Ending on M5-Branes
M2-branes ending on M5-branes Vasilis Niarchos Crete Center for Theoretical Physics, University of Crete 7th Crete Regional Meeting on String Theory, 27/06/2013 based on recent work with K. Siampos 1302.0854, ``The black M2-M5 ring intersection spins’‘ Proceedings Corfu Summer School, 2012 1206.2935, ``Entropy of the self-dual string soliton’’, JHEP 1207 (2012) 134 1205.1535, ``M2-M5 blackfold funnels’’, JHEP 1206 (2012) 175 and older work with R. Emparan, T. Harmark and N. A. Obers ➣ blackfold theory 1106.4428, ``Blackfolds in Supergravity and String Theory’’, JHEP 1108 (2011) 154 0912.2352, ``New Horizons for Black Holes and Branes’’, JHEP 1004 (2010) 046 0910.1601, ``Essentials of Blackfold Dynamics’’, JHEP 1003 (2010) 063 0902.0427, ``World-Volume Effective Theory for Higher-Dimensional Black Holes’’, PRL 102 (2009)191301 0708.2181, ``The Phase Structure of Higher-Dimensional Black Rings and Black Holes’‘ + M.J. Rodriguez JHEP 0710 (2007) 110 2 Important lessons about the fundamentals of string/M-theory (and QFT) are obtained by studying the low-energy theories on D-branes and M-branes. Most notably in M-theory, recent progress has clarified the low-energy QFT on N M2-brane and the N3/2 dof that it exhibits. Bagger-Lambert ’06, Gustavsson ’07, ABJM ’08 Drukker-Marino-Putrov ’10 Our understanding of the M5-brane theory is more rudimentary, but efforts to identify analogous properties, e.g. the N3 scaling of the massless dof, is underway. Douglas ’10 Lambert,Papageorgakis,Schmidt-Sommerfeld ’10 Hosomichi-Seong-Terashima ’12 Kim-Kim ’12 Kallen-Minahan-Nedelin-Zabzine ’12 .. -
Kaluza-Klein Gravity, Concentrating on the General Rel- Ativity, Rather Than Particle Physics Side of the Subject
Kaluza-Klein Gravity J. M. Overduin Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, British Columbia, Canada, V8W 3P6 and P. S. Wesson Department of Physics, University of Waterloo, Ontario, Canada N2L 3G1 and Gravity Probe-B, Hansen Physics Laboratories, Stanford University, Stanford, California, U.S.A. 94305 Abstract We review higher-dimensional unified theories from the general relativity, rather than the particle physics side. Three distinct approaches to the subject are identi- fied and contrasted: compactified, projective and noncompactified. We discuss the cosmological and astrophysical implications of extra dimensions, and conclude that none of the three approaches can be ruled out on observational grounds at the present time. arXiv:gr-qc/9805018v1 7 May 1998 Preprint submitted to Elsevier Preprint 3 February 2008 1 Introduction Kaluza’s [1] achievement was to show that five-dimensional general relativity contains both Einstein’s four-dimensional theory of gravity and Maxwell’s the- ory of electromagnetism. He however imposed a somewhat artificial restriction (the cylinder condition) on the coordinates, essentially barring the fifth one a priori from making a direct appearance in the laws of physics. Klein’s [2] con- tribution was to make this restriction less artificial by suggesting a plausible physical basis for it in compactification of the fifth dimension. This idea was enthusiastically received by unified-field theorists, and when the time came to include the strong and weak forces by extending Kaluza’s mechanism to higher dimensions, it was assumed that these too would be compact. This line of thinking has led through eleven-dimensional supergravity theories in the 1980s to the current favorite contenders for a possible “theory of everything,” ten-dimensional superstrings. -
Uncertainty Relation on a World Crystal and Its Applications to Micro Black Holes
PHYSICAL REVIEW D 81, 084030 (2010) Uncertainty relation on a world crystal and its applications to micro black holes Petr Jizba,1,2,* Hagen Kleinert,1,† and Fabio Scardigli3,‡ 1ITP, Freie Universita¨t Berlin, Arnimallee 14 D-14195 Berlin, Germany 2FNSPE, Czech Technical University in Prague, Brˇehova´ 7, 115 19 Praha 1, Czech Republic 3Leung Center for Cosmology and Particle Astrophysics (LeCosPA), Department of Physics, National Taiwan University, Taipei 106, Taiwan (Received 17 December 2009; published 16 April 2010) We formulate generalized uncertainty relations in a crystal-like universe—a ‘‘world crystal’’—whose lattice spacing is of the order of Planck length. In the particular case when energies lie near the border of the Brillouin zone, i.e., for Planckian energies, the uncertainty relation for position and momenta does not pose any lower bound on involved uncertainties. We apply our results to micro black holes physics, where we derive a new mass-temperature relation for Schwarzschild micro black holes. In contrast to standard results based on Heisenberg and stringy uncertainty relations, our mass-temperature formula predicts both a finite Hawking’s temperature and a zero rest-mass remnant at the end of the micro black hole evaporation. We also briefly mention some connections of the world-crystal paradigm with ’t Hooft’s quantization and double special relativity. DOI: 10.1103/PhysRevD.81.084030 PACS numbers: 04.70.Dy, 03.65. w À I. INTRODUCTION from numerical computations. One may, however, inves- tigate the consequences of taking the lattice no longer as a Recent advances in gravitational and quantum physics mere computational device, but as a bona fide discrete indicate that in order to reconcile the two fields with each network, whose links define the only possible propagation other, a dramatic conceptual shift is required in our under- directions for signals carrying the interactions between standing of spacetime. -
Durham E-Theses
Durham E-Theses Black holes, vacuum decay and thermodynamics CUSPINERA-CONTRERAS, JUAN,LEOPOLDO How to cite: CUSPINERA-CONTRERAS, JUAN,LEOPOLDO (2020) Black holes, vacuum decay and thermodynamics, Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/13421/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk Black holes, vacuum decay and thermodynamics Juan Leopoldo Cuspinera Contreras A Thesis presented for the degree of Doctor of Philosophy Institute for Particle Physics Phenomenology Department of Physics University of Durham England September 2019 To my family Black holes, vacuum decay and thermodynamics Juan Leopoldo Cuspinera Contreras Submitted for the degree of Doctor of Philosophy September 2019 Abstract In this thesis we study two fairly different aspects of gravity: vacuum decay seeded by black holes and black hole thermodynamics. The first part of this work is devoted to the study of black holes within the (higher dimensional) Randall- Sundrum braneworld scenario and their effect on vacuum decay rates. -
Emergent Gravity As the Nematic Dual of Lorentz-Invariant Elasticity
SMR 1646 - 12 ___________________________________________________________ Conference on Higher Dimensional Quantum Hall Effect, Chern-Simons Theory and Non-Commutative Geometry in Condensed Matter Physics and Field Theory 1 - 4 March 2005 ___________________________________________________________ Emergent gravity as the nematic dual of Lorentz-invariant Elasticity Johannes ZAANEN Stanford Univ., Stanford, U.S.A. ___________________________________________________________________ These are preliminary lecture notes, intended only for distribution to participants. EmergentEmergent gravitygravity asas thethe nematicnematic dualdual ofof LorentzLorentz--invariantinvariant ElasticityElasticityTalk Jan Zaanen Hagen Kleinert Sergei Mukhin Zohar Nussinov Vladimir Cvetkovic 1 Emergent Einstein Gravity c 3 S =− dV −g R + S 16πG ∫ matter Einstein’s space time = the Lorentz invariant topological nematic superfluid (at least in 2+1D) A medium characterized by: - emergent general covariance - absence of torsion- and compressional rigidity - presence of curvature rigidity (topological order) 2 Plan of talk 1. Plasticity (defected elasticity) and differential geometry 2. Fluctuating order and high Tc superconductivity 3. Dualizing non-relativistic quantum elasticity 3.a Quantum nematic orders 3.b Superconductivity: dual Higgs is Higgs 4. The quantum nematic world crystal and Einstein’s space time 3 Quantum-elasticity: basics Quantum elastic action, isotropic medium ν ⎡ 2 2 2 2 2 2⎤ S = µ u + 2u + u + ()u + u + ()∂τ u + ()∂τ u ⎣⎢ xx xy yy 1−ν xx yy x y ⎦⎥ Shear modulus µ, Poisson ratio ν, compression modulus κ = µ()1 + ν /1()− ν 2 = µ ρ = = = ()∂ + ∂ c ph 2 / 1, h 1, uab a ub b ua /2 Describes transversal- (T) and longitudinal (L) phonon, 2 2 ⎡⎛ q ⎞ ⎛ q ⎞ ⎤ S = µ ⎢⎜ + ω 2 ⎟ | uT |2 +⎜ + ω 2 ⎟ | uL |2⎥ ⎣⎝ 2 ⎠ ⎝ 1−ν ⎠ ⎦ 4 Elasticity and topology: the dislocation J.M. -
Link to the Live Plenary Sessions
IWARA2020 Video Conference Mexico City time zone, Mexico 9th International Workshop on Astronomy and Relativistic Astrophysics 6 – 12 September, 2020 Live Plenary Talks Program SUNDAY MONDAY TUESDAY WEDNESDAY THURSDAY FRIDAY SATURDAY DAYS/HOUR 06/09/2020 07/09/2020 08/09/2020 09/09/2020 10/09/2020 11/09/2020 12/09/2020 COSMOLOGY, DE MMA, DE, DM, CCGG COMPSTARS, DM, GWS DENSE MATTER, QCD DM, DE, GWS, BHS DENSE MATTER, SNOVAE ARCHAEOASTRONOMY TOPICS DM, COMPACT STARS X- & CR- RAYS, MWA PARTICLES, ϒ-RAYS QGP, QFT, HIC, GWS GRAVITATION, GALAXIES DM, COMPACT STARS BHS, GRBS, SNOVAE GRAVITY, BHS, GWS NSS, SNOVAE, GRAVITY QCD, HIC, SNOVAE DM, COSMOLOGY EROSITA DE, BHS, COSMOLOGY LIVE PLENARY TALKS PETER HESS & THOMAS BOLLER & STEVEN GULLBERG & PETER HESS & Steven Gullberg & LUIS UREÑA-LOPEZ & PETER HESS & MODERATORS CESAR ZEN GABRIELLA PICCINELLI CESAR ZEN THOMAS BOLLER Luis Ureña-Lopes BENNO BODMANN CESAR ZEN 07:00 WAITING ROOM WAITING ROOM WAITING ROOM WAITING ROOM WAITING ROOM WAITING ROOM WAITING ROOM 07:45 OPENING 08:00 R. SACAHUI P. SLANE A. SANDOVAL S. FROMENTEAU G. PICCINELLI V. KARAS F. MIRABEL60’ 08:30 M. GAMARRA U. BARRES G. WOLF J. RUEDA R. XU J. STRUCKMEIER60’ 09:00 ULLBERG ARRISON ANAUSKE ENEZES EXHEIMER S. G D. G M. H D. M 60’ V. D D. ROSIŃSKA 09:30 V. ORTEGA G. ROMERO D. VASAK D. PAGE J. AICHELIN M. VARGAS 10:00 – CONFERENCE-BREAK: VIDEO-SYNTHESIS OF RECORDED VIDEOS LIVE SPOTLIGHTS TALKS MODERATORS MARIANA VARGAS MAGAÑA & GABRIELLA PICCINELLI 10:15 J. HORVATH Spotlight Session 1 SPOTLIGHT SESSION 2 Spotlight Session 3 Spotlight Session 4 Spotlight Session 5 SPOTLIGHT SESSION 6 MARCOS MOSHINSKY 10:45 AWARD 11:15 – CONFERENCE-BREAK: VIDEO-SYNTHESIS OF RECORDED VIDEOS LIVE PLENARY TALKS PETER HESS & THOMAS BOLLER & STEVEN GULLBERG & PETER HESS & Steven Gullberg & LUIS UREÑA-LOPEZ & PETER HESS & MODERATORS CESAR ZEN GABRIELLA PICCINELLI CESAR ZEN THOMAS BOLLER Luis Ureña-Lopes BENNO BODMANN CESAR ZEN C. -
From Vibrating Strings to a Unified Theory of All Interactions
Barton Zwiebach From Vibrating Strings to a Unified Theory of All Interactions or the last twenty years, physicists have investigated F String Theory rather vigorously. The theory has revealed an unusual depth. As a result, despite much progress in our under- standing of its remarkable properties, basic features of the theory remain a mystery. This extended period of activity is, in fact, the second period of activity in string theory. When it was first discov- ered in the late 1960s, string theory attempted to describe strongly interacting particles. Along came Quantum Chromodynamics— a theoryof quarks and gluons—and despite their early promise, strings faded away. This time string theory is a credible candidate for a theoryof all interactions—a unified theoryof all forces and matter. The greatest complication that frustrated the search for such a unified theorywas the incompatibility between two pillars of twen- tieth century physics: Einstein’s General Theoryof Relativity and the principles of Quantum Mechanics. String theory appears to be 30 ) zwiebach mit physics annual 2004 the long-sought quantum mechani- cal theory of gravity and other interactions. It is almost certain that string theory is a consistent theory. It is less certain that it describes our real world. Nevertheless, intense work has demonstrated that string theory incorporates many features of the physical universe. It is reasonable to be very optimistic about the prospects of string theory. Perhaps one of the most impressive features of string theory is the appearance of gravity as one of the fluctuation modes of a closed string. Although it was not discov- ered exactly in this way, we can describe a logical path that leads to the discovery of gravity in string theory. -
The Fuzzball Proposal for Black Holes: an Elementary Review
hep-th/0502050 The fuzzball proposal for black holes: an elementary review1 Samir D. Mathur Department of Physics, The Ohio State University, Columbus, OH 43210, USA [email protected] Abstract We give an elementary review of black holes in string theory. We discuss BPS holes, the microscopic computation of entropy and the ‘fuzzball’ picture of the arXiv:hep-th/0502050v1 3 Feb 2005 black hole interior suggested by microstates of the 2-charge system. 1Lecture given at the RTN workshop ‘The quantum structure of space-time and the geometric nature of fundamental interactions’, in Crete, Greece (September 2004). 1 Introduction The quantum theory of black holes presents many paradoxes. It is vital to ask how these paradoxes are to be resolved, for the answers will likely lead to deep changes in our understanding of quantum gravity, spacetime and matter. Bekenstein [1] argued that black holes should be attributed an entropy A S = (1.1) Bek 4G where A is the area of the horizon and G is the Newton constant of gravitation. (We have chosen units to set c = ~ = 1.) This entropy must be attributed to the hole if we are to prevent a violation of the second law of thermodynamics. We can throw a box of gas with entropy ∆S into a black hole, and see it vanish into the central singularity. This would seem to decrease the entropy of the Universe, but we note that the area of the horizon increases as a result of the energy added by the box. It turns out that if we assign (1.1) as the entropy of the hole then the total entropy is nondecreasing dS dS Bek + matter 0 (1.2) dt dt ≥ This would seem to be a good resolution of the entropy problem, but it leads to another problem. -
String Theory for Pedestrians
String Theory for Pedestrians – CERN, Jan 29-31, 2007 – B. Zwiebach, MIT This series of 3 lecture series will cover the following topics 1. Introduction. The classical theory of strings. Application: physics of cosmic strings. 2. Quantum string theory. Applications: i) Systematics of hadronic spectra ii) Quark-antiquark potential (lattice simulations) iii) AdS/CFT: the quark-gluon plasma. 3. String models of particle physics. The string theory landscape. Alternatives: Loop quantum gravity? Formulations of string theory. 1 Introduction For the last twenty years physicists have investigated String Theory rather vigorously. Despite much progress, the basic features of the theory remain a mystery. In the late 1960s, string theory attempted to describe strongly interacting particles. Along came Quantum Chromodynamics (QCD)– a theory of quarks and gluons – and despite their early promise, strings faded away. This time string theory is a credible candidate for a theory of all interactions – a unified theory of all forces and matter. Additionally, • Through the AdS/CFT correspondence, it is a valuable tool for the study of theories like QCD. • It has helped understand the origin of the Bekenstein-Hawking entropy of black holes. • Finally, it has inspired many of the scenarios for physics Beyond the Standard Model of Particle physics. 2 Greatest problem of twentieth century physics: the incompatibility of Einstein’s General Relativity and the principles of Quantum Mechanics. String theory appears to be the long-sought quantum mechanical theory of gravity and other interactions. It is almost certain that string theory is a consistent theory. It is less certain that it describes our real world. -
Arxiv:0912.2253V2 [Hep-Th] 19 Dec 2009 ‡ † ∗ Rcsi Ellratmt 1,1,1,1,15]
Uncertainty relation on world crystal and its applications to micro black holes Petr Jizba,1,2, ∗ Hagen Kleinert,1, † and Fabio Scardigli3, ‡ 1ITP, Freie Universit¨at Berlin, Arnimallee 14 D-14195 Berlin, Germany 2FNSPE, Czech Technical University in Prague, B˘rehov´a7, 115 19 Praha 1, Czech Republic 3Leung Center for Cosmology and Particle Astrophysics (LeCosPA), Department of Physics, National Taiwan University, Taipei 106, Taiwan We formulate generalized uncertainty relations in a crystal-like universe whose lattice spacing is of the order of Planck length — “world crystal”. In the particular case when energies lie near the border of the Brillouin zone, i.e., for Planckian energies, the uncertainty relation for position and momenta does not pose any lower bound on involved uncertainties. We apply our results to micro black holes physics, where we derive a new mass-temperature relation for Schwarzschild micro black holes. In contrast to standard results based on Heisenberg and stringy uncertainty relations, our mass-temperature formula predicts both a finite Hawking’s temperature and a zero rest-mass remnant at the end of the micro black hole evaporation. We also briefly mention some connections of the world crystal paradigm with ’t Hooft’s quantization and double special relativity. PACS numbers: 04.70.Dy, 03.65.-w I. INTRODUCTION tions. One may, however, investigate the consequences of taking the lattice no longer as a mere computational Recent advances in gravitational and quantum physics device, but as a bona-fide discrete network, whose links indicate that in order to reconcile the two fields with define the only possible propagation directions for sig- each other, a dramatic conceptual shift is required in nals carrying the interactions between fields sitting on our understanding of spacetime. -
Generic Affinities, Posthumanisms and Science-Fictional Imaginings
GENERIC AFFINITIES, POSTHUMANISMS, SCIENCE-FICTIONAL IMAGININGS SPECULATIVE MATTER: GENERIC AFFINITIES, POSTHUMANISMS AND SCIENCE-FICTIONAL IMAGININGS By LAURA M. WIEBE, B.A., M.A. A Thesis Submitted to the School of Graduate Studies in Partial Fulfilment of the Requirements for the Degree of Doctor of Philosophy McMaster University © Copyright by Laura Wiebe, October 2012 McMaster University DOCTOR OF PHILOSOPHY (2012) Hamilton, Ontario (English and Cultural Studies) TITLE: Speculative Matter: Generic Affinities, Posthumanisms and Science-Fictional Imaginings AUTHOR: Laura Wiebe, B.A. (University of Waterloo), M.A. (Brock University) SUPERVISOR: Professor Anne Savage NUMBER OF PAGES: vi, 277 ii ABSTRACT Amidst the technoscientific ubiquity of the contemporary West (or global North), science fiction has come to seem the most current of genres, the narrative form best equipped to comment on and work through the social, political and ethical quandaries of rapid technoscientific development and the ways in which this development challenges conventional understandings of human identity and rationality. By this framing, the continuing popularity of stories about paranormal phenomena and supernatural entities – on mainstream television, or in print genres such as urban fantasy and paranormal romance – may seem to be a regressive reaction against the authority of and experience of living in technoscientific modernity. Nevertheless, the boundaries of science fiction, as with any genre, are relational rather than fixed, and critical engagements with Western/Northern technoscientific knowledge and practice and modern human identity and being may be found not just in science fiction “proper,” or in the scholarly field of science and technology studies, but also in the related genres of fantasy and paranormal romance. -
Introduction to String Theory A.N
Introduction to String Theory A.N. Schellekens Based on lectures given at the Radboud Universiteit, Nijmegen Last update 6 July 2016 [Word cloud by www.worldle.net] Contents 1 Current Problems in Particle Physics7 1.1 Problems of Quantum Gravity.........................9 1.2 String Diagrams................................. 11 2 Bosonic String Action 15 2.1 The Relativistic Point Particle......................... 15 2.2 The Nambu-Goto action............................ 16 2.3 The Free Boson Action............................. 16 2.4 World sheet versus Space-time......................... 18 2.5 Symmetries................................... 19 2.6 Conformal Gauge................................ 20 2.7 The Equations of Motion............................ 21 2.8 Conformal Invariance.............................. 22 3 String Spectra 24 3.1 Mode Expansion................................ 24 3.1.1 Closed Strings.............................. 24 3.1.2 Open String Boundary Conditions................... 25 3.1.3 Open String Mode Expansion..................... 26 3.1.4 Open versus Closed........................... 26 3.2 Quantization.................................. 26 3.3 Negative Norm States............................. 27 3.4 Constraints................................... 28 3.5 Mode Expansion of the Constraints...................... 28 3.6 The Virasoro Constraints............................ 29 3.7 Operator Ordering............................... 30 3.8 Commutators of Constraints.......................... 31 3.9 Computation of the Central Charge.....................