Special Relativity from Soft Gravitons

Size: px
Start display at page:

Download "Special Relativity from Soft Gravitons"

Transcription

1 Special Relativity from Soft Gravitons Mark Hertzberg, Tufts University CosPA, December 14, 2017 with McCullen Sandora, PRD ( )

2 Can the laws of special relativity be violated in principle? Are they exact?

3 Special Relativity in QED QED Spin 1 Photons Coupled to Spin 1/2 Electrons

4 Special Relativity in QED QED L = 1 4 F µ µ F + (i µ D µ m)

5 Special Relativity in QED QED L = 1 4 F µ µ F + (i µ D µ m) { µ, } =2 µ µ = c c c 2 1 C A E 2 q = c 2 q 2 E 2 = c 2 p 2 + m 2 c 4

6 Violate Special Relativity in QED QED L = 1 4 F µ µ F + (i µ e D µ m) { µ e, e } =2 e µ µ = c c c 2 1 C A µ e = c 2 e c 2 e c 2 e 1 C A E 2 q = c 2 q 2 E 2 = c 2 e p 2 + m 2 c 4 e

7 Violate Special Relativity in QED c e 6= c Cherenkov radiation in vacuum (Related processes constrain faster than light neutrinos) (Cohen, Glashow)

8 Violate Special Relativity in Standard Model Colladay and Kostelecky 1998 Coleman and Glashow Lorentz violating couplings (CPT even)

9 Violate Special Relativity in Standard Model - Local - Causal - Unitary - Renormalizable (EFT) - No vacuum instability - No gauge anomalies - Same # degrees of freedom - Obeys laws of thermodynamics - (Gauge invariant) -

10 More Violations of Special Relativity L = 1 4 F µ µ F + X n n(i µ nd µ m n ) n µ! µ ( ) i nd i! f n ( i nd i ) E 2 q = K 1 (q) E 2 n = K n (p n ) K 1 (q) =c 2 q 2 + d q K n (p) =c 2 n p 2 + m 2 nc 4 n + d n p

11 In this talk Principles: Locality (and Rot. + Trans. Invariance)

12 In this talk Principles: Locality (and Rot. + Trans. Invariance) Apply to Spin 2

13 In this talk Principles: Locality (and Rot. + Trans. Invariance) Apply to Spin 2 Special Relativity E 2 = p 2 c 2 + m 2 c 4

14 Particle Spin Rotation invariance organizes particles by spin Spin s =0, 1 2, 1, 3 2, 2,...

15 Particle Spin Rotation invariance organizes particles by spin Spin s =0, 1 2, 1, 3 2, 2,... Massive s z = s, s +1,...,s 1,s Massless h = ±s

16 Particle Spin Rotation invariance organizes particles by spin Spin s =0, 1 2, 1, 3 2, 2,... Massive s z = s, s +1,...,s 1,s Massless h = ±s

17 Massless Spin 1 and Spin 2 State: hx i = (q) e iq x

18 Massless Spin 1 and Spin 2 State: hx i = (q) e iq x Spin 1 i, i q i =0 (Transverse)

19 Massless Spin 1 and Spin 2 State: hx i = (q) e iq x Spin 1 i, i q i =0 (Transverse) Spin 2 ij, ij q i =0, ii =0 (TT) Manifest rotation invariance (no need for gauge invariance for manifest symmetry)

20 Propagator for Spin 1 and Spin 2 Spin 1 i j G ij = E 2 ij q i q j q 2 K 1 (q)

21 Propagator for Spin 1 and Spin 2 Spin 1 i j G ij = E 2 ij q i q j q 2 K 1 (q) Spin 2 ij kl G ijkl = ij q i q j q 2 E 2 kl q k q k q 2 K 2 (q) (j $ k, l)

22 Action from Tree-Exchange S = Z d 4 q (2 ) 4 " J i (q) q i q j ij q 2 J j! 2 (q)+ (q) (q) K 1 (q) L 1 (q) # Dynamical Non-dynamical i spin 1 j spin 0 Magnetic+Electric (Non-Local) Electric [Coulombic] (Non-Local)

23 Locality Principle: No instantaneous action at a distance

24 Locality Principle: No instantaneous action at a distance Turn on sources at t=0 d p dt p x n(t = 0) = 0 (p 2) Acceleration Time

25 Locality S = Z d 4 q (2 ) 4 " J i (q) q i q j ij q 2 J j! 2 (q)+ (q) (q) K 1 (q) L 1 (q) # Constitutive relation q i J i (q) =M 1 (q)! (q)

26 Locality S = Z d 4 q (2 ) 4 " J i (q) q i q j ij q 2 J j! 2 (q)+ (q) (q) K 1 (q) L 1 (q) # Constitutive relation q i J i (q) =M 1 (q)! (q) d p dt p x n(t = 0) = 0 (p 2) =) Z d 4 q S = (2 ) 4 " X Poly p ( q 2 # )! p p

27 Locality S = Z d 4 q (2 ) 4 " J i (q) q i q j ij q 2 J j! 2 (q)+ (q) (q) K 1 (q) L 1 (q) # Constitutive relation q i J i (q) =M 1 (q)! (q) K 1 (q) =c 2 q 2 + q 4 P a ( q 2 ) L 1 (q) 1 = 1 q 2 + P b( q 2 ) (locality) M 1 (q) 2 =1+ q 2 P c ( q 2 )

28 Local Lagrangian for Photon Fields Field: ( i (q)â q + i (q)â q)/ p 2E q! A i (x) L = 1 2 Ȧ r A K1( ) r A + A J L 1( ) + Ȧ M 1( )r + (r A) 2 Not gauge invariant

29 Local Lagrangian for Photon Fields Field: ( i (q)â q + i (q)â q)/ p 2E q! A i (x) L = 1 2 Ȧ r A K1( ) r A + A J L 1( ) + Ȧ M 1( )r + (r A) 2 Not gauge invariant K 1 = c 2 + O( 2 ), L 1 = + O( 2 ), M 1 =1+O( )

30 Soft Gauge Invariance for Spin 1 E B L = 1 2 Ȧ + r 2 c 2 2 r A 2 + A J + O( 2 ) 4-component vector: A µ (, A) Locality =) A µ A µ µ (slowly varying ) µ (q)! µ (q)+q µ (soft )

31 Soft Gauge Invariance for Spin 2

32 Soft Gauge Invariance for Spin 2

33 Soft Gauge Invariance for Spin 2 G ijkl = ij q i q j q 2 E 2 kl q k q k q 2 K 2 (q) (j $ k, l) 2 types of non-localities Add non-dynamical h 00 (Newton) h 0i

34 Soft Gauge Invariance for Spin 2 G ijkl = ij q i q j q 2 E 2 kl q k q k q 2 K 2 (q) (j $ k, l) 2 types of non-localities Add non-dynamical h 00 (Newton) h 0i V (r) 1 r +... Find K 2 (q) =c 2 g q Locality =) h µ h µ µ µ (slowly varying µ ) µ (q)! µ (q)+q µ + q µ (soft µ )

35 Soft Gauge Invariance for Spin 1 and 2 Soft gauge invariance is required to ensure that the nondynamical fields are mixed with the propagating degrees of freedom, such that long range forces inherit the finite speed of propagation of the spin 1 or spin 2 particles

36 (Soft) Gauge Invariant Spin 2 Theories Difficult. Simple attempts fail Leading to many questions: What restrictions are placed on E? n 2 = K n (p n ) What if we include fermions and gauge/vector bosons? What constraints apply to E? q 2 = K q (q) Is the equivalence principle still required for consistency? What objects can we couple to? Need systematic analysis

37 Soft Graviton Scattering

38 Soft Graviton Scattering M N+1 = M N + X f " X i µ (q) T µ i (p i ) (E i E q ) 2 Ki (p i q) µ (q) T µ f (p f ) (E f + E q ) 2 Kf (p f + q) #

39 Soft Graviton Scattering M N+1 = M N Denominator: + X f " X i µ (q) T µ i (p i ) (E i E q ) 2 Ki (p i q) µ (q) T µ f (p f ) (E f + E q ) 2 Kf (p f + q) (E n E q ) 2 Kn (p n q) = 2 q n (p n ) #! q (E q, q) n (p n ) E n, 1 K p n

40 Soft Graviton Scattering M N+1 = M N " + X f X i µ (q) T µ i (p i ) 2 q i (p i) µ (q) T µ f (p f ) 2 q f (p f ) # Denominator: (E n E q ) 2 Kn (p n q) = 2 q n (p n )! q (E q, q) n (p n ) E n, 1 K p n

41 Unitarity and Locality Constraint µ (q)! µ (q)+q µ + q µ (soft µ )

42 Unitarity and Locality Constraint µ (q)! µ (q)+q µ + q µ (soft µ ) X i q µ T µ i (p i ) q i (p i) = X f q µ T µ f (p f ) q f (p f )

43 Unitarity and Locality Constraint µ (q)! µ (q)+q µ + q µ (soft µ ) X i q µ T µ i (p i ) q i (p i) = X f q µ T µ f (p f ) q f (p f ) Cancel graviton momenta T µ n (p n ) / µ n(p n )

44 Unitarity and Locality Constraint µ (q)! µ (q)+q µ + q µ (soft µ ) X i q µ T µ i (p i ) q i (p i) = X f q µ T µ f (p f ) q f (p f ) Cancel graviton momenta T µ n (p n )=g n (E n ) µ n(p n ) n(p n )

45 Unitarity and Locality Constraint µ (q)! µ (q)+q µ + q µ (soft µ ) X i q µ T µ i (p i ) q i (p i) = X f q µ T µ f (p f ) q f (p f ) Cancel graviton momenta X i T µ n (p n )=g n (E n ) µ n(p n ) n(p n ) g i (E i ) i (p i )= X f g f (E f ) f (p f )

46 Conservation Laws =0 X g i (E i ) E i = X f g f (E f ) E f i (Grav. Coupling) g n (E n )=apple + Q n E n

47 Conservation Laws =0 X g i (E i ) E i = X f g f (E f ) E f i (Grav. Coupling) g n (E n )=apple + Q n E n

48 Conservation Laws =0 X g i (E i ) E i = X f g f (E f ) E f i (Grav. Coupling) g n (E n )=apple + Q n E n = i X i g i (E i K p i = X f g f (E f K p f g n (E n K p n = a p n

49 Conservation Laws =0 X g i (E i ) E i = X f g f (E f ) E f i (Grav. Coupling) g n (E n )=apple + Q n E n = i X i g i (E i K p i = X f g f (E f K p f g n (E n K p n = a p n (Disp. Relation) apple E 2 n +2Q n E n = a 2 p n 2 + b n

50 Dispersion Relation apple E 2 n +2Q n E n = apple c 2 g p n 2 + b n Complete the square: E n! E n Q n apple,

51 Dispersion Relation apple E 2 n +2Q n E n = apple c 2 g p n 2 + b n Complete the square: E n! E n Q n apple, E 2 n = p n 2 c 2 g + m 2 n c 4 g Special Relativistic Dispersion Relation

52 Some Consequences - Lorentz violating Standard Model - Lorentz violating approaches to quantum gravity - Doubly/deformed special relativity - Lorentz violating alternatives to inflation Brings into doubt the viability of these models

53 Conclusions - Locality requires soft gauge invariance - For spin, special relativity is easily violated in principle apple 1 - For spin 2, special relativity is difficult to violate: - The relativistic energy-momentum relation must be exact - The leading interactions must be Lorentz invariant - It remains to be proven if all higher order interactions are too

electrodynamics and Lorentz violation

electrodynamics and Lorentz violation Vacuum Cherenkov radiation in Lorentz violating quantum electrodynamics and experimental limits on the scale of Lorentz violation Damiano Anselmi (IHEP/CAS, Beijing, & Pisa University) Lorentz symmetry

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

Part III. Interacting Field Theory. Quantum Electrodynamics (QED)

Part III. Interacting Field Theory. Quantum Electrodynamics (QED) November-02-12 8:36 PM Part III Interacting Field Theory Quantum Electrodynamics (QED) M. Gericke Physics 7560, Relativistic QM 183 III.A Introduction December-08-12 9:10 PM At this point, we have the

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

Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016

Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016 Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016 We are directly observing the history of the universe as we look deeply into the sky. JUN 30, 2016 ZZXianyu (CMSA) 2 At ~10 4 yrs the universe becomes

More information

David Mattingly University of California-Davis

David Mattingly University of California-Davis David Mattingly University of California-Davis Quantum gravity in the Americas III Penn State August 26 th, 2006 What is QG phenomenology? The search for effects at low energies(

More information

Fundamental Interactions (Forces) of Nature

Fundamental Interactions (Forces) of Nature Chapter 14 Fundamental Interactions (Forces) of Nature Interaction Gauge Boson Gauge Boson Mass Interaction Range (Force carrier) Strong Gluon 0 short-range (a few fm) Weak W ±, Z M W = 80.4 GeV/c 2 short-range

More information

Gravity, Strings and Branes

Gravity, Strings and Branes Gravity, Strings and Branes Joaquim Gomis International Francqui Chair Inaugural Lecture Leuven, 11 February 2005 Fundamental Forces Strong Weak Electromagnetism QCD Electroweak SM Gravity Standard Model

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

What We Really Know About Neutrino Speeds

What We Really Know About Neutrino Speeds What We Really Know About Neutrino Speeds Brett Altschul University of South Carolina March 22, 2013 In particle physics, the standard model has been incredibly successful. If the Higgs boson discovered

More information

Gravity, Strings and Branes

Gravity, Strings and Branes Gravity, Strings and Branes Joaquim Gomis Universitat Barcelona Miami, 23 April 2009 Fundamental Forces Strong Weak Electromagnetism QCD Electroweak SM Gravity Standard Model Basic building blocks, quarks,

More information

Loop corrections in Yukawa theory based on S-51

Loop corrections in Yukawa theory based on S-51 Loop corrections in Yukawa theory based on S-51 Similarly, the exact Dirac propagator can be written as: Let s consider the theory of a pseudoscalar field and a Dirac field: the only couplings allowed

More information

Lecture 6:Feynman diagrams and QED

Lecture 6:Feynman diagrams and QED Lecture 6:Feynman diagrams and QED 0 Introduction to current particle physics 1 The Yukawa potential and transition amplitudes 2 Scattering processes and phase space 3 Feynman diagrams and QED 4 The weak

More information

Aspects of Spontaneous Lorentz Violation

Aspects of Spontaneous Lorentz Violation Aspects of Spontaneous Lorentz Violation Robert Bluhm Colby College IUCSS School on CPT & Lorentz Violating SME, Indiana University, June 2012 Outline: I. Review & Motivations II. Spontaneous Lorentz Violation

More information

The path integral for photons

The path integral for photons The path integral for photons based on S-57 We will discuss the path integral for photons and the photon propagator more carefully using the Lorentz gauge: as in the case of scalar field we Fourier-transform

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

Manifestly diffeomorphism invariant classical Exact Renormalization Group

Manifestly diffeomorphism invariant classical Exact Renormalization Group Manifestly diffeomorphism invariant classical Exact Renormalization Group Anthony W. H. Preston University of Southampton Supervised by Prof. Tim R. Morris Talk prepared for Asymptotic Safety seminar,

More information

Fundamentals of Neutrino Physics and Astrophysics

Fundamentals of Neutrino Physics and Astrophysics Fundamentals of Neutrino Physics and Astrophysics Carlo Giunti Istituto Nazionale di Fisica Nucleare, Sezione di Torino and Dipartimento di Fisica Teorica, Universita di Torino, Italy Chung W. Kim Korea

More information

Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo

Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo Particle Physics Fall 2015 1 Course Overview Lecture 1: Introduction, Decay Rates and Cross Sections Lecture 2: The Dirac Equation and Spin

More information

arxiv: v1 [hep-ph] 16 Aug 2012

arxiv: v1 [hep-ph] 16 Aug 2012 Low Energy Tests of Lorentz and CPT Violation Don Colladay 5800 Bay Shore Road, New College of Florida arxiv:1208.3474v1 [hep-ph] 16 Aug 2012 Abstract. An overview of the theoretical framework of the Standard

More information

Chris Verhaaren Joint Theory Seminar 31 October With Zackaria Chacko, Rashmish Mishra, and Simon Riquelme

Chris Verhaaren Joint Theory Seminar 31 October With Zackaria Chacko, Rashmish Mishra, and Simon Riquelme Chris Verhaaren Joint Theory Seminar 31 October 2016 With Zackaria Chacko, Rashmish Mishra, and Simon Riquelme It s Halloween A time for exhibiting what some find frightening And seeing that it s not so

More information

Lecture notes for QFT I (662)

Lecture notes for QFT I (662) Preprint typeset in JHEP style - PAPER VERSION Lecture notes for QFT I (66) Martin Kruczenski Department of Physics, Purdue University, 55 Northwestern Avenue, W. Lafayette, IN 47907-036. E-mail: markru@purdue.edu

More information

Elementary Particles, Flavour Physics and all that...

Elementary Particles, Flavour Physics and all that... Elementary Particles, Flavour Physics and all that... 1 Flavour Physics The term Flavour physics was coined in 1971 by Murray Gell-Mann and his student at the time, Harald Fritzsch, at a Baskin-Robbins

More information

arxiv:hep-ph/ v1 1 Feb 2005

arxiv:hep-ph/ v1 1 Feb 2005 Vector Goldstone Boson and Lorentz Invariance arxiv:hep-ph/050011v1 1 Feb 005 Ling-Fong Li Department of Physics, Carnegie Mellon University, Pittsburgh, PA 1513 January 5, 018 Abstract Spontanous symmetry

More information

Weak interactions and vector bosons

Weak interactions and vector bosons Weak interactions and vector bosons What do we know now about weak interactions? Theory of weak interactions Fermi's theory of weak interactions V-A theory Current - current theory, current algebra W and

More information

An Introduction to the Standard Model of Particle Physics

An Introduction to the Standard Model of Particle Physics An Introduction to the Standard Model of Particle Physics W. N. COTTINGHAM and D. A. GREENWOOD Ж CAMBRIDGE UNIVERSITY PRESS Contents Preface. page xiii Notation xv 1 The particle physicist's view of Nature

More information

chapter 3 Spontaneous Symmetry Breaking and

chapter 3 Spontaneous Symmetry Breaking and chapter 3 Spontaneous Symmetry Breaking and Nambu-Goldstone boson History 1961 Nambu: SSB of chiral symmetry and appearance of zero mass boson Goldstone s s theorem in general 1964 Higgs (+others): consider

More information

Feynman Diagrams of the Standard Model Sedigheh Jowzaee

Feynman Diagrams of the Standard Model Sedigheh Jowzaee tglied der Helmholtz-Gemeinschaft Feynman Diagrams of the Standard Model Sedigheh Jowzaee PhD Seminar, 5 July 01 Outlook Introduction to the standard model Basic information Feynman diagram Feynman rules

More information

The Standard Model of Electroweak Physics. Christopher T. Hill Head of Theoretical Physics Fermilab

The Standard Model of Electroweak Physics. Christopher T. Hill Head of Theoretical Physics Fermilab The Standard Model of Electroweak Physics Christopher T. Hill Head of Theoretical Physics Fermilab Lecture I: Incarnations of Symmetry Noether s Theorem is as important to us now as the Pythagorean Theorem

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

Stephen Blaha, Ph.D. M PubHsMtw

Stephen Blaha, Ph.D. M PubHsMtw Quantum Big Bang Cosmology: Complex Space-time General Relativity, Quantum Coordinates,"Dodecahedral Universe, Inflation, and New Spin 0, 1 / 2,1 & 2 Tachyons & Imagyons Stephen Blaha, Ph.D. M PubHsMtw

More information

Suppressing the Lorentz violations in the matter sector A class of extended Hořava gravity

Suppressing the Lorentz violations in the matter sector A class of extended Hořava gravity Suppressing the Lorentz violations in the matter sector A class of extended Hořava gravity A. Emir Gümrükçüoğlu University of Nottingham [Based on arxiv:1410.6360; 1503.07544] with Mattia Colombo and Thomas

More information

Introduction to string theory 2 - Quantization

Introduction to string theory 2 - Quantization Remigiusz Durka Institute of Theoretical Physics Wroclaw / 34 Table of content Introduction to Quantization Classical String Quantum String 2 / 34 Classical Theory In the classical mechanics one has dynamical

More information

The cosmological constant puzzle

The cosmological constant puzzle The cosmological constant puzzle Steven Bass Cosmological constant puzzle: Accelerating Universe: believed to be driven by energy of nothing (vacuum) Vacuum energy density (cosmological constant or dark

More information

The Minimal Lorentz-Violating Standard Model Extension

The Minimal Lorentz-Violating Standard Model Extension The Minimal Lorentz-Violating Standard Model Extension Brett Altschul University of South Carolina June 17, 2018 We have been testing relativity experimentally for a long time. The first good test was

More information

SM predicts massless neutrinos

SM predicts massless neutrinos MASSIVE NEUTRINOS SM predicts massless neutrinos What is the motivation for considering neutrino masses? Is the question of the existence of neutrino masses an isolated one, or is connected to other outstanding

More information

Effective Field Theory

Effective Field Theory Effective Field Theory Iain Stewart MIT The 19 th Taiwan Spring School on Particles and Fields April, 2006 Physics compartmentalized Quantum Field Theory String Theory? General Relativity short distance

More information

Electroweak Physics. Krishna S. Kumar. University of Massachusetts, Amherst

Electroweak Physics. Krishna S. Kumar. University of Massachusetts, Amherst Electroweak Physics Krishna S. Kumar University of Massachusetts, Amherst Acknowledgements: M. Grunewald, C. Horowitz, W. Marciano, C. Quigg, M. Ramsey-Musolf, www.particleadventure.org Electroweak Physics

More information

The Standard Model Part. II

The Standard Model Part. II Our Story Thus Far The Standard Model Part. II!!We started with QED (and!)!!we extended this to the Fermi theory of weak interactions! Adding G F!!Today we will extended this to Glashow-Weinberg-Salam

More information

Gravitational radiation

Gravitational radiation Lecture 28: Gravitational radiation Gravitational radiation Reading: Ohanian and Ruffini, Gravitation and Spacetime, 2nd ed., Ch. 5. Gravitational equations in empty space The linearized field equations

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

Quantum ElectroDynamics III

Quantum ElectroDynamics III Quantum ElectroDynamics III Feynman diagram Dr.Farida Tahir Physics department CIIT, Islamabad Human Instinct What? Why? Feynman diagrams Feynman diagrams Feynman diagrams How? What? Graphic way to represent

More information

The Non-commutative S matrix

The Non-commutative S matrix The Suvrat Raju Harish-Chandra Research Institute 9 Dec 2008 (work in progress) CONTEMPORARY HISTORY In the past few years, S-matrix techniques have seen a revival. (Bern et al., Britto et al., Arkani-Hamed

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

Mathematical and Physical Foundations of Extended Gravity (II)

Mathematical and Physical Foundations of Extended Gravity (II) Mathematical and Physical Foundations of Extended Gravity (II) -The Gravitational Waves era- Salvatore Capozziello Università di Napoli Federico II INFN sez. di Napoli SIGRAV Open Fundamental Issues! What

More information

Beyond Einstein: gravitational waves from extended gravities

Beyond Einstein: gravitational waves from extended gravities Beyond Einstein: gravitational waves from extended gravities Salvatore Capozziello Università di Napoli Federico II and INFN sez. di Napoli in collaboration with Mariafelicia De Laurentis Institute for

More information

Massless and massive vector Goldstone bosons in nonlinear quantum electrodynamics

Massless and massive vector Goldstone bosons in nonlinear quantum electrodynamics Massless and massive vector Goldstone bosons in nonlinear quantum electrodynamics J. L. Chkareuli, Z. R. Kepuladze E. Andronikashvili Institute of Physics and I. Chavchavadze State University 0177 Tbilisi,

More information

An Introduction to. Michael E. Peskin. Stanford Linear Accelerator Center. Daniel V. Schroeder. Weber State University. Advanced Book Program

An Introduction to. Michael E. Peskin. Stanford Linear Accelerator Center. Daniel V. Schroeder. Weber State University. Advanced Book Program An Introduction to Quantum Field Theory Michael E. Peskin Stanford Linear Accelerator Center Daniel V. Schroeder Weber State University 4B Advanced Book Program TT Addison-Wesley Publishing Company Reading,

More information

Scattering Amplitudes

Scattering Amplitudes Scattering Amplitudes LECTURE 1 Jaroslav Trnka Center for Quantum Mathematics and Physics (QMAP), UC Davis ICTP Summer School, June 2017 Particle experiments: our probe to fundamental laws of Nature Theorist

More information

Experiments testing macroscopic quantum superpositions must be slow

Experiments testing macroscopic quantum superpositions must be slow Experiments testing macroscopic quantum superpositions must be slow spatial (Scientic Reports (2016) - arxiv:1509.02408) Andrea Mari, Giacomo De Palma, Vittorio Giovannetti NEST - Scuola Normale Superiore

More information

4. The Standard Model

4. The Standard Model 4. The Standard Model Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 4. The Standard Model 1 In this section... Standard Model particle content Klein-Gordon equation Antimatter Interaction

More information

Vacuum Energy and the cosmological constant puzzle

Vacuum Energy and the cosmological constant puzzle Vacuum Energy and the cosmological constant puzzle Cosmological constant puzzle: Steven Bass Accelerating Universe: believed to be driven by energy of nothing (vacuum) Positive vacuum energy = negative

More information

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 14: CP and CP Violation

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 14: CP and CP Violation Particle Physics Dr Victoria Martin, Spring Semester 01 Lecture 14: CP and CP Violation!Parity Violation in Weak Decay!CP and CPT!Neutral meson mixing!mixing and decays of kaons!cp violation in K 0 and

More information

Gauge Theories of the Standard Model

Gauge Theories of the Standard Model Gauge Theories of the Standard Model Professors: Domènec Espriu (50%, coordinador) Jorge Casalderrey (25%) Federico Mescia (25%) Time Schedule: Mon, Tue, Wed: 11:50 13:10 According to our current state

More information

Momentum relaxation in holographic massive gravity

Momentum relaxation in holographic massive gravity Momentum relaxation in holographic massive gravity Richard Davison Lorentz Institute, Leiden Based on 1306.5792 [hep-th] Gauge/Gravity Duality 2013, Munich July 30 th 2013 Introduction and motivation We

More information

Why Cerenkov Radiation May Not Occur, Even When It Is Allowed by Lorentz-Violating Kinematics

Why Cerenkov Radiation May Not Occur, Even When It Is Allowed by Lorentz-Violating Kinematics S S symmetry Article Why Cerenkov Radiation May Not Occur, Even When It Is Allowed by Lorentz-Violating Kinematics Brett Altschul ID Department of Physics and Astronomy, University of South Carolina, Columbia,

More information

PRINCIPLES OF PHYSICS. \Hp. Ni Jun TSINGHUA. Physics. From Quantum Field Theory. to Classical Mechanics. World Scientific. Vol.2. Report and Review in

PRINCIPLES OF PHYSICS. \Hp. Ni Jun TSINGHUA. Physics. From Quantum Field Theory. to Classical Mechanics. World Scientific. Vol.2. Report and Review in LONDON BEIJING HONG TSINGHUA Report and Review in Physics Vol2 PRINCIPLES OF PHYSICS From Quantum Field Theory to Classical Mechanics Ni Jun Tsinghua University, China NEW JERSEY \Hp SINGAPORE World Scientific

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

Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material. From last time

Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material. From last time Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material From last time Quantum field theory is a relativistic quantum theory of fields and interactions. Fermions

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

Modern Approaches to Scattering Amplitudes

Modern Approaches to Scattering Amplitudes Ph.D. Workshop, 10 October 2017 Outline Scattering Amplitudes 1 Scattering Amplitudes Introduction The Standard Method 2 On-Shell vs Off-Shell On-Shell building blocks BCFW Recursion Relations 3 Amplitudes

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

Towards solution of string theory in AdS3 x S 3

Towards solution of string theory in AdS3 x S 3 Towards solution of string theory in AdS3 x S 3 Arkady Tseytlin based on work with Ben Hoare: arxiv:1303.1037, 1304.4099 Introduction / Review S-matrix for string in AdS3 x S3 x T4 with RR and NSNS flux

More information

Part III The Standard Model

Part III The Standard Model Part III The Standard Model Theorems Based on lectures by C. E. Thomas Notes taken by Dexter Chua Lent 2017 These notes are not endorsed by the lecturers, and I have modified them (often significantly)

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

Vacuum Energy and. Cosmological constant puzzle:

Vacuum Energy and. Cosmological constant puzzle: Vacuum Energy and the cosmological constant puzzle Steven Bass Cosmological constant puzzle: (arxiv:1503.05483 [hep-ph], MPLA in press) Accelerating Universe: believed to be driven by energy of nothing

More information

The Quantum Theory of Fields. Volume I Foundations Steven Weinberg

The Quantum Theory of Fields. Volume I Foundations Steven Weinberg The Quantum Theory of Fields Volume I Foundations Steven Weinberg PREFACE NOTATION x x xxv 1 HISTORICAL INTRODUCTION 1 1.1 Relativistic Wave Mechanics 3 De Broglie waves q Schrödinger-Klein-Gordon wave

More information

Lecture notes for FYS610 Many particle Quantum Mechanics

Lecture notes for FYS610 Many particle Quantum Mechanics UNIVERSITETET I STAVANGER Institutt for matematikk og naturvitenskap Lecture notes for FYS610 Many particle Quantum Mechanics Note 20, 19.4 2017 Additions and comments to Quantum Field Theory and the Standard

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

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

The 2015 Data Tables for Lorentz and CPT Violation

The 2015 Data Tables for Lorentz and CPT Violation The 2015 Data Tables for Lorentz and CPT Violation Reviews of Modern Physics 83, 11 (2011) update: arxiv:0801.0287v8 (January 2015) Kostelecký, NR Second IUCSS Summer School on the Lorentz- and CPT-violating

More information

The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten

The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten Lecture 4 QCD as a Gauge Theory Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local

More information

Towards a manifestly diffeomorphism invariant Exact Renormalization Group

Towards a manifestly diffeomorphism invariant Exact Renormalization Group Towards a manifestly diffeomorphism invariant Exact Renormalization Group Anthony W. H. Preston University of Southampton Supervised by Prof. Tim R. Morris Talk prepared for UK QFT-V, University of Nottingham,

More information

Introduction to Elementary Particles

Introduction to Elementary Particles David Criffiths Introduction to Elementary Particles Second, Revised Edition WILEY- VCH WILEY-VCH Verlag GmbH & Co. KGaA Preface to the First Edition IX Preface to the Second Edition XI Formulas and Constants

More information

Exotic BSM Physics and N-N oscillation R. N. Mohapatra University of Maryland

Exotic BSM Physics and N-N oscillation R. N. Mohapatra University of Maryland Exotic BSM Physics and N-N oscillation R. N. Mohapatra University of Maryland K. S. Babu and R.N.M, PRD91,096009 (2015); PRD94, 054034(2016) NNbar search and BSM physics Nnbar is a gold mine of informaeon

More information

Particles and Strings Probing the Structure of Matter and Space-Time

Particles and Strings Probing the Structure of Matter and Space-Time Particles and Strings Probing the Structure of Matter and Space-Time University Hamburg DPG-Jahrestagung, Berlin, March 2005 2 Physics in the 20 th century Quantum Theory (QT) Planck, Bohr, Heisenberg,...

More information

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM Lecture 03 The Standard Model of Particle Physics Part II The Higgs Boson Properties of the SM The Standard Model So far we talked about all the particles except the Higgs If we know what the particles

More information

Overview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions.

Overview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions. Overview The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions. Our understanding is about to take a giant leap.. the Large Hadron Collider

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

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama Lorentz-covariant spectrum of single-particle states and their field theory Physics 30A, Spring 007, Hitoshi Murayama 1 Poincaré Symmetry In order to understand the number of degrees of freedom we need

More information

with EFTCAMB: The Hořava gravity case

with EFTCAMB: The Hořava gravity case Testing dark energy and modified gravity models with EFTCAMB: The Hořava gravity case Noemi Frusciante UPMC-CNRS, Institut d Astrophysique de Paris, Paris ERC-NIRG project no.307934 Based on NF, M. Raveri,

More information

REVIEW REVIEW. Quantum Field Theory II

REVIEW REVIEW. Quantum Field Theory II Quantum Field Theory II PHYS-P 622 Radovan Dermisek, Indiana University Notes based on: M. Srednicki, Quantum Field Theory Chapters: 13, 14, 16-21, 26-28, 51, 52, 61-68, 44, 53, 69-74, 30-32, 84-86, 75,

More information

Quantum Field Theory II

Quantum Field Theory II Quantum Field Theory II PHYS-P 622 Radovan Dermisek, Indiana University Notes based on: M. Srednicki, Quantum Field Theory Chapters: 13, 14, 16-21, 26-28, 51, 52, 61-68, 44, 53, 69-74, 30-32, 84-86, 75,

More information

On-shell Recursion Relations of Scattering Amplitudes at Tree-level

On-shell Recursion Relations of Scattering Amplitudes at Tree-level On-shell Recursion Relations of Scattering Amplitudes at Tree-level Notes for Journal Club by Yikun Wang June 9, 206 We will introduce the on-shell recursion relations of scattering amplitudes at tree-level

More information

Soft Theorem and its Classical Limit

Soft Theorem and its Classical Limit Soft Theorem and its Classical Limit Ashoke Sen Harish-Chandra Research Institute, Allahabad, India Kyoto, July 2018 1 In this talk we focus on soft graviton theorem however similar results exist for soft

More information

Why Does Gravity Obey an Inverse Square Law?

Why Does Gravity Obey an Inverse Square Law? Why Does Gravity Obey an Inverse Square Law? This paper uncovers the reason why gravity obeys an inverse square law and not, for example, an inverse cubic law, or any other law with any other power. A

More information

Quarks, Leptons and Gauge Fields Downloaded from by on 03/13/18. For personal use only.

Quarks, Leptons and Gauge Fields Downloaded from  by on 03/13/18. For personal use only. QUARKS, LEPTONS & GAUGE FIELDS 2nd edition Kerson Huang Professor of Physics Mussuchusetts Institute qf Technology Y 8 World Scientific Singapore New Jersey London Hong Kong Publirhed by World Scientific

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

Vacuum Energy and Effective Potentials

Vacuum Energy and Effective Potentials Vacuum Energy and Effective Potentials Quantum field theories have badly divergent vacuum energies. In perturbation theory, the leading term is the net zero-point energy E zeropoint = particle species

More information

Theory of anomalous couplings. in Effective Field Theory (EFT)

Theory of anomalous couplings. in Effective Field Theory (EFT) Theory of Anomalous Couplings in Effective Field Theory (EFT) Nicolas Greiner Max Planck Institut für Physik, München aqgc Dresden, 30.9. 2.10. 2103 Motivation July 4, 2012: New particle found! (Compatible

More information

Review of scalar field theory. Srednicki 5, 9, 10

Review of scalar field theory. Srednicki 5, 9, 10 Review of scalar field theory Srednicki 5, 9, 10 2 The LSZ reduction formula based on S-5 In order to describe scattering experiments we need to construct appropriate initial and final states and calculate

More information

- ~200 times heavier than the e GeV µ travels on average. - does not interact strongly. - does emit bremsstrahlung in

- ~200 times heavier than the e GeV µ travels on average. - does not interact strongly. - does emit bremsstrahlung in Muons M. Swartz 1 Muons: everything you ve ever wanted to know The muon was first observed in cosmic ray tracks in a cloud chamber by Carl Anderson and Seth Neddermeyer in 1937. It was eventually shown

More information

Basics of Higgs Physics

Basics of Higgs Physics Basics of iggs Physics Sven einemeyer, IFCA (Santander) Karlsruhe, 07/2007 1. The iggs Boson in the SM 2. The iggs Boson in the MSSM Sven einemeyer Basics of iggs Physics presusy07 (Karlsruhe) 23.07.2007

More information

A Review of Higgs Particle Physics

A Review of Higgs Particle Physics Prespacetime Journal July 2012 Vol. 3 Issue 9 pp. 809-817 809 A Review of Higgs Particle Physics Higgs Essay Lawrence B. Crowell 1 Alpha Institute of Advanced Study 10600 Cibola Lp 311 NW Albuquerque,

More information

QCD in the light quark (up & down) sector (QCD-light) has two mass scales M(GeV)

QCD in the light quark (up & down) sector (QCD-light) has two mass scales M(GeV) QCD in the light quark (up & down) sector (QCD-light) has two mass scales M(GeV) 1 m N m ρ Λ QCD 0 m π m u,d In a generic physical system, there are often many scales involved. However, for a specific

More information

THERMAL HISTORY OF THE UNIVERSE

THERMAL HISTORY OF THE UNIVERSE M. Pettini: Introduction to Cosmology Lecture 7 THERMAL HISTORY OF THE UNIVERSE The Universe today is bathed in an all-pervasive radiation field, the Cosmic Microwave Background (CMB) which we introduced

More information

Modern Physics for Frommies V Gravitation Lecture 8

Modern Physics for Frommies V Gravitation Lecture 8 /6/017 Fromm Institute for Lifelong Learning University of San Francisco Modern Physics for Frommies V Gravitation Lecture 8 Administrative Matters Suggested reading Agenda What do we mean by Quantum Gravity

More information

QUANTUM FIELD THEORY. A Modern Introduction MICHIO KAKU. Department of Physics City College of the City University of New York

QUANTUM FIELD THEORY. A Modern Introduction MICHIO KAKU. Department of Physics City College of the City University of New York QUANTUM FIELD THEORY A Modern Introduction MICHIO KAKU Department of Physics City College of the City University of New York New York Oxford OXFORD UNIVERSITY PRESS 1993 Contents Quantum Fields and Renormalization

More information

2-Group Global Symmetry

2-Group Global Symmetry 2-Group Global Symmetry Clay Córdova School of Natural Sciences Institute for Advanced Study April 14, 2018 References Based on Exploring 2-Group Global Symmetry in collaboration with Dumitrescu and Intriligator

More information

Topics in Standard Model. Alexey Boyarsky Autumn 2013

Topics in Standard Model. Alexey Boyarsky Autumn 2013 Topics in Standard Model Alexey Boyarsky Autumn 2013 New particles Nuclear physics, two types of nuclear physics phenomena: α- decay and β-decay See Introduction of this article for the history Cosmic

More information