Mathematics and Physics of Branes in String and M -Theory 3 January – 29 June 2012 Isaac Newton Institute Final Report
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String Phenomenology
Introduction Model Building Moduli Stabilisation Flavour Problem String Phenomenology Joseph Conlon (Oxford University) EPS HEP Conference, Krakow July 17, 2009 Joseph Conlon (Oxford University) String Phenomenology Introduction Model Building Moduli Stabilisation Flavour Problem Chalk and Cheese? Figure: String theory and phenomenology? Joseph Conlon (Oxford University) String Phenomenology Introduction Model Building Moduli Stabilisation Flavour Problem String Theory ◮ String theory is where one is led by studying quantised relativistic strings. ◮ It encompasses lots of areas ( black holes, quantum field theory, quantum gravity, mathematics, particle physics....) and is studied by lots of different people. ◮ This talk is on string phenomenology - the part of string theory that aims at connecting to the Standard Model and its extensions. ◮ It aims to provide a (brief) overview of this area. (cf Angel Uranga’s plenary talk) Joseph Conlon (Oxford University) String Phenomenology Introduction Model Building Moduli Stabilisation Flavour Problem String Theory ◮ For technical reasons string theory is consistent in ten dimensions. ◮ Six dimensions must be compactified. ◮ Ten = (Four) + (Six) ◮ Spacetime = (M4) + Calabi-Yau Space ◮ All scales, matter, particle spectra and couplings come from the geometry of the extra dimensions. ◮ All scales, matter, particle spectra and couplings come from the geometry of the extra dimensions. Joseph Conlon (Oxford University) String Phenomenology Introduction Model Building Moduli Stabilisation Flavour Problem Model Building Various approaches in string theory to realising Standard Model-like spectra: ◮ E8 E8 heterotic string with gauge bundles × ◮ Type I string with gauge bundles ◮ IIA/IIB D-brane constructions ◮ Heterotic M-Theory ◮ M-Theory on G2 manifolds Joseph Conlon (Oxford University) String Phenomenology Introduction Model Building Moduli Stabilisation Flavour Problem Heterotic String Start with an E8 vis E8 hid gauge group in ten dimensions. -
Summary of Indian Strings Meeting 2007
Conference Statistics The Talks Summary of Indian Strings Meeting 2007 Sunil Mukhi, TIFR HRI, Allahabad October 15-19 2007 Sunil Mukhi, TIFR Summary of Indian Strings Meeting 2007 Conference Statistics The Talks Outline 1 Conference Statistics 2 The Talks Sunil Mukhi, TIFR Summary of Indian Strings Meeting 2007 There were 3 discussion sessions of 90 minutes each. At four full days (Monday afternoon – Friday lunch) this must be the shortest ISM ever! Conference Statistics The Talks Conference Statistics This conference featured 27 talks: 4 × 90 minutes 23 × 30 minutes Sunil Mukhi, TIFR Summary of Indian Strings Meeting 2007 At four full days (Monday afternoon – Friday lunch) this must be the shortest ISM ever! Conference Statistics The Talks Conference Statistics This conference featured 27 talks: 4 × 90 minutes 23 × 30 minutes There were 3 discussion sessions of 90 minutes each. Sunil Mukhi, TIFR Summary of Indian Strings Meeting 2007 Conference Statistics The Talks Conference Statistics This conference featured 27 talks: 4 × 90 minutes 23 × 30 minutes There were 3 discussion sessions of 90 minutes each. At four full days (Monday afternoon – Friday lunch) this must be the shortest ISM ever! Sunil Mukhi, TIFR Summary of Indian Strings Meeting 2007 IOPB, IMSc and SINP were out for a ! South Zone and East Zone were very scarcely represented. Conference Statistics The Talks The scorecard for the talks was as follows: Institute Faculty Postdocs Students Total HRI 4 3 5 12 TIFR 3 3 2 8 IIT-K 1 0 1 2 Utkal 1 0 0 1 IIT-R 1 0 0 1 IIT-M 0 0 1 1 IACS 0 0 1 1 Kings 1 0 0 1 Total 11 6 10 27 Sunil Mukhi, TIFR Summary of Indian Strings Meeting 2007 South Zone and East Zone were very scarcely represented. -
Mathematical Physics and String Theory
TIFR Annual Report 2001-02 THEORETICAL PHYSICS String Theory and Mathematical Physics Tachyon Condensation and Black Hole Entropy Condensation of tahcyons in closed string theory was analyzed and its connection with the computation of the black hole entropy was pointed out. The entropy computed in this manner was found to be in precise agreement with the the Bekenstein-Hawking Entropy. [Atish Dabholkar] Tachyon Potential and C-function A tachyon potential with the appropriate critical points was proposed in terms of an effective c-function of the worldsheet theory and it was determined as a solution of certain integrable equations. [Atish Dabholkar and C. Vafa of Harvard University] D-branes in PP-wave Backgrounds Dirichlet branes in the background of a PP wave were constructed and the open string spectrum was in agreement with the gauge theory spectrum. [Atish Dabholkar and Sharoukh Parvizi] Loop Equation and Wilson Line Correlators in Non-commutative Gauge Theories Loop equations for correlators of Wilson line operators in non-commutative gauge theories were derived. Unlike what happens for closed Wilson loops, the joining term survives in the planar equations. This fact was used to obtain a NEW loop equation which relates the correlation function of an arbitrary number of Wilson lines to a set of closed Wilson loops, obtained by joining the individual Wilson lines together by a series of well-defined cutting and joining manipulations. For closed loops, we showed that the non-planar contributions do not have a smooth limit in the limit of vanishing non-commutativity and hence the equations do not reduce to their commutative counterparts [Avinash Dhar and Y. -
String Phenomenology 1 Minimal Supersymmetric Standard Model
Swedish String/Supergravity Course 2008 String Phenomenology Marcus Berg 1 Minimal Supersymmetric Standard Model A good reference is Martin [2], a review that was first posted on hep-ph in 1997 but which has been updated three times, most recently in 2006. The MSSM consists of a number of chiral and vector supermultiplets, one for each existing quark or 1 lepton or gauge boson Aµ in the Standard Model (SM): spin: 0 1/2 1 N = 1 chiral supermultiplet φ N = 1 vector supermultiplet λ Aµ The new fields, the superpartners of and Aµ, are denoted by tildes and called "s-" for the new scalars, ~, and "-ino" for the new fermions, A~: 0 1/2 1 squarks, sleptons −! ~ − quarks, leptons gauginos−! A~ Aµ − gauge bosons This is just the generic notation; usually one is more specific. So for example, one N = 1 chiral mul- tiplet has the t quark as the fermionic field, and the scalar superpartner is the "stop", t~. We impose that the superpartner masses are around the TeV scale, or even a little lower. The scale of superpartner masses is not \derived" in any real sense2 in the MSSM, but from the point of view of particle phenomenology, an MSSM-like theory with only very heavy superpartners would be indistinguishable from the nonsuper- symmetric standard model at any experiments done in the foreseeable future, so why bother? In fact, even string theorists should have some favored scenario what will happen at near-future experiments and observations, so let's try to understand where people who do experiments for a living have put their money. -
IISER AR PART I A.Cdr
dm{f©H$ à{VdoXZ Annual Report 2016-17 ^maVr¶ {dkmZ {ejm Ed§ AZwg§YmZ g§ñWmZ nwUo Indian Institute of Science Education and Research Pune XyaX{e©Vm Ed§ bú` uCƒV‘ j‘Vm Ho$ EH$ Eogo d¡km{ZH$ g§ñWmZ H$s ñWmnZm {Og‘| AË`mYw{ZH$ AZwg§YmZ g{hV AÜ`mnZ Ed§ {ejm nyU©ê$n go EH$sH¥$V hmo& u{Okmgm Am¡a aMZmË‘H$Vm go `wº$ CËH¥$ï> g‘mH$bZmË‘H$ AÜ`mnZ Ho$ ‘mÜ`m‘ go ‘m¡{bH$ {dkmZ Ho$ AÜ``Z H$mo amoMH$ ~ZmZm& ubMrbo Ed§ Agr‘ nmR>çH«$‘ VWm AZwg§YmZ n[a`moOZmAm| Ho$ ‘mÜ`‘ go N>moQ>r Am`w ‘| hr AZwg§YmZ joÌ ‘| àdoe& Vision & Mission uEstablish scientific institution of the highest caliber where teaching and education are totally integrated with state-of-the-art research uMake learning of basic sciences exciting through excellent integrative teaching driven by curiosity and creativity uEntry into research at an early age through a flexible borderless curriculum and research projects Annual Report 2016-17 Correct Citation IISER Pune Annual Report 2016-17, Pune, India Published by Dr. K.N. Ganesh Director Indian Institute of Science Education and Research Pune Dr. Homi J. Bhabha Road Pashan, Pune 411 008, India Telephone: +91 20 2590 8001 Fax: +91 20 2025 1566 Website: www.iiserpune.ac.in Compiled and Edited by Dr. Shanti Kalipatnapu Dr. V.S. Rao Ms. Kranthi Thiyyagura Photo Courtesy IISER Pune Students and Staff © No part of this publication be reproduced without permission from the Director, IISER Pune at the above address Printed by United Multicolour Printers Pvt. -
Star Products from Commutative String Theory
hep-th/0108072 TIFR/TH/01-28 Star Products from Commutative String Theory Sunil Mukhi Tata Institute of Fundamental Research, Homi Bhabha Rd, Mumbai 400 005, India ABSTRACT A boundary-state computation is performed to obtain derivative corrections to the Chern-Simons coupling between a p-brane and the RR gauge potential Cp−3. We work to quadratic order in the gauge field strength F , but all orders in derivatives. In a certain limit, which requires the presence of a constant B-field background, it is found that these corrections neatly sum up into the product of (commutative) gauge fields. The result ∗2 is in agreement with a recent prediction using noncommutativity. arXiv:hep-th/0108072v1 10 Aug 2001 August 2001 Introduction In a recent paper[1] it was shown that the noncommutative formulation of open-string theory can actually give detailed information about ordinary commutative string theory. Once open Wilson lines are included in the noncommutative action, one has exact equality of commutative and noncommutative actions including all α′ corrections on both sides. As a result, a lot of information about α′ corrections on the commutative side is encoded in the lowest-order term (Chern-Simons or DBI) on the noncommutative side, and can be extracted explicitly. The predictions of Ref.[1] were tested against several boundary-state computations in commutative open-string theory performed in Ref.[2], and impressive agreement was found. The latter calculations were restricted to low-derivative orders, largely because the boundary-state computation becomes rather tedious when we go to high derivative order. However, in some specific cases, particularly when focusing on Chern-Simons couplings in the Seiberg-Witten limit[3], the predictions from noncommutativity in Ref.[1] are simple and elegant to all derivative orders as long as we work with weak field strengths (quadratic order in F ). -
Aspects of String Phenomenology
Aspects of string phenomenology I. Antoniadis CERN New Perspectives in String Theory: opening conference Galileo Galilei Institute, Florence, 6-8 April 2009 1 main questions and list of possibilities 2 phenomenology of low string scale 3 general issues of high string scale 4 string GUTs 5 framework of magnetized branes I. Antoniadis (CERN) 1 / 27 Are there low energy string predictions testable at LHC ? What can we hope from LHC on string phenomenology ? I. Antoniadis (CERN) 2 / 27 Very different answers depending mainly on the value of the string scale Ms - arbitrary parameter : Planck mass MP TeV −→ - physical motivations => favored energy regions: ∗ 18 MP 10 GeV Heterotic scale High : ≃ 16 ( MGUT 10 GeV Unification scale ≃ 11 2 Intermediate : around 10 GeV (M /MP TeV) s ∼ SUSY breaking, strong CP axion, see-saw scale Low : TeV (hierarchy problem) I. Antoniadis (CERN) 3 / 27 Low string scale =>experimentally testable framework - spectacular model independent predictions perturbative type I string setup - radical change of high energy physics at the TeV scale explicit model building is not necessary at this moment but unification has to be probably dropped particle accelerators - TeV extra dimensions => KK resonances of SM gauge bosons - Extra large submm dimensions => missing energy: gravity radiation - string physics and possible strong gravity effects : string Regge excitations · production of micro-black holes ? [9] · microgravity experiments - change of Newton’s law, new forces at short distances I. Antoniadis (CERN) 4 / 27 Universal -
Lecture Course: Introduction to String Phenomenology
Lecture Course: Introduction to String Phenomenology WS 2014/15 • Lecturer: Prof. Jan Louis II. Institut f¨ur Theoretische Physik der Universit¨at Hamburg Luruper Chaussee 149, 22761 Hamburg Office: Campus Bahrenfeld, Bldg. 2a, Rm 601 Phone: 8998-2261 E-mail: [email protected] home page: www.desy.de/∼jlouis/ • Date and Place: Fr, 11:00 – 12:30, SR 2/2a, Bldg. 2a, Campus Bahrenfeld supplementary classes are offered biweekly: Mon, 11:00 – 12:30, SR 2/2a, Bldg. 2a, Campus Bahrenfeld • Credit Points: Please contact me at the beginning if you need Credit Points for this course. • Recomended Textbooks [1 ] K. Becker, M. Becker and J. Schwarz, String Theory and M-Theory, Cam- bridge University Press, 2007. [2 ] R. Blumenhagen, D. L¨ust, S. Theisen, Basic Concepts of String Theory, Springer, 2013 [3 ] M. Dine, Supersymmetry and String Theory, Cambridge University Press, 2007. [4 ] D. Freedman and A. Van Proeyen, Supergravity, Cambridge University Press, 2012. [5 ] M. Green, J. Schwarz and E. Witten, Superstring Theory, Vol I& II, Cam- bridge University Press, 1987. [6 ] L. Ibanez and A. Uranga, String Theory and Particle Physics, Cambridge University Press, 2012. [7 ] J. Polchinski, String Theory, Vol I& II, Cambridge University Press, 1998. • Course syllabus (Fr, 11:00 – 12:30): 16.10: Introduction to string theory 24.10: The low energy effective action of string theory 31.10: Calabi-Yau compactifications 07.11: Calabi-Yau compactifications of the heterotic string 14.11: Supersymmtry breaking and gaugino condensation 21.11: D-branes in type II Calabi-Yau -
String Phenomenology and Model Building Gary Shiu
String Phenomenology and Model Building \New Trends in High Energy Physics and QCD" School and Workshop Natal, Brazil, October 2014 Gary Shiu Department of Physics, University of Wisconsin, Madison, WI 53706, USA 1 Abstract This is a set of 3 lectures (50 minutes each) prepared for the Natal School 2014. The aim of these lectures is to introduce the basic ideas of string theory and their applications to particle physics. These lectures hopefully serve to complement the lectures by Eduardo Ponton (BSM and Extra Dimensions), Marc Besanon (Phenomenology and experimental aspects of SUSY and searches for extra dimensions at the LHC), Dmitry Melnikov (Holography and Hadron Physics), and Jorge Noronha (AdS/CFT and applications to particle physics). These lectures are an update of my lectures at the TASI 2008 Summer School and the Trieste 2010 Spring School { both serve as useful references for this course. 2 1 Introduction This is the first of 3 lectures on \String Phenomenology and Model Building". My plan for these lectures is roughly as follows: Lecture I: String Phenomenology, with Branes • Lecture II: D-brane Model Building • Lecture III: Randall-Sundrum Scenario in String Theory: Warped Throats & their Field Theory • Duals Basic Theme: The basic theme of these lectures is to introduce some modern string theory tools useful for building models and scenarios of particle physics beyond the Standard Model. Of course, particle physics is not all what string phenomenology is about. String theory, being a quantum theory of gravity, is also a natural arena to address questions about early universe cosmology. However, string cosmology is a topic that warrants a set of lectures on its own. -
Schedule Titles and Zoom Links: Please Note That IST = UTC + 5:30
The Dual Mysteries of Gauge Theories and Gravity IIT Madras 2020 Schedule Titles and zoom links: Please note that IST = UTC + 5:30 Mon, Oct 19, Session 1: Chair: Suresh Govindarajan 09:00--9:30 IST Opening address by David Gross and Director’s welcome speech Zvi Bern 9:30- 10:25 IST Scattering Amplitudes as a Tool for Understanding Gravity Aninda Sinha 10:40--11:20 IST Rebooting the S-matrix bootstrap Mon, Oct 19, Session 2: Chair: Jyotirmoy Bhattacharyya Jerome Gauntlett 14:00-14:40 IST Spatially Modulated & Supersymmetric Mass Deformations of N=4 SYM Elias Kiritsis 14:55-15:35 IST Emergent gravity from hidden sectors and TT deformations Rene Meyer 15:50 -16:30 IST Strongly Correlated Dirac Materials, Electron Hydrodynamics & AdS/CFT Mon, Oct 19, Session 3: Chair: Bindusar Sahoo Chethan Krishnan 19:30-20:10 IST Cosmic Censorship of Trans-Planckian Field Ranges in Gravitational Collapse Timm Wrase 20:25 - 21:05 IST Misaligned SUSY in string theory Thomas van Riet 21:20 -22:00 IST A de Sitter landscape and Russel's teapot 1 The Dual Mysteries of Gauge Theories and Gravity Tue, Oct 20, Session 1: Chair: Nabamita Banerjee Rajesh Gopakumar 9:00 - 9:40 IST Branched Covers and Worldsheet Localisation in AdS_3 Gustavo Joaquin Turiaci 9:55- 10:35 IST The gravitational path integral near extremality Ayan Mukhopadhyay 10:50- 11:30 IST Analogue quantum black holes Tue, Oct 20, Session 2: Chair: Koushik Ray David Mateos 14:00-14:40 IST Holographic Dynamics near a Critical Point Shiraz Minwalla 14:55 - 15:35 IST Fermi seas from Bose condensates and a bosonic exclusion principle in matter Chern Simons theories. -
Arxiv:2010.07320V3 [Hep-Ph] 15 Jun 2021 Yecag Portal
Preprint typeset in JHEP style - HYPER VERSION UWThPh 2020-15 CCTP-2020-7 ITCP-IPP-2020/7 String (gravi)photons, “dark brane photons”, holography and the hypercharge portal P. Anastasopoulos1,∗ M. Bianchi2,† D. Consoli1,‡ E. Kiritsis3 1 Mathematical Physics Group, University of Vienna, Boltzmanngasse 5, 1090 Vienna, Austria 2 Dipartimento di Fisica, Universit`adi Roma “Tor Vergata” & I.N.F.N. Sezione di Roma “Tor Vergata”, Via della Ricerca Scientifica, 00133 Roma, Italy 3 Crete Center for Theoretical Physics, Institute for Theoretical and Computational Physics, Department of Physics, University of Crete, 70013, Heraklion, Greece and Universite de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France Abstract: The mixing of graviphotons and dark brane photons to the Standard Model hypercharge is analyzed in full generality, in weakly-coupled string theory. Both the direct mixing as well as effective terms that provide mixing after inclusion of arXiv:2010.07320v3 [hep-ph] 15 Jun 2021 SM corrections are estimated to lowest order. The results are compared with Effective Field Theory (EFT) couplings, originating in a hidden large-N theory coupled to the SM where the dark photons are composite. The string theory mixing terms are typically subleading compared with the generic EFT couplings. The case where the hidden theory is a holographic theory is also analyzed, providing also suppressed mixing terms to the SM hypercharge. Keywords: Emergent photon, dark photon, graviphoton, holography, mixing, hypercharge portal. ∗[email protected] †[email protected] ‡[email protected] Contents 1. Introduction 2 1.1 The field theory setup 5 1.2 Results and outlook 7 2. -
LHC String Phenomenology
IOP PUBLISHING JOURNAL OF PHYSICS G: NUCLEAR AND PARTICLE PHYSICS J. Phys. G: Nucl. Part. Phys. 34 (2007) 1993–2036 doi:10.1088/0954-3899/34/9/011 LHC string phenomenology Gordon L Kane, Piyush Kumar and Jing Shao Michigan Center for Theoretical Physics, University of Michigan, Ann Arbor, MI 48109, USA Received 5 June 2007 Published 31 July 2007 Online at stacks.iop.org/JPhysG/34/1993 Abstract We argue that it is possible to address the deeper LHC inverse problem, to gain insight into the underlying theory from LHC signatures of new physics. We propose a technique which may allow us to distinguish among, and favor or disfavor, various classes of underlying theoretical constructions using (assumed) new physics signals at the LHC. We think that this can be done with limited data (5–10 fb−1), and improved with more data. This is because of two reasons: (a) it is possible in many cases to reliably go from (semi)realistic microscopic string constructions to the space of experimental observables, say, LHC signatures, and (b) the patterns of signatures at the LHC are sensitive to the structure of the underlying theoretical constructions. We illustrate our approach by analyzing two promising classes of string compactifications along with six other string-motivated constructions. Even though these constructions are not complete, they illustrate the point we want to emphasize. We think that using this technique effectively over time can eventually help us to meaningfully connect experimental data to microscopic theory. (Some figures in this article are in colour only in the electronic version) Contents 1.