Massive Photon and Cosmology

Size: px
Start display at page:

Download "Massive Photon and Cosmology"

Transcription

1 Massive Photon and Cosmology Phillial Oh Sungkyunkwan University KIAS

2

3 Contents I. Introduction II. Massive QED and Cosmology III. Massive Dark Photon and Cosmology IV. Conslusions

4 Massive Photon: Introduction Maxwell-Proca Equations de Broglie: Photon mass would lead to a larger speed of violet light than that of the red one Schrödinger: Magnetic field of the Earth would be exponentially cut off at distances of the order of the photon Compton wave length λ γ 1/m γ The longitudinal photons do not manifest themselves in the black body radiation: Bass and Schrödinger

5 Massive Photon: Introduction Coester, Umezawa, Glauber, Stueckelberg, Boulware and Gilbert: massive QED smoothly goes over to QED. Amplitudes describing longitudinal modes suppressed as m γ 0, provided that electromagnetic current is conserved Deser: Longitudinal mode is transformed into a scalar mode decoupled from the current, remains coupled to gravitation Reviews on massive photon: Goldhaber and Nieto (2010) Reviews on Stuckelberg theory: Ruegg and Ruiz-Altaba (2003)

6 Massive QED and Cosmology Invariant Action L inv = 1 4 F μνf μν 1 2 m2 (A μ + 1 m μφ)(a μ + 1 m μ φ) + ˉψ(iγ μ μ m f )ψ + A μ ˉψγ μ ψ Invariant under A μ A μ μ Λ, φ φ + mλ, ψ e iλ ψ

7 Massive QED and Cosmology Invariant Action L inv = 1 4 F μνf μν 1 2 m2 (A μ + 1 m μφ)(a μ + 1 m μ φ) + ˉψ(iγ μ μ m f )ψ + A μ ˉψγ μ ψ Invariant under A μ A μ μ Λ, φ φ + mλ, ψ e iλ ψ Gauge fixed action L ξ = 1 4 F μνf μν 1 2 m2 A μ A μ 1 2 μφ μ φ 1 2 ξm2 φ 2 1 2ξ ( μa μ ) 2 + ˉψ(iγ μ μ m f )ψ + A μ ˉψγ μ ψ

8 Massive QED and Cosmology Propagator: A : [g μν (1 ξ)kμ k ν ] 1 k 2 + ξm 2 k 2 + m 2 φ : 1 k 2 ξm 2 m 0 exists, gives the gauge-fixed massless propagator Good high energy behavior, provided ξ 1 [g μν k 2 + m 2 + kμ k ν ] k μ k ν m 2 + m 2 (k 2 + ξm 2 ) ξ gives Proca propagator ξ dependent poles cancel each other: In the limit, ξ, they disappear

9 Massive QED and Cosmology Unitary and Renormalizable Dirac Monopole Infrared cutoff Indistinguishable from QED with photon mass limit

10 Massive QED and Cosmology

11 Massive QED and Cosmology

12 Massive QED and Cosmology

13 Massive QED and Cosmology

14 Massive QED and Cosmology

15 Massive QED and Cosmology

16 Summary Massive QED could be a viable model for dark energy Λ m 2 γ The vacuum A μ = f μ breaks Lorentz symmetry A small deviation from ΛCDM Non-minimal coupling of the Stuckelberg scalar field to gravity ξ-(in)dependence in quantum cosmology?

17 Dark Massive Vector and Cosmology S inv = { d 4 x 1 4 F μνf μν 1 4 C μνc μν 1 2 m2 (A μ + αs μ + 1 m μφ 1 )(A μ + αs μ + 1 m μ φ 1 ) 1 2 μ2 (S μ + 1 μ μφ 2 )(S μ + 1 } μ μφ 2 ) Invariant under A μ A μ μ Λ 1, S μ S μ μ Λ 2 φ 1 φ 1 + mλ 1 + αmλ 2, φ 2 φ 2 + μλ 2

18 Double Massive Vector and Cosmology Gauge fixing term: 1 2ξ 1 [ μ A μ + α μ S μ + ξ 1 mφ 1 + λ(a μ + αs μ )S μ ] 2 1 2ξ 2 ( μ S μ + ξ 2 μφ 2 ) 2 { S gf = d 4 x 1 4 F μνf μν 1 4 C μνc μν 1 2 m2 (A μ + αs μ )(A μ + αs μ ) 1 2 μ2 S μ S μ 1 2 μφ 1 μ φ ξ 1m 2 φ μφ 2 μ φ ξ 2μ 2 φ ξ 1 [( μ A μ + α μ S μ ) + λ(a μ + αs μ )S μ ] 2 1 2ξ 2 ( μ S μ ) 2 λmφ 1 (A μ + αs μ )S μ }

19 Dark Massive Vector and Cosmology Redefine: A μ + αs μ A μ, 1 + α 2 S μ S μ, α 1+α 2 χ S gf = { d 4 x 1 4 F μνf μν + χ 2 F μνc μν 1 4 C μνc μν 1 2 m2 A μ A μ 1 2 μ2 (1 χ 2 )S μ S μ 1 2 μφ 1 μ φ ξ 1m 2 φ μφ 2 μ φ ξ 2μ 2 φ [ μ A μ + λ ] 2 1 χ 2ξ 2 A μ S μ 1 1 2ξ 2 (1 χ 2 )( μ S μ ) 2 λ 1 χ 2 mφ 1 A μ S μ }

20 Dark Massive Vector and Cosmology S = d 4 x { R g F μνf μν + χ 2 F μνc μν 1 4 C μνc μν 1 2 m2 A μ A μ 1 2 μ2 S μ S μ + 1 2α [ μa μ + ξ (S μ A μ )] } 2β ( μs μ ) 2 Constant solution: G μν = κt μν A μ = f μ, S μ = h μ

21 Dark Massive Vector and Cosmology ds 2 = dt 2 + a(t) 2 dx i dx i T μν = F μα F ν α 1 4 g μνf αβ F αβ m 2 [ A μ A ν 1 2 g μνa α A α ] +C μα C ν α 1 4 g μνc αβ C αβ + μ 2 [ S μ S ν 1 2 g μνs α S α ] g μν 2α = Λg μν [ ( μ A μ ) + ξ (S α A α ) 2] 2 g μν 2β ( μs μ ) 2

22 Dark Massive Vector and Cosmology Λ = α [ 2ξ 2 m2 μ α β Proca limit: β h μ h μ = 3 4 ( m 2 μ 2 Λ = α 2ξ 2 m2 μ 2 ( αm 2 μ 2 ) [ 4ξ 2 ξ 4 3μ 2 1 ± ) )] (1 ξ2 αm h μh μ 2 ] 1 8ξ2 3μ 2 μ ξ2 Λ 4 3 αm2

23 Summary ρ Λ m 2 μ 2 Inclusion of Stuckelberg fields for cosmology Unified description of dark matter and dark energy ( ) M 2 4 Cosmic coincidence: ρ Λ EW M pl (Alkani-Hamed et al, 2000) Photon oscillations? EW theory with a massive photon (Ruegg and Ruiz-Altaba, 2003)

24

25

Cosmological perturbations in nonlinear massive gravity

Cosmological perturbations in nonlinear massive gravity Cosmological perturbations in nonlinear massive gravity A. Emir Gümrükçüoğlu IPMU, University of Tokyo AEG, C. Lin, S. Mukohyama, JCAP 11 (2011) 030 [arxiv:1109.3845] AEG, C. Lin, S. Mukohyama, To appear

More information

Cosmology in generalized Proca theories

Cosmology in generalized Proca theories 3-rd Korea-Japan workshop on dark energy, April, 2016 Cosmology in generalized Proca theories Shinji Tsujikawa (Tokyo University of Science) Collaboration with A.De Felice, L.Heisenberg, R.Kase, S.Mukohyama,

More information

Non-local infrared modifications of gravity and dark energy

Non-local infrared modifications of gravity and dark energy Non-local infrared modifications of gravity and dark energy Michele Maggiore Los Cabos, Jan. 2014 based on M. Jaccard, MM and E. Mitsou, 1305.3034, PR D88 (2013) MM, arxiv: 1307.3898 S. Foffa, MM and E.

More information

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 7: Lectures 13, 14.

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 7: Lectures 13, 14. As usual, these notes are intended for use by class participants only, and are not for circulation. Week 7: Lectures 13, 14 Majorana spinors March 15, 2012 So far, we have only considered massless, two-component

More information

Week 3: Renormalizable lagrangians and the Standard model lagrangian 1 Reading material from the books

Week 3: Renormalizable lagrangians and the Standard model lagrangian 1 Reading material from the books Week 3: Renormalizable lagrangians and the Standard model lagrangian 1 Reading material from the books Burgess-Moore, Chapter Weiberg, Chapter 5 Donoghue, Golowich, Holstein Chapter 1, 1 Free field Lagrangians

More information

A brief introduction to modified theories of gravity

A brief introduction to modified theories of gravity (Vinc)Enzo Vitagliano CENTRA, Lisboa May, 14th 2015 IV Amazonian Workshop on Black Holes and Analogue Models of Gravity Belém do Pará The General Theory of Relativity dynamics of the Universe behavior

More information

Gauge field localization on brane worlds

Gauge field localization on brane worlds Gauge field localization on brane worlds Rommel Guerrero and R. Omar Rodriguez Universidad Centroccidental Lisandro Alvarado - Venezuela Miami 2013 R. Guerrero UCLA) Gauge field localization December 2013

More information

752 Final. April 16, Fadeev Popov Ghosts and Non-Abelian Gauge Fields. Tim Wendler BYU Physics and Astronomy. The standard model Lagrangian

752 Final. April 16, Fadeev Popov Ghosts and Non-Abelian Gauge Fields. Tim Wendler BYU Physics and Astronomy. The standard model Lagrangian 752 Final April 16, 2010 Tim Wendler BYU Physics and Astronomy Fadeev Popov Ghosts and Non-Abelian Gauge Fields The standard model Lagrangian L SM = L Y M + L W D + L Y u + L H The rst term, the Yang Mills

More information

Quantum Field Theory I Examination questions will be composed from those below and from questions in the textbook and previous exams

Quantum Field Theory I Examination questions will be composed from those below and from questions in the textbook and previous exams Quantum Field Theory I Examination questions will be composed from those below and from questions in the textbook and previous exams III. Quantization of constrained systems and Maxwell s theory 1. The

More information

Two Fundamental Principles of Nature s Interactions

Two Fundamental Principles of Nature s Interactions Two Fundamental Principles of Nature s Interactions Tian Ma, Shouhong Wang Supported in part by NSF, ONR and Chinese NSF http://www.indiana.edu/ fluid I. Gravity and Principle of Interaction Dynamics PID)

More information

NTNU Trondheim, Institutt for fysikk

NTNU Trondheim, Institutt for fysikk NTNU Trondheim, Institutt for fysikk Examination for FY3464 Quantum Field Theory I Contact: Michael Kachelrieß, tel. 998971 Allowed tools: mathematical tables 1. Spin zero. Consider a real, scalar field

More information

Lecture 9: RR-sector and D-branes

Lecture 9: RR-sector and D-branes Lecture 9: RR-sector and D-branes José D. Edelstein University of Santiago de Compostela STRING THEORY Santiago de Compostela, March 6, 2013 José D. Edelstein (USC) Lecture 9: RR-sector and D-branes 6-mar-2013

More information

Aspects of massive gravity

Aspects of massive gravity Aspects of massive gravity Sébastien Renaux-Petel CNRS - IAP Paris Rencontres de Moriond, 22.03.2015 Motivations for modifying General Relativity in the infrared Present acceleration of the Universe: {z

More information

Thermal production of gravitinos

Thermal production of gravitinos Thermal production of gravitinos Slava Rychkov Scuola Normale Superiore & INFN, Pisa Università di Padova April 5 2007 hep-ph/0701104 with Alessandro Strumia (to appear in PhysRevD) Outline Gravitino in

More information

On the uniqueness of Einstein-Hilbert kinetic term (in massive (multi-)gravity)

On the uniqueness of Einstein-Hilbert kinetic term (in massive (multi-)gravity) On the uniqueness of Einstein-Hilbert kinetic term (in massive (multi-)gravity) Andrew J. Tolley Case Western Reserve University Based on: de Rham, Matas, Tolley, ``New Kinetic Terms for Massive Gravity

More information

Concistency of Massive Gravity LAVINIA HEISENBERG

Concistency of Massive Gravity LAVINIA HEISENBERG Universite de Gene ve, Gene ve Case Western Reserve University, Cleveland September 28th, University of Chicago in collaboration with C.de Rham, G.Gabadadze, D.Pirtskhalava What is Dark Energy? 3 options?

More information

Group Structure of Spontaneously Broken Gauge Theories

Group Structure of Spontaneously Broken Gauge Theories Group Structure of SpontaneouslyBroken Gauge Theories p. 1/25 Group Structure of Spontaneously Broken Gauge Theories Laura Daniel ldaniel@ucsc.edu Physics Department University of California, Santa Cruz

More information

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 8: Lectures 15, 16

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 8: Lectures 15, 16 As usual, these notes are intended for use by class participants only, and are not for circulation. Week 8: Lectures 15, 16 Masses for Vectors: the Higgs mechanism April 6, 2012 The momentum-space propagator

More information

Hunting New Physics in the Higgs Sector

Hunting New Physics in the Higgs Sector HS Hunting New Physics in the Higgs Sector SM Higgs Sector - Test of the Higgs Mechanism Oleg Kaikov KIT, Seminar WS 2015/16 Prof. Dr. M. Margarete Mühlleitner, Dr. Roger Wolf, Dr. Hendrik Mantler Advisor:

More information

Status of Hořava Gravity

Status of Hořava Gravity Status of Institut d Astrophysique de Paris based on DV & T. P. Sotiriou, PRD 85, 064003 (2012) [arxiv:1112.3385 [hep-th]] DV & T. P. Sotiriou, JPCS 453, 012022 (2013) [arxiv:1212.4402 [hep-th]] DV, arxiv:1502.06607

More information

Green s function of the Vector fields on DeSitter Background

Green s function of the Vector fields on DeSitter Background Green s function of the Vector fields on DeSitter Background Gaurav Narain The Institute for Fundamental Study (IF) March 10, 2015 Talk Based On Green s function of the Vector fields on DeSitter Background,

More information

Theory of Elementary Particles homework VIII (June 04)

Theory of Elementary Particles homework VIII (June 04) Theory of Elementary Particles homework VIII June 4) At the head of your report, please write your name, student ID number and a list of problems that you worked on in a report like II-1, II-3, IV- ).

More information

Dark energy and nonlocal gravity

Dark energy and nonlocal gravity Dark energy and nonlocal gravity Michele Maggiore Vacuum 2015, Barcelona based on Jaccard, MM, Mitsou, PRD 2013, 1305.3034 MM, PRD 2014, 1307.3898 Foffa, MM, Mitsou, PLB 2014, 1311.3421 Foffa, MM, Mitsou,

More information

The θ term. In particle physics and condensed matter physics. Anna Hallin. 601:SSP, Rutgers Anna Hallin The θ term 601:SSP, Rutgers / 18

The θ term. In particle physics and condensed matter physics. Anna Hallin. 601:SSP, Rutgers Anna Hallin The θ term 601:SSP, Rutgers / 18 The θ term In particle physics and condensed matter physics Anna Hallin 601:SSP, Rutgers 2017 Anna Hallin The θ term 601:SSP, Rutgers 2017 1 / 18 1 Preliminaries 2 The θ term in general 3 The θ term in

More information

Solitons and point particles

Solitons and point particles Solitons and point particles Martin Speight University of Leeds July 28, 2009 What are topological solitons? Smooth, spatially localized solutions of nonlinear relativistic classical field theories Stable;

More information

Scalar field dark matter and the Higgs field

Scalar field dark matter and the Higgs field Scalar field dark matter and the Higgs field Catarina M. Cosme in collaboration with João Rosa and Orfeu Bertolami Phys. Lett., B759:1-8, 2016 COSMO-17, Paris Diderot University, 29 August 2017 Outline

More information

Physics 582, Problem Set 1 Solutions

Physics 582, Problem Set 1 Solutions Physics 582, Problem Set 1 Solutions TAs: Hart Goldman and Ramanjit Sohal Fall 2018 1. THE DIRAC EQUATION [20 PTS] Consider a four-component fermion Ψ(x) in 3+1D, L[ Ψ, Ψ] = Ψ(i/ m)ψ, (1.1) where we use

More information

Solution set #7 Physics 571 Tuesday 3/17/2014. p 1. p 2. Figure 1: Muon production (e + e µ + µ ) γ ν /p 2

Solution set #7 Physics 571 Tuesday 3/17/2014. p 1. p 2. Figure 1: Muon production (e + e µ + µ ) γ ν /p 2 Solution set #7 Physics 571 Tuesday 3/17/2014 μ 1. The amplitude is Figure 1: Muon production ( e µ + µ ) it = ie2 s (v 2γ µ u 1 )(u 1 γ µ v 2 ), (1) so the spin averaged squared amplitude is T 2 = e4

More information

arxiv:quant-ph/ v5 1 Aug 2005

arxiv:quant-ph/ v5 1 Aug 2005 Constraints of the Dynamic Equations and Lagrangian required by Superposition of Field X. Sun a, Z. Yang b,c a Institute of High Energy Physics, Beijing 100039, China a Graduate University of the Chinese

More information

QFT Dimensional Analysis

QFT Dimensional Analysis QFT Dimensional Analysis In the h = c = 1 units, all quantities are measured in units of energy to some power. For example m = p µ = E +1 while x µ = E 1 where m stands for the dimensionality of the mass

More information

Quantum Field Theory. and the Standard Model. !H Cambridge UNIVERSITY PRESS MATTHEW D. SCHWARTZ. Harvard University

Quantum Field Theory. and the Standard Model. !H Cambridge UNIVERSITY PRESS MATTHEW D. SCHWARTZ. Harvard University Quantum Field Theory and the Standard Model MATTHEW D. Harvard University SCHWARTZ!H Cambridge UNIVERSITY PRESS t Contents v Preface page xv Part I Field theory 1 1 Microscopic theory of radiation 3 1.1

More information

Renormalization in Lorentz-violating field theory: external states

Renormalization in Lorentz-violating field theory: external states Renormalization in Lorentz-violating field theory: external states Robertus Potting CENTRA and Physics Department Faculdade de Ciências e Tecnologia Universidade do Algarve Faro, Portugal SME2015 Summer

More information

Gauge coupling unification without leptoquarks Mikhail Shaposhnikov

Gauge coupling unification without leptoquarks Mikhail Shaposhnikov Gauge coupling unification without leptoquarks Mikhail Shaposhnikov March 9, 2017 Work with Georgios Karananas, 1703.02964 Heidelberg, March 9, 2017 p. 1 Outline Motivation Gauge coupling unification without

More information

Some Quantum Aspects of D=3 Space-Time Massive Gravity.

Some Quantum Aspects of D=3 Space-Time Massive Gravity. Some Quantum Aspects of D=3 Space-Time Massive Gravity. arxiv:gr-qc/96049v 0 Nov 996 Carlos Pinheiro, Universidade Federal do Espírito Santo, Departamento de Física, Vitória-ES, Brazil, Gentil O. Pires,

More information

A Brief Introduction to Relativistic Quantum Mechanics

A Brief Introduction to Relativistic Quantum Mechanics A Brief Introduction to Relativistic Quantum Mechanics Hsin-Chia Cheng, U.C. Davis 1 Introduction In Physics 215AB, you learned non-relativistic quantum mechanics, e.g., Schrödinger equation, E = p2 2m

More information

XIII. The Very Early Universe and Inflation. ASTR378 Cosmology : XIII. The Very Early Universe and Inflation 171

XIII. The Very Early Universe and Inflation. ASTR378 Cosmology : XIII. The Very Early Universe and Inflation 171 XIII. The Very Early Universe and Inflation ASTR378 Cosmology : XIII. The Very Early Universe and Inflation 171 Problems with the Big Bang The Flatness Problem The Horizon Problem The Monopole (Relic Particle)

More information

Robustness of GR, Attempts to Modify Gravity

Robustness of GR, Attempts to Modify Gravity Robustness of GR, Attempts to Modify Gravity Lecturer: Prof. Nima Arkani-Hamed Transcriber: Alexander Chen August 7, 2011 Contents 1 Lecture 1 2 2 Lecture 2 6 3 Lecture 3 10 4 Lecture 4 14 1 Attempts to

More information

Quantum Field Theory 2 nd Edition

Quantum Field Theory 2 nd Edition Quantum Field Theory 2 nd Edition FRANZ MANDL and GRAHAM SHAW School of Physics & Astromony, The University of Manchester, Manchester, UK WILEY A John Wiley and Sons, Ltd., Publication Contents Preface

More information

Quantum Field Theory II

Quantum Field Theory II Quantum Field Theory II T. Nguyen PHY 391 Independent Study Term Paper Prof. S.G. Rajeev University of Rochester April 2, 218 1 Introduction The purpose of this independent study is to familiarize ourselves

More information

On the QCD of a Massive Vector Field in the Adjoint Representation

On the QCD of a Massive Vector Field in the Adjoint Representation On the QCD of a Massive Vector Field in the Adjoint Representation Alfonso R. Zerwekh UTFSM December 9, 2012 Outlook 1 Motivation 2 A Gauge Theory for a Massive Vector Field Local Symmetry 3 Quantum Theory:

More information

Part I. Many-Body Systems and Classical Field Theory

Part I. Many-Body Systems and Classical Field Theory Part I. Many-Body Systems and Classical Field Theory 1. Classical and Quantum Mechanics of Particle Systems 3 1.1 Introduction. 3 1.2 Classical Mechanics of Mass Points 4 1.3 Quantum Mechanics: The Harmonic

More information

HIGHER SPIN PROBLEM IN FIELD THEORY

HIGHER SPIN PROBLEM IN FIELD THEORY HIGHER SPIN PROBLEM IN FIELD THEORY I.L. Buchbinder Tomsk I.L. Buchbinder (Tomsk) HIGHER SPIN PROBLEM IN FIELD THEORY Wroclaw, April, 2011 1 / 27 Aims Brief non-expert non-technical review of some old

More information

Quantum discontinuity between zero and infinitesimal graviton mass with a Λ term. Abstract

Quantum discontinuity between zero and infinitesimal graviton mass with a Λ term. Abstract MCTP-01-06 hep-th/010093 Quantum discontinuity between zero and infinitesimal graviton mass with a Λ term F. A. Dilkes, M. J. Duff, James T. Liu and H. Sati Michigan Center for Theoretical Physics Randall

More information

arxiv: v2 [hep-th] 28 Mar 2013

arxiv: v2 [hep-th] 28 Mar 2013 Preprint typeset in JHEP style - HYPER VERSION arxiv:111.0441v [hep-th] 8 Mar 013 A longitudinal gauge degree of freedom and the Pais Uhlenbeck field Jose Beltrán Jiménez a,b, Enea Di Dio b and Ruth Durrer

More information

NTNU Trondheim, Institutt for fysikk

NTNU Trondheim, Institutt for fysikk NTNU Trondheim, Institutt for fysikk Examination for FY3464 Quantum Field Theory I Contact: Michael Kachelrieß, tel. 99890701 Allowed tools: mathematical tables 1. Procca equation. 5 points A massive spin-1

More information

NTNU Trondheim, Institutt for fysikk

NTNU Trondheim, Institutt for fysikk NTNU Trondheim, Institutt for fysikk Examination for FY3464 Quantum Field Theory I Contact: Michael Kachelrieß, tel. 99890701 Allowed tools: mathematical tables Some formulas can be found on p.2. 1. Concepts.

More information

Origin of the Photon Mass and ECE Spin Field in the Spin Connection of Space-Time

Origin of the Photon Mass and ECE Spin Field in the Spin Connection of Space-Time 12 Origin of the Photon Mass and ECE Spin Field in the Spin Connection of Space-Time by Myron W. Evans, Alpha Institute for Advanced Study, Civil List Scientist. (emyrone@aol.com and www.aias.us) Abstract

More information

New Model of massive spin-2 particle

New Model of massive spin-2 particle New Model of massive spin-2 particle Based on Phys.Rev. D90 (2014) 043006, Y.O, S. Akagi, S. Nojiri Phys.Rev. D90 (2014) 123013, S. Akagi, Y.O, S. Nojiri Yuichi Ohara QG lab. Nagoya univ. Introduction

More information

The Extended Gauge Transformations

The Extended Gauge Transformations Progress In Electromagnetics Research M, Vol. 39, 07 4, 204 The Extended Gauge Transformations Arbab I. Arbab, 2, * Abstract In this work, new extended gauge transformations involving current fields are

More information

arxiv:quant-ph/ v1 16 Jun 2005

arxiv:quant-ph/ v1 16 Jun 2005 Black-body radiation in extra dimensions Haavard Alnes, Finn Ravndal 2 and Ingunn Kathrine Wehus 3 Institute of Physics, University of Oslo, N-036 Oslo, Norway. arxiv:quant-ph/05063 v 6 Jun 2005 Abstract

More information

NTNU Trondheim, Institutt for fysikk

NTNU Trondheim, Institutt for fysikk FY3464 Quantum Field Theory II Final exam 0..0 NTNU Trondheim, Institutt for fysikk Examination for FY3464 Quantum Field Theory II Contact: Kåre Olaussen, tel. 735 9365/4543770 Allowed tools: mathematical

More information

LOCALIZATION OF FIELDS ON A BRANE IN SIX DIMENSIONS.

LOCALIZATION OF FIELDS ON A BRANE IN SIX DIMENSIONS. LOCALIZATION OF FIELDS ON A BRANE IN SIX DIMENSIONS Merab Gogberashvili a and Paul Midodashvili b a Andronikashvili Institute of Physics, 6 Tamarashvili Str., Tbilisi 3877, Georgia E-mail: gogber@hotmail.com

More information

General Relativity Lecture 20

General Relativity Lecture 20 General Relativity Lecture 20 1 General relativity General relativity is the classical (not quantum mechanical) theory of gravitation. As the gravitational interaction is a result of the structure of space-time,

More information

QED and the Standard Model Autumn 2014

QED and the Standard Model Autumn 2014 QED and the Standard Model Autumn 2014 Joel Goldstein University of Bristol Joel.Goldstein@bristol.ac.uk These lectures are designed to give an introduction to the gauge theories of the standard model

More information

2P + E = 3V 3 + 4V 4 (S.2) D = 4 E

2P + E = 3V 3 + 4V 4 (S.2) D = 4 E PHY 396 L. Solutions for homework set #19. Problem 1a): Let us start with the superficial degree of divergence. Scalar QED is a purely bosonic theory where all propagators behave as 1/q at large momenta.

More information

Special Relativity from Soft Gravitons

Special Relativity from Soft Gravitons Special Relativity from Soft Gravitons Mark Hertzberg, Tufts University CosPA, December 14, 2017 with McCullen Sandora, PRD 96 084048 (1704.05071) Can the laws of special relativity be violated in principle?

More information

Lecturer: Bengt E W Nilsson

Lecturer: Bengt E W Nilsson 9 3 19 Lecturer: Bengt E W Nilsson Last time: Relativistic physics in any dimension. Light-cone coordinates, light-cone stuff. Extra dimensions compact extra dimensions (here we talked about fundamental

More information

Non-Abelian tensor multiplet in four dimensions

Non-Abelian tensor multiplet in four dimensions PASCOS 2012 18th nternational Symposium on Particles Strings and Cosmology OP Publishing Non-Abelian tensor multiplet in four dimensions Hitoshi Nishino and Subhash Rajpoot, Department of Physics and Astronomy,

More information

Coupled Dark Energy and Dark Matter from dilatation symmetry

Coupled Dark Energy and Dark Matter from dilatation symmetry Coupled Dark Energy and Dark Matter from dilatation symmetry Cosmological Constant - Einstein - Constant λ compatible with all symmetries Constant λ compatible with all observations No time variation in

More information

Maxwell s equations. electric field charge density. current density

Maxwell s equations. electric field charge density. current density Maxwell s equations based on S-54 Our next task is to find a quantum field theory description of spin-1 particles, e.g. photons. Classical electrodynamics is governed by Maxwell s equations: electric field

More information

The Role Of Magnetic Monopoles In Quark Confinement (Field Decomposition Approach)

The Role Of Magnetic Monopoles In Quark Confinement (Field Decomposition Approach) The Role Of Magnetic Monopoles In Quark Confinement (Field Decomposition Approach) IPM school and workshop on recent developments in Particle Physics (IPP11) 2011, Tehran, Iran Sedigheh Deldar, University

More information

(a) (b) Notes 6: The Higgs. Spontaneous symmetry breaking

(a) (b) Notes 6: The Higgs. Spontaneous symmetry breaking Notes 6: The Higgs This is a middle difficulty explaination. The text books are either much more detailed or simpler. This is a useful guide for those who want to look at HM, Griffiths or Burcham and Jobes

More information

Cosmology (Cont.) Lecture 19

Cosmology (Cont.) Lecture 19 Cosmology (Cont.) Lecture 19 1 General relativity General relativity is the classical theory of gravitation, and as the gravitational interaction is due to the structure of space-time, the mathematical

More information

Versatility of the Abelian Higgs Model

Versatility of the Abelian Higgs Model Versatility of the Abelian Higgs Model Ernest Ma Physics and Astronomy Department University of California Riverside, CA 92521, USA Versatility of the Abelian Higgs Model (2013) back to start 1 Contents

More information

arxiv:gr-qc/ v3 10 Nov 1994

arxiv:gr-qc/ v3 10 Nov 1994 1 Nonsymmetric Gravitational Theory J. W. Moffat Department of Physics University of Toronto Toronto, Ontario M5S 1A7 Canada arxiv:gr-qc/9411006v3 10 Nov 1994 Abstract A new version of nonsymmetric gravitational

More information

Scale symmetry a link from quantum gravity to cosmology

Scale symmetry a link from quantum gravity to cosmology Scale symmetry a link from quantum gravity to cosmology scale symmetry fluctuations induce running couplings violation of scale symmetry well known in QCD or standard model Fixed Points Quantum scale symmetry

More information

Cavendish Laboratory Institute of Astronomy

Cavendish Laboratory Institute of Astronomy Andy Parker George Efstathiou Cavendish Laboratory Institute of Astronomy This is a 16 lecture Part III Minor Option. Tuesdays and Thursdays 10 am Textbooks: Perkins Particle Astrophysics Bergstrom and

More information

2.4 Parity transformation

2.4 Parity transformation 2.4 Parity transformation An extremely simple group is one that has only two elements: {e, P }. Obviously, P 1 = P, so P 2 = e, with e represented by the unit n n matrix in an n- dimensional representation.

More information

arxiv: v3 [hep-th] 30 May 2018

arxiv: v3 [hep-th] 30 May 2018 arxiv:1010.0246v3 [hep-th] 30 May 2018 Graviton mass and cosmological constant: a toy model Dimitrios Metaxas Department of Physics, National Technical University of Athens, Zografou Campus, 15780 Athens,

More information

Superfluids and the Cosmological Constant Problem

Superfluids and the Cosmological Constant Problem Superfluids and the Cosmological Constant Problem Adam R. Solomon Carnegie Mellon University With Justin Khoury & Jeremy Sakstein (UPenn) arxiv:1805.05937 (JCAP) Outline 1. Intro to the cosmological constant

More information

A model of the basic interactions between elementary particles is defined by the following three ingredients:

A model of the basic interactions between elementary particles is defined by the following three ingredients: I. THE STANDARD MODEL A model of the basic interactions between elementary particles is defined by the following three ingredients:. The symmetries of the Lagrangian; 2. The representations of fermions

More information

SM, EWSB & Higgs. MITP Summer School 2017 Joint Challenges for Cosmology and Colliders. Homework & Exercises

SM, EWSB & Higgs. MITP Summer School 2017 Joint Challenges for Cosmology and Colliders. Homework & Exercises SM, EWSB & Higgs MITP Summer School 017 Joint Challenges for Cosmology and Colliders Homework & Exercises Ch!"ophe Grojean Ch!"ophe Grojean DESY (Hamburg) Humboldt University (Berlin) ( christophe.grojean@desy.de

More information

Non-relativistic Limit of Dirac Equations in Gravitational Field and Quantum Effects of Gravity

Non-relativistic Limit of Dirac Equations in Gravitational Field and Quantum Effects of Gravity Commun. Theor. Phys. Beijing, China) 45 26) pp. 452 456 c International Academic Publishers Vol. 45, No. 3, March 15, 26 Non-relativistic Limit of Dirac Equations in Gravitational Field and Quantum Effects

More information

Anisotropic to Isotropic Phase Transitions in the Early Universe

Anisotropic to Isotropic Phase Transitions in the Early Universe Anisotropic to Isotropic Phase Transitions in the Early Universe Muhammad Adeel Ajaib Department of Physics and Astronomy University of Delaware, Newark, Delaware 19716. We attempt to develop a minimal

More information

GRAVITATION F10. Lecture Maxwell s Equations in Curved Space-Time 1.1. Recall that Maxwell equations in Lorentz covariant form are.

GRAVITATION F10. Lecture Maxwell s Equations in Curved Space-Time 1.1. Recall that Maxwell equations in Lorentz covariant form are. GRAVITATION F0 S. G. RAJEEV Lecture. Maxwell s Equations in Curved Space-Time.. Recall that Maxwell equations in Lorentz covariant form are. µ F µν = j ν, F µν = µ A ν ν A µ... They follow from the variational

More information

Higgs Boson Phenomenology Lecture I

Higgs Boson Phenomenology Lecture I iggs Boson Phenomenology Lecture I Laura Reina TASI 2011, CU-Boulder, June 2011 Outline of Lecture I Understanding the Electroweak Symmetry Breaking as a first step towards a more fundamental theory of

More information

The Dirac Equation. Topic 3 Spinors, Fermion Fields, Dirac Fields Lecture 13

The Dirac Equation. Topic 3 Spinors, Fermion Fields, Dirac Fields Lecture 13 The Dirac Equation Dirac s discovery of a relativistic wave equation for the electron was published in 1928 soon after the concept of intrisic spin angular momentum was proposed by Goudsmit and Uhlenbeck

More information

Review and Preview. We are testing QED beyond the leading order of perturbation theory. We encounter... IR divergences from soft photons;

Review and Preview. We are testing QED beyond the leading order of perturbation theory. We encounter... IR divergences from soft photons; Chapter 9 : Radiative Corrections 9.1 Second order corrections of QED 9. Photon self energy 9.3 Electron self energy 9.4 External line renormalization 9.5 Vertex modification 9.6 Applications 9.7 Infrared

More information

6. QED. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 6. QED 1

6. QED. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 6. QED 1 6. QED Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 6. QED 1 In this section... Gauge invariance Allowed vertices + examples Scattering Experimental tests Running of alpha Dr. Tina Potter

More information

General Relativity and Cosmology Mock exam

General Relativity and Cosmology Mock exam Physikalisches Institut Mock Exam Universität Bonn 29. June 2011 Theoretische Physik SS 2011 General Relativity and Cosmology Mock exam Priv. Doz. Dr. S. Förste Exercise 1: Overview Give short answers

More information

HOMEWORK 10. Applications: special relativity, Newtonian limit, gravitational waves, gravitational lensing, cosmology, 1 black holes

HOMEWORK 10. Applications: special relativity, Newtonian limit, gravitational waves, gravitational lensing, cosmology, 1 black holes General Relativity 8.96 (Petters, spring 003) HOMEWORK 10. Applications: special relativity, Newtonian limit, gravitational waves, gravitational lensing, cosmology, 1 black holes 1. Special Relativity

More information

Particle Physics I Lecture Exam Question Sheet

Particle Physics I Lecture Exam Question Sheet Particle Physics I Lecture Exam Question Sheet Five out of these 16 questions will be given to you at the beginning of the exam. (1) (a) Which are the different fundamental interactions that exist in Nature?

More information

Introduction to String Theory ETH Zurich, HS11. 9 String Backgrounds

Introduction to String Theory ETH Zurich, HS11. 9 String Backgrounds Introduction to String Theory ETH Zurich, HS11 Chapter 9 Prof. N. Beisert 9 String Backgrounds Have seen that string spectrum contains graviton. Graviton interacts according to laws of General Relativity.

More information

3 Quantization of the Dirac equation

3 Quantization of the Dirac equation 3 Quantization of the Dirac equation 3.1 Identical particles As is well known, quantum mechanics implies that no measurement can be performed to distinguish particles in the same quantum state. Elementary

More information

Finite-temperature Field Theory

Finite-temperature Field Theory Finite-temperature Field Theory Aleksi Vuorinen CERN Initial Conditions in Heavy Ion Collisions Goa, India, September 2008 Outline Further tools for equilibrium thermodynamics Gauge symmetry Faddeev-Popov

More information

Introduction to Orientifolds.

Introduction to Orientifolds. Introduction to Orientifolds http://www.physto.se/~mberg Overview Orientability in Quantum Field Theory: spinors S R(2π) ψ = ψ Orientability in Quantum Field Theory: spinors (S R(2π) ) 2 ψ =+ ψ S R(2π)

More information

Problem 1(a): As discussed in class, Euler Lagrange equations for charged fields can be written in a manifestly covariant form as L (D µ φ) L

Problem 1(a): As discussed in class, Euler Lagrange equations for charged fields can be written in a manifestly covariant form as L (D µ φ) L PHY 396 K. Solutions for problem set #. Problem 1a: As discussed in class, Euler Lagrange equations for charged fields can be written in a manifestly covariant form as D µ D µ φ φ = 0. S.1 In particularly,

More information

3P1a Quantum Field Theory: Example Sheet 1 Michaelmas 2016

3P1a Quantum Field Theory: Example Sheet 1 Michaelmas 2016 3P1a Quantum Field Theory: Example Sheet 1 Michaelmas 016 Corrections and suggestions should be emailed to B.C.Allanach@damtp.cam.ac.uk. Starred questions may be handed in to your supervisor for feedback

More information

Note 1: Some Fundamental Mathematical Properties of the Tetrad.

Note 1: Some Fundamental Mathematical Properties of the Tetrad. Note 1: Some Fundamental Mathematical Properties of the Tetrad. As discussed by Carroll on page 88 of the 1997 notes to his book Spacetime and Geometry: an Introduction to General Relativity (Addison-Wesley,

More information

Introduction to gauge theory

Introduction to gauge theory Introduction to gauge theory 2008 High energy lecture 1 장상현 연세대학교 September 24, 2008 장상현 ( 연세대학교 ) Introduction to gauge theory September 24, 2008 1 / 72 Table of Contents 1 Introduction 2 Dirac equation

More information

Relativistic Quantum Mechanics

Relativistic Quantum Mechanics Physics 342 Lecture 34 Relativistic Quantum Mechanics Lecture 34 Physics 342 Quantum Mechanics I Wednesday, April 30th, 2008 We know that the Schrödinger equation logically replaces Newton s second law

More information

Quantum field theory on curved Spacetime

Quantum field theory on curved Spacetime Quantum field theory on curved Spacetime YOUSSEF Ahmed Director : J. Iliopoulos LPTENS Paris Laboratoire de physique théorique de l école normale supérieure Why QFT on curved In its usual formulation QFT

More information

Large Extra Dimensions and the Hierarchy Problem

Large Extra Dimensions and the Hierarchy Problem Large Extra Dimensions and the Hierarchy Problem The Hierarchy Problem - At Planck energies (M P L 10 19 GeV ) all four forces have the same strength. -At the Electroweak scale (M EW 1T ev ) the four forces

More information

MSci EXAMINATION. Date: XX th May, Time: 14:30-17:00

MSci EXAMINATION. Date: XX th May, Time: 14:30-17:00 MSci EXAMINATION PHY-415 (MSci 4242 Relativistic Waves and Quantum Fields Time Allowed: 2 hours 30 minutes Date: XX th May, 2010 Time: 14:30-17:00 Instructions: Answer THREE QUESTIONS only. Each question

More information

9 Quantum Field Theory for Children

9 Quantum Field Theory for Children 101 9 Quantum Field Theory for Children The theories (known and hypothetical) needed to describe the (very) early universe are quantum field theories (QFT). The fundamental entities of these theories are

More information

Maxwell s equations. based on S-54. electric field charge density. current density

Maxwell s equations. based on S-54. electric field charge density. current density Maxwell s equations based on S-54 Our next task is to find a quantum field theory description of spin-1 particles, e.g. photons. Classical electrodynamics is governed by Maxwell s equations: electric field

More information

be stationary under variations in A, we obtain Maxwell s equations in the form ν J ν = 0. (7.5)

be stationary under variations in A, we obtain Maxwell s equations in the form ν J ν = 0. (7.5) Chapter 7 A Synopsis of QED We will here sketch the outlines of quantum electrodynamics, the theory of electrons and photons, and indicate how a calculation of an important physical quantity can be carried

More information

RADIATIVE CORRECTIONS TO THE STEFAN-BOLTZMANN LAW. FINN RAVNDAL a. Institute of Physics, University of Oslo, N-0316 Oslo, Norway

RADIATIVE CORRECTIONS TO THE STEFAN-BOLTZMANN LAW. FINN RAVNDAL a. Institute of Physics, University of Oslo, N-0316 Oslo, Norway RADIATIVE CORRECTIONS TO THE STEFAN-BOLTZMANN LAW FINN RAVNDAL a Institute of Physics, University of Oslo, N-0316 Oslo, Norway Abstract Photons in blackbody radiation have non-zero interactions due to

More information

Curiosités géométriques et physique de l'univers

Curiosités géométriques et physique de l'univers Curiosités géométriques et physique de l'univers MidiSciences, Grenoble, 05/2010 String Theory & Invisible Dimensions Ecole Normale Supérieure de Lyon plan fundamental interactions standard model vs. general

More information

Beta functions in quantum electrodynamics

Beta functions in quantum electrodynamics Beta functions in quantum electrodynamics based on S-66 Let s calculate the beta function in QED: the dictionary: Note! following the usual procedure: we find: or equivalently: For a theory with N Dirac

More information