All the fundamental massless fields in bosonic string theory

Size: px
Start display at page:

Download "All the fundamental massless fields in bosonic string theory"

Transcription

1 Early View publication on wileyonlinelibrary.com (issue and page numbers not yet assigned; citable using Digital Object Identifier DOI) Fortschr. Phys., 8 (0) / DOI 0.00/prop All the fundamental massless fields in bosonic string theory E. B. Manoukian The Institute for Fundamental Study, Naresuan University, Phitsanulok 65000, Thailand Received 9 January 0, revised 9 January 0, accepted January 0 Published online 3 February 0 Key words Massless fields of bosonic strings, propagator theory, particle polarizations, higher dimensions, constraints, non-constrained external sources. A systematic analysis of the massless fields in the mass spectra of bosonic strings is carried in arbitrary spacetime dimension D>. The emphasis is put on the derivations of their propagators, their polarization aspects and the underlying constraints involved. The treatment is given, in the presence of external sources, in the celebrated Coulomb gauge for the second rank tensors and vector fields, which ensures positivity - a result which is also established in the process. No constraints are imposed on the external sources so that their components may be varied independently generating complete expressions for the propagators. This latter condition is an important one in the generation of dynamical theories with constraints involving such modifications as Faddeev-Popov factors. 0 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim Introduction What is remarkable about string theory is that the fundamental fields that are required to describe the dynamics of elementary particles arise naturally in the mass spectra of oscillating strings and are not, a priori, assumed to exist or put in by hand in the the underlying theories. At present only the massless fields string modes are really physically relevant because of the enormous masses of the massive fields string-excitation modes. A massless vector field, for example, may be thought to acquire mass by some mechanism such as, for example, from open strings whose end points are attached to different branes or by some other means such as the Higgs mechanism. In this paper, we are interested in all the massless fields excitations of bosonic strings. The massless fields in question are: the second rank symmetric tensor field, the second-rank anti-symmetric tensor field, the vector field and the scalar one (c.f. [ 3]) which arise in the mass spectra of oscillating bosonic strings in D =6dimensionalspacetime. The second rank symmetric tensor field is associated with the graviton and the scalar one with the dilaton which is thought to provide a coupling strength in string theory through its vacuum expectation value. We are interested in dynamical aspects of these fields. To this end, we are concerned about underlying constraints and the explicit expressions of their propagators. We set the dimension of spacetime arbitrarily to D>. We work in the celebrated Coulomb gauge, as applied to the second rank tensors and vector fields, which ensures positivity of the formalism as will be established in each case. For earlier four-dimensional studies of the massless symmetric second rank tensor, c.f [4], and for the anti-symmetric one, c.f. [5 7]. Our analysis, however, is involved with dynamical aspects by deriving expressions of the underlying propagators, as just mentioned, and obtain the basic polarization aspects of the fields and the inherit degrees of freedom in arbitrary dimensional spacetime D>. Quite importantly, the fields are coupled to non-constrainedexternal sources so that each of their components may be varied independently and thus the complete expressions of the propagators are obtained. Also the variations of each of the components of external sources is necessary in describing full field theory interactions, such as deriving Faddeev-Popov factors. A fairly detailed manoukian eb@hotmail.com 0 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

2 E. B. Manoukian: All the fundamental massless fields in bosonic string theory demonstration of the importance of varying the components of the external sources independently with applications to gauge theories is given in Sect. 3 of [4] for the convenience of the reader. In the present work, the scalar field presents no challenge and nothing new emerges about it here. The vector field is relatively simpler to analyze than the second rank tensor cases, but we provide a detailed analysis for it to set up the formalism involved in our analysis, and we also need aspects of its underlying polarization vectors for the other cases. This is given in Sect.. Sections 3 and 4 constitute the main contribution of this paper dealing, in turn, with the symmetric and anti-symmetric tensor field cases, respectively. The Minkowski metric is defined by [η μν ]=diag[,,...,], the Greek indices μ,ν,...go over 0,,...,D, while the Latin ones i,j,...go over,...,d. Vector field The Lagrangian density of a massless vector field A μ, may be defined by L = 4 F μν F μν, F μν (x) = μ A ν (x) ν A μ (x). () It is invariant under the gauge transformation A μ A μ + μ Λ. We work in the Coulomb gauge i A i =0, () with a summation over i is understood as a repeated index. We add an external source contribution to (), obtaining L = 4 F μν F μν + J μ A μ. (3) Quite generally, we may write A μ = A 0 η μ0 + η μi A j. (4) Due to the constraint in (), one cannot vary the components of A j independently. We may, however, introduce a field with components A i that may be varied independently and set A i (x) =π ij A j (x), (5) π ij = (δ ij i j ) k k, (6) satisfying the identities π ij = π ji, i π ij =0, π ij j =0, π ij π jk = π ik, (7) operating as a projection operator. Upon varying A 0, A j the Lagrangian density (3) leads to μ μ A i = (δ ij i j ) k k J j, (8) k k A 0 = J 0. (9) Clearly only the A i may propagate. Since no constraints were imposed on J μ (x), we may vary its components independently. Upon taking the vacuum expectation values of (8), (9), setting 0 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

3 Fortschr. Phys. (0) A μ (x) 0 = ( iδ/δj μ (x)) 0 + 0, and integrating with respect to the source components, we obtain =exp[ i (dx)(dx ) J μ (x)δ μν + (x x )J ν (x )], (0) Δ μν + (x x )= (dp) (π) D eip(x x ) Δ μν + (p), () and Δ 0i + =Δi0 + =0, Δ 00 + (p) = p, () Δ ij + = p iɛ πij, ɛ +0, (3) now π ij = δ ij pi p j p. (4) Let e,..., e D, p/ p,bed mutually pairwise orthonormal vectors spanning a (D ) Euclidean space, i.e., from which δ ij = pi p p i D p + e i λ e j λ, (5) λ= π ij = D λ= e i λ ej λ. (6) Clearly, Δ 00 + (p) gives rise to a phase to Upon using the identity [ i p iɛ ] p = π +iɛ p [ δ(p0 p )+δ(p 0 + p )], (7) and ()-(6), we obtain for the vacuum persistence probability D =exp[ λ= establishing the positivity of the formalism, d D p p (π) D J(λ, p) ] <, (8) J(λ, p) =J i (p) ɛ i λ, p0 =+ p. (9) The number of independent polarization states may be obtained from (6) to be D λ= e i λ e i λ = π ii = δ ii =D. (0) 0 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

4 4 E. B. Manoukian: All the fundamental massless fields in bosonic string theory 3 Symmetric traceless second rank tensor field The Lagrangian density of a massless symmetric tensor field is given by (c.f. [8]) L = σ h μν σ h μν + μ h μν σ h σ ν σ h σμ μ h + μ h μ h, () h = h μ μ, h μν = h νμ. It is invariant under the gauge transformation h μν h μν + μ Λ ν + ν Λ μ, () up to a total derivative. We work in the Coulomb-like gauge i h iν =0, (3) with a sum over i. We add an external source contribution to the Lagrangian density in () to obtain L = σ h μν σ h μν + μ h μν σ h σ ν σ h σμ μ h + μ h μ h + T μν h μν. (4) We may write h μν = η μi η νj h ij (η μ0 η νi + η μi η ν0 )h 0i + η μ0 η ν0 h 00. (5) Due to the constraint in (3), the components h ij, h 0i, cannot be varied independently. We can, however, introduce fields H kl, φ j, whose components may be varied independently, and set h ij = (πik π jl + π il π jk )H hl, (6) h 0i = π ij φ j, (7) with π ij defined in (6). The variations of the fields φ j, h 00, H kl, lead from the Lagrangian density (4), after some labor, to h ii = k k T 00, h 00 [ = (D ) k k (D 3) l l T 00 + π ij T ij], (8) h 0i = l l πik T 0k, π ij = (δ ij i j k k ), (9) h ij = [ D D recalling that δ i i = D, = μ μ. Clearly, only h ij may propagate. We note that if constraints are imposed on the external sources on the right-hand of these equations, the complete expression of the propagator in question would not follow. Since no constraints were imposed on T μν (x), we may vary its components independently. Upon taking the vacuum expectation values of (9), (30), setting 0 + h μν (x) 0 =( iδ/δt μν (x)) 0 + 0, and integrating with respect to the source components, we obtain (π ik π jl + π il π jk ) π ij π kl] T kl + D πij k k T 00, (30) [ ] i =exp (dx)(dx ) T μν (x)δ μν,λσ + (x x )T λσ (x ), (3) Δ μν,λσ + (x x )= (dp) ) (π) D eip(x x Δ μν,λσ + (p), (3) 0 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

5 Fortschr. Phys. (0) 5 Δ 00,00 + (p) = D 3 D Δ 00,ij + (p) = D (p ) p 4, p = p (p 0 ), (33) p πij, Δ 00,0i + =Δ 0i,00 + =0, (34) Δ 0i,0k + (p) = p πik, (35) Δ ij,kl + = p iɛ D [ D (π ik π jl + π il π jk ) π ij π kl],ɛ +0, (36) Δ ij,00 + (p) = D πij p, (37) and π ij is given in (4). Clearly, Δ 00 + (p), Δ0i,0k + (p), Δij,00 + (p), Δ00,ij + (p), provide phase factors to Weusethecompleteness relation in (5), the identity in (6), and the following identity [ D (π ik π jl + π il π jk ) π ij π kl] = D ɛ ij (λ, λ )= D [ D D D (e i λ ej λ + e i λ ej λ ) δ λ,λ ɛ ij (λ, λ ) ɛ kl (λ, λ ), (38) κ= e i κ ej κ ], (39) obtained after a few steps. Finally the identity in (7) gives for the vacuum persistence probability the expression =exp[ D establishing the positivity of the formalism, and d D p p (π) D T (λ, λ,p) ] <, (40) T (λ, λ,p)=t ij (p) ɛ ij (λ, λ ), p 0 =+ p. (4) The number of independent polarization states is obtained from the identity (38) and is worked out as follows: D ɛ ij (λ, λ ) ɛ ij (λ, λ )= D [ D we have used the set of equalities on the right-hand side of (0), and (π ii π jj + π ij π ji ) π ij π ij] = D(D 3), (4) π ij π ij = π ij δ ij = D. (43) 0 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

6 6 E. B. Manoukian: All the fundamental massless fields in bosonic string theory 4 Anti-symmetric second rank tensor field Consider an anti-symmetric tensor field C μν = C νμ, and introduce the tensor field F μνσ = μ C νσ + σ C μν + ν C σμ, (44) defined as a cyclic permutation of the indices. We define the Lagrangian density L = 6 F μνσ F μνσ. (45) The Lagrangian density is invariant under the gauge transformation C μν C μν + μ Λ ν ν Λ μ. (46) We work in the Coulomb-like gauge i C iν =0, (47) with a sum over i. We add an external source contribution to the Lagrangian density in (45) to obtain L = 6 F μνσ F μνσ + F μνσ J μνσ. (48) up to an overall multiplicative dimensional constant. We may write C μν = η μi η νj C ij (η μ0 η νi η μi η ν0 ) C 0i. (49) Due to the constraint in (47), one cannot vary all the components of C iν independently, we can, however, introduce fields with component χ kl, ϕ j, that may be varied independently, and set C ij = (πik π jl π il π jk ) χ kl, C 0i = π ij ϕ j, π ij = δ ij i j The variations of the components χ kl, ϕ j, lead from the Lagrangian density in (48) to k k. (50) k k C 0i = π ij J 0j, (5) C ij = (πik π jl π il π jk ) J kl. (5) Clearly, only C ij may propagate. Again if a constraint is imposed on the external source on the righthand sides of these equations, such as a transversality condition i J ij =0, the complete expression of the propagator in question would not follow. Upon taking the vacuum expectation values of (5), (5), setting 0 + C μν (x) 0 =( iδ/δj μν (x)) 0 + 0, and integrating with respect to the source components, we obtain =exp[ i (dx)(dx μν,λσ ) J μν (x) Δ + (x x )J λσ (x )] (53) Δ μν,σλ + (x x )= (dp) (π) D eip(x x ) Δμν,σλ + (p), (54) 0 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

7 Fortschr. Phys. (0) 7 Δ 00,00 00,0i 0i,00 ij,00 + =0= Δ + = Δ + = Δ +, Δ 0i,0j + (p) = p πij, (55) Clearly, Δ ij,kl + (p) = p iɛ (π ik π jl π il π jk ), ɛ +0. (56) Δ 0i,0j + (p) gives rise to a phase factor to Upon using the identity (π ik π jl π il π jk ) = D ε ij (λ, λ )ε kl (λ, λ ), (57) now ε ij (λ, λ )= (ei λ ej λ e i λ ej λ ), (58) the vacuum persistence probability emerges as with =exp[ D d D p p (π) D J(λ, λ,p) ] <, (59) J(λ, λ,p)=j ij (p) ε ij (λ, λ ), p 0 = p, (60) establishing the positivity of the formalism, except now for the number of independent polarization states, we obtain D ε ij (λ, λ ) ε ij (λ, λ )= [ π ii π jj π ij π ji] = (D )(D 3). (6) 5 Conclusion Detailed analysis of the massless fields of string theory was carried out in arbitrary dimensions of spacetime D(> ). We have worked in the celebrated Coulomb gauge, ensuring positivity, and no constraints were imposed on the external sources thus generating the complete expressions for the corresponding propagators. Much emphasis was put on polarization aspects of the fields, and the number of independent degrees of freedom naturally followed. It is interesting to note that for D =4, we recover our earlier expression of the graviton propagator derived in [4] by much more involved and a lengthy method. The importance of such propagators and their polarization aspects are expected to be useful in finding connections between string theory and field theory for computations and for the generation of non-trivial effective actions. These points will be taken up in subsequent reports, as well as the investigation of the massless fields in superstring theory. Acknowledgements The author would like to thank his colleagues at the Institute for their interest in this work. 0 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

8 8 E. B. Manoukian: All the fundamental massless fields in bosonic string theory References [] M. B. Green, J. H. Schwarz, and E. Witten, Superstring Theory, Vol., (Cambridge University Press, Cambridge, 988). [] K. Becker, M. Becker, and J. H. Schwarz, String Theory and M-Theory, (Cambridge University Press, Cambridge, 007). [3] J. Polchinski, String Theory, Vol. I, (Cambridge University Press, Cambridge, 005). [4] E. B. Manoukian and S. Sukkhasena, Fortschr. Phys. 55( ), 8 88 (007). [5] M. Kalb and P. Raymond, Phys. Rev. D 9, 73 (974). [6] E. Cremmer and J. Scherk, Nucl. Phys. B 7, 7 (974). [7] K. Hayashi, Phys. Lett. B 44, 497 (973). [8] J. Schwinger, Particles, Sources and Fields, (Addison-Wesley, Reading, Massachusets, 970). 0 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

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

Vector and Tensor Calculus

Vector and Tensor Calculus Appendices 58 A Vector and Tensor Calculus In relativistic theory one often encounters vector and tensor expressions in both three- and four-dimensional form. The most important of these expressions 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

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

Lecturer: Bengt E W Nilsson

Lecturer: Bengt E W Nilsson 009 04 8 Lecturer: Bengt E W Nilsson Chapter 3: The closed quantised bosonic string. Generalised τ,σ gauges: n µ. For example n µ =,, 0,, 0).. X ±X ) =0. n x = α n p)τ n p)σ =π 0σ n P τ τ,σ )dσ σ 0, π]

More information

A Brief Introduction to AdS/CFT Correspondence

A Brief Introduction to AdS/CFT Correspondence Department of Physics Universidad de los Andes Bogota, Colombia 2011 Outline of the Talk Outline of the Talk Introduction Outline of the Talk Introduction Motivation Outline of the Talk Introduction Motivation

More information

Wave propagation in electromagnetic systems with a linear response

Wave propagation in electromagnetic systems with a linear response Wave propagation in electromagnetic systems with a linear response Yakov Itin Institute of Mathematics, Hebrew University of Jerusalem and Jerusalem College of Technology GIF4, JCT, Jerusalem October,

More information

Brane Gravity from Bulk Vector Field

Brane Gravity from Bulk Vector Field Brane Gravity from Bulk Vector Field Merab Gogberashvili Andronikashvili Institute of Physics, 6 Tamarashvili Str., Tbilisi 380077, Georgia E-mail: gogber@hotmail.com September 7, 00 Abstract It is shown

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

Théorie des cordes: quelques applications. Cours II: 4 février 2011

Théorie des cordes: quelques applications. Cours II: 4 février 2011 Particules Élémentaires, Gravitation et Cosmologie Année 2010-11 Théorie des cordes: quelques applications Cours II: 4 février 2011 Résumé des cours 2009-10: deuxième partie 04 février 2011 G. Veneziano,

More information

Construction of Field Theories

Construction of Field Theories Physics 411 Lecture 24 Construction of Field Theories Lecture 24 Physics 411 Classical Mechanics II October 29th, 2007 We are beginning our final descent, and I ll take the opportunity to look at the freedom

More information

SUPERSTRING REALIZATIONS OF SUPERGRAVITY IN TEN AND LOWER DIMENSIONS. John H. Schwarz. Dedicated to the memory of Joël Scherk

SUPERSTRING REALIZATIONS OF SUPERGRAVITY IN TEN AND LOWER DIMENSIONS. John H. Schwarz. Dedicated to the memory of Joël Scherk SUPERSTRING REALIZATIONS OF SUPERGRAVITY IN TEN AND LOWER DIMENSIONS John H. Schwarz Dedicated to the memory of Joël Scherk SOME FAMOUS SCHERK PAPERS Dual Models For Nonhadrons J. Scherk, J. H. Schwarz

More information

Physics 411 Lecture 22. E&M and Sources. Lecture 22. Physics 411 Classical Mechanics II

Physics 411 Lecture 22. E&M and Sources. Lecture 22. Physics 411 Classical Mechanics II Physics 411 Lecture 22 E&M and Sources Lecture 22 Physics 411 Classical Mechanics II October 24th, 2007 E&M is a good place to begin talking about sources, since we already know the answer from Maxwell

More information

Supercurrents. Nathan Seiberg IAS

Supercurrents. Nathan Seiberg IAS Supercurrents Nathan Seiberg IAS 2011 Zohar Komargodski and NS arxiv:0904.1159, arxiv:1002.2228 Tom Banks and NS arxiv:1011.5120 Thomas T. Dumitrescu and NS arxiv:1106.0031 Summary The supersymmetry algebra

More information

Quantum Field Theory. Kerson Huang. Second, Revised, and Enlarged Edition WILEY- VCH. From Operators to Path Integrals

Quantum Field Theory. Kerson Huang. Second, Revised, and Enlarged Edition WILEY- VCH. From Operators to Path Integrals Kerson Huang Quantum Field Theory From Operators to Path Integrals Second, Revised, and Enlarged Edition WILEY- VCH WILEY-VCH Verlag GmbH & Co. KGaA I vh Contents Preface XIII 1 Introducing Quantum Fields

More information

BFT embedding of noncommutative D-brane system. Abstract

BFT embedding of noncommutative D-brane system. Abstract SOGANG-HEP 271/00 BFT embedding of noncommutative D-brane system Soon-Tae Hong,WonTaeKim, Young-Jai Park, and Myung Seok Yoon Department of Physics and Basic Science Research Institute, Sogang University,

More information

Solutions to problem set 6

Solutions to problem set 6 Solutions to problem set 6 Donal O Connell February 3, 006 1 Problem 1 (a) The Lorentz transformations are just t = γ(t vx) (1) x = γ(x vt). () In S, the length δx is at the points x = 0 and x = δx for

More information

arxiv:hep-th/ v1 6 Oct 1998

arxiv:hep-th/ v1 6 Oct 1998 DAMTP-1998-137 hep-th/9810041 arxiv:hep-th/9810041v1 6 Oct 1998 On Gauged Maximal Supergravity In Six Dimensions P.M.Cowdall DAMTP, University of Cambridge, Silver Street, Cambridge, U.K. ABSTRACT The

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

Lagrangian. µ = 0 0 E x E y E z 1 E x 0 B z B y 2 E y B z 0 B x 3 E z B y B x 0. field tensor. ν =

Lagrangian. µ = 0 0 E x E y E z 1 E x 0 B z B y 2 E y B z 0 B x 3 E z B y B x 0. field tensor. ν = Lagrangian L = 1 4 F µνf µν j µ A µ where F µν = µ A ν ν A µ = F νµ. F µν = ν = 0 1 2 3 µ = 0 0 E x E y E z 1 E x 0 B z B y 2 E y B z 0 B x 3 E z B y B x 0 field tensor. Note that F µν = g µρ F ρσ g σν

More information

Physics 218 Polarization sum for massless spin-one particles Winter 2016

Physics 218 Polarization sum for massless spin-one particles Winter 2016 Physics 18 Polarization sum for massless spin-one particles Winter 016 We first consider a massless spin-1 particle moving in the z-direction with four-momentum k µ = E(1; 0, 0, 1). The textbook expressions

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

Introduction to relativistic quantum mechanics

Introduction to relativistic quantum mechanics Introduction to relativistic quantum mechanics. Tensor notation In this book, we will most often use so-called natural units, which means that we have set c = and =. Furthermore, a general 4-vector will

More information

e θ 1 4 [σ 1,σ 2 ] = e i θ 2 σ 3

e θ 1 4 [σ 1,σ 2 ] = e i θ 2 σ 3 Fermions Consider the string world sheet. We have bosons X µ (σ,τ) on this world sheet. We will now also put ψ µ (σ,τ) on the world sheet. These fermions are spin objects on the worldsheet. In higher dimensions,

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

Conformal Field Theory with Two Kinds of Bosonic Fields and Two Linear Dilatons

Conformal Field Theory with Two Kinds of Bosonic Fields and Two Linear Dilatons Brazilian Journal of Physics, vol. 40, no. 4, December, 00 375 Conformal Field Theory with Two Kinds of Bosonic Fields and Two Linear Dilatons Davoud Kamani Faculty of Physics, Amirkabir University of

More information

Free totally (anti)symmetric massless fermionic fields in d-dimensional anti-de Sitter space

Free totally (anti)symmetric massless fermionic fields in d-dimensional anti-de Sitter space Free totally (anti)symmetric massless fermionic fields in d-dimensional anti-de Sitter space R. R. Metsaev Department of Theoretical Physics, P. N. Lebedev Physical Institute, Leninsky prospect 53, 11794,

More information

arxiv:hep-th/ v1 28 Jan 1999

arxiv:hep-th/ v1 28 Jan 1999 N=1, D=10 TENSIONLESS SUPERBRANES II. 1 arxiv:hep-th/9901153v1 28 Jan 1999 P. Bozhilov 2 Bogoliubov Laboratory of Theoretical Physics, JINR, 141980 Dubna, Russia We consider a model for tensionless (null)

More information

1 Canonical quantization conformal gauge

1 Canonical quantization conformal gauge Contents 1 Canonical quantization conformal gauge 1.1 Free field space of states............................... 1. Constraints..................................... 3 1..1 VIRASORO ALGEBRA...........................

More information

Rank Three Tensors in Unified Gravitation and Electrodynamics

Rank Three Tensors in Unified Gravitation and Electrodynamics 5 Rank Three Tensors in Unified Gravitation and Electrodynamics by Myron W. Evans, Alpha Institute for Advanced Study, Civil List Scientist. (emyrone@aol.com and www.aias.us) Abstract The role of base

More information

etc., etc. Consequently, the Euler Lagrange equations for the Φ and Φ fields may be written in a manifestly covariant form as L Φ = m 2 Φ, (S.

etc., etc. Consequently, the Euler Lagrange equations for the Φ and Φ fields may be written in a manifestly covariant form as L Φ = m 2 Φ, (S. PHY 396 K. Solutions for problem set #3. Problem 1a: Let s start with the scalar fields Φx and Φ x. Similar to the EM covariant derivatives, the non-abelian covariant derivatives may be integrated by parts

More information

Exercise 1 Classical Bosonic String

Exercise 1 Classical Bosonic String Exercise 1 Classical Bosonic String 1. The Relativistic Particle The action describing a free relativistic point particle of mass m moving in a D- dimensional Minkowski spacetime is described by ) 1 S

More information

Coordinate/Field Duality in Gauge Theories: Emergence of Matrix Coordinates

Coordinate/Field Duality in Gauge Theories: Emergence of Matrix Coordinates Coordinate/Field Duality in Gauge Theories: Emergence of Matrix Coordinates Amir H. Fatollahi Department of Physics, Alzahra University, P. O. Box 19938, Tehran 91167, Iran fath@alzahra.ac.ir Abstract

More information

Spinor Representation of Conformal Group and Gravitational Model

Spinor Representation of Conformal Group and Gravitational Model Spinor Representation of Conformal Group and Gravitational Model Kohzo Nishida ) arxiv:1702.04194v1 [physics.gen-ph] 22 Jan 2017 Department of Physics, Kyoto Sangyo University, Kyoto 603-8555, Japan Abstract

More information

Thick Brane World. Seyen Kouwn Korea Astronomy and Space Science Institute Korea

Thick Brane World. Seyen Kouwn Korea Astronomy and Space Science Institute Korea Thick Brane World Seyen Kouwn Korea Astronomy and Space Science Institute Korea Introduction - Multidimensional theory 1 Why are the physically observed dimensions of our Universe = 3 + 1 (space + time)?

More information

AdS/CFT duality. Agnese Bissi. March 26, Fundamental Problems in Quantum Physics Erice. Mathematical Institute University of Oxford

AdS/CFT duality. Agnese Bissi. March 26, Fundamental Problems in Quantum Physics Erice. Mathematical Institute University of Oxford AdS/CFT duality Agnese Bissi Mathematical Institute University of Oxford March 26, 2015 Fundamental Problems in Quantum Physics Erice What is it about? AdS=Anti de Sitter Maximally symmetric solution of

More information

Theoretical Cosmology and Astrophysics Lecture notes - Chapter 7

Theoretical Cosmology and Astrophysics Lecture notes - Chapter 7 Theoretical Cosmology and Astrophysics Lecture notes - Chapter 7 A. Refregier April 24, 2017 7 Cosmological Perturbations 1 In this chapter, we will consider perturbations to the FRW smooth model of the

More information

Faraday Tensor & Maxwell Spinor (Part I)

Faraday Tensor & Maxwell Spinor (Part I) February 2015 Volume 6 Issue 2 pp. 88-97 Faraday Tensor & Maxwell Spinor (Part I) A. Hernández-Galeana #, R. López-Vázquez #, J. López-Bonilla * & G. R. Pérez-Teruel & 88 Article # Escuela Superior de

More information

Week 1, solution to exercise 2

Week 1, solution to exercise 2 Week 1, solution to exercise 2 I. THE ACTION FOR CLASSICAL ELECTRODYNAMICS A. Maxwell s equations in relativistic form Maxwell s equations in vacuum and in natural units (c = 1) are, E=ρ, B t E=j (inhomogeneous),

More information

Exact solutions in supergravity

Exact solutions in supergravity Exact solutions in supergravity James T. Liu 25 July 2005 Lecture 1: Introduction and overview of supergravity Lecture 2: Conditions for unbroken supersymmetry Lecture 3: BPS black holes and branes Lecture

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

String Theory and The Velo-Zwanziger Problem

String Theory and The Velo-Zwanziger Problem String Theory and The Velo-Zwanziger Problem Rakibur Rahman Scuola Normale Superiore & INFN, Pisa February 10, 2011 DAMTP, University of Cambridge M. Porrati A. Sagnotti M. Porrati, RR and A. Sagnotti,

More information

Notes on General Relativity Linearized Gravity and Gravitational waves

Notes on General Relativity Linearized Gravity and Gravitational waves Notes on General Relativity Linearized Gravity and Gravitational waves August Geelmuyden Universitetet i Oslo I. Perturbation theory Solving the Einstein equation for the spacetime metric is tremendously

More information

Cartesian Tensors. e 2. e 1. General vector (formal definition to follow) denoted by components

Cartesian Tensors. e 2. e 1. General vector (formal definition to follow) denoted by components Cartesian Tensors Reference: Jeffreys Cartesian Tensors 1 Coordinates and Vectors z x 3 e 3 y x 2 e 2 e 1 x x 1 Coordinates x i, i 123,, Unit vectors: e i, i 123,, General vector (formal definition to

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

Lecturer: Bengt E W Nilsson

Lecturer: Bengt E W Nilsson 2009 05 07 Lecturer: Bengt E W Nilsson From the previous lecture: Example 3 Figure 1. Some x µ s will have ND or DN boundary condition half integer mode expansions! Recall also: Half integer mode expansions

More information

String theory triplets and higher-spin curvatures

String theory triplets and higher-spin curvatures String theory triplets and higher-spin curvatures Dario Francia Institute of Physics - Academy of Sciences of the Czech Republic SFT2010 YITP Kyoto October 19th, 2010 based on: D. F. J.Phys. Conf. Ser.

More information

Tachyon Condensation in String Theory and Field Theory

Tachyon Condensation in String Theory and Field Theory Tachyon Condensation in String Theory and Field Theory N.D. Lambert 1 and I. Sachs 2 1 Dept. of Physics and Astronomy Rutgers University Piscataway, NJ 08855 USA nlambert@physics.rutgers.edu 2 School of

More information

The boundary state from open string fields. Yuji Okawa University of Tokyo, Komaba. March 9, 2009 at Nagoya

The boundary state from open string fields. Yuji Okawa University of Tokyo, Komaba. March 9, 2009 at Nagoya The boundary state from open string fields Yuji Okawa University of Tokyo, Komaba March 9, 2009 at Nagoya Based on arxiv:0810.1737 in collaboration with Kiermaier and Zwiebach (MIT) 1 1. Introduction Quantum

More information

One Loop Tests of Higher Spin AdS/CFT

One Loop Tests of Higher Spin AdS/CFT One Loop Tests of Higher Spin AdS/CFT Simone Giombi UNC-Chapel Hill, Jan. 30 2014 Based on 1308.2337 with I. Klebanov and 1401.0825 with I. Klebanov and B. Safdi Massless higher spins Consistent interactions

More information

A Comment on String Solitons

A Comment on String Solitons CTP/TAMU-18/93 A Comment on String Solitons arxiv:hep-th/9305143v1 26 May 1993 Ramzi R. Khuri Center for Theoretical Physics Texas A&M University College Station, TX 77843 We derive an exact string-like

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

γγ αβ α X µ β X µ (1)

γγ αβ α X µ β X µ (1) Week 3 Reading material from the books Zwiebach, Chapter 12, 13, 21 Polchinski, Chapter 1 Becker, Becker, Schwartz, Chapter 2 Green, Schwartz, Witten, chapter 2 1 Polyakov action We have found already

More information

Generalizations of Yang Mills theory with nonlinear constitutive equations

Generalizations of Yang Mills theory with nonlinear constitutive equations INSTITUTE OF PHYSICS PUBLISHING JOURNAL OF PHYSICS A: MATHEMATICAL AND GENERAL J. Phys. A: Math. Gen. 37 (2004) 10711 10718 PII: S0305-4470(04)79205-7 Generalizations of Yang Mills theory with nonlinear

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

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

We start by recalling electrodynamics which is the first classical field theory most of us have encountered in theoretical physics.

We start by recalling electrodynamics which is the first classical field theory most of us have encountered in theoretical physics. Quantum Field Theory I ETH Zurich, HS12 Chapter 6 Prof. N. Beisert 6 Free Vector Field Next we want to find a formulation for vector fields. This includes the important case of the electromagnetic field

More information

Regularization Physics 230A, Spring 2007, Hitoshi Murayama

Regularization Physics 230A, Spring 2007, Hitoshi Murayama Regularization Physics 3A, Spring 7, Hitoshi Murayama Introduction In quantum field theories, we encounter many apparent divergences. Of course all physical quantities are finite, and therefore divergences

More information

Cosmological solutions of Double field theory

Cosmological solutions of Double field theory Cosmological solutions of Double field theory Haitang Yang Center for Theoretical Physics Sichuan University USTC, Oct. 2013 1 / 28 Outlines 1 Quick review of double field theory 2 Duality Symmetries in

More information

Wound String Scattering in NCOS Theory

Wound String Scattering in NCOS Theory UUITP-09/00 hep-th/0005 Wound String Scattering in NCOS Theory Fredric Kristiansson and Peter Rajan Institutionen för Teoretisk Fysik, Box 803, SE-75 08 Uppsala, Sweden fredric.kristiansson@teorfys.uu.se,

More information

Topological DBI actions and nonlinear instantons

Topological DBI actions and nonlinear instantons 8 November 00 Physics Letters B 50 00) 70 7 www.elsevier.com/locate/npe Topological DBI actions and nonlinear instantons A. Imaanpur Department of Physics, School of Sciences, Tarbiat Modares University,

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

Light-Cone Fields and Particles

Light-Cone Fields and Particles Chapter 10 Light-Cone Fields and Particles We study the classical equations of motion for scalar fields, Maxwell fields, and gravitational fields. We use the light-cone gauge to find plane-wave solutions

More information

Quantum Field Theory Notes. Ryan D. Reece

Quantum Field Theory Notes. Ryan D. Reece Quantum Field Theory Notes Ryan D. Reece November 27, 2007 Chapter 1 Preliminaries 1.1 Overview of Special Relativity 1.1.1 Lorentz Boosts Searches in the later part 19th century for the coordinate transformation

More information

ds/cft Contents Lecturer: Prof. Juan Maldacena Transcriber: Alexander Chen August 7, Lecture Lecture 2 5

ds/cft Contents Lecturer: Prof. Juan Maldacena Transcriber: Alexander Chen August 7, Lecture Lecture 2 5 ds/cft Lecturer: Prof. Juan Maldacena Transcriber: Alexander Chen August 7, 2011 Contents 1 Lecture 1 2 2 Lecture 2 5 1 ds/cft Lecture 1 1 Lecture 1 We will first review calculation of quantum field theory

More information

Higher-Spin Fermionic Gauge Fields & Their Electromagnetic Coupling

Higher-Spin Fermionic Gauge Fields & Their Electromagnetic Coupling Higher-Spin Fermionic Gauge Fields & Their Electromagnetic Coupling Rakibur Rahman Université Libre de Bruxelles, Belgium April 18, 2012 ESI Workshop on Higher Spin Gravity Erwin Schrödinger Institute,

More information

Stress-energy tensor is the most important object in a field theory and have been studied

Stress-energy tensor is the most important object in a field theory and have been studied Chapter 1 Introduction Stress-energy tensor is the most important object in a field theory and have been studied extensively [1-6]. In particular, the finiteness of stress-energy tensor has received great

More information

Geons in Asymptotically Anti-de Sitter spacetimes

Geons in Asymptotically Anti-de Sitter spacetimes Geons in Asymptotically Anti-de Sitter spacetimes Grégoire Martinon in collaboration with Gyula Fodor Philippe Grandclément Observatoire de Paris Université Paris Diderot 6 Juillet 2016 Grégoire Martinon

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

Conservation Theorem of Einstein Cartan Evans Field Theory

Conservation Theorem of Einstein Cartan Evans Field Theory 28 Conservation Theorem of Einstein Cartan Evans Field Theory by Myron W. Evans, Alpha Institute for Advanced Study, Civil List Scientist. (emyrone@aol.com and www.aias.us) Abstract The conservation theorems

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

TOPIC IV STRING THEORY

TOPIC IV STRING THEORY TOPIC IV STRING THEORY General relativity is a beautiful, complete theory of gravity. It agrees well with observations. For example it predicts the correct precession of the orbit of Mercury, and its prediction

More information

Applications of AdS/CFT correspondence to cold atom physics

Applications of AdS/CFT correspondence to cold atom physics Applications of AdS/CFT correspondence to cold atom physics Sergej Moroz in collaboration with Carlos Fuertes ITP, Heidelberg Outline Basics of AdS/CFT correspondence Schrödinger group and correlation

More information

A Short Note on D=3 N=1 Supergravity

A Short Note on D=3 N=1 Supergravity A Short Note on D=3 N=1 Supergravity Sunny Guha December 13, 015 1 Why 3-dimensional gravity? Three-dimensional field theories have a number of unique features, the massless states do not carry helicity,

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

q form field and Hodge duality on brane

q form field and Hodge duality on brane Lanzhou University (=²ŒÆ) With C.E. Fu, H. Guo and S.L. Zhang [PRD 93 (206) 064007] 4th International Workshop on Dark Matter, Dark Energy and Matter-Antimatter Asymmetry December 29-3, 206, December 3,

More information

D-Branes at Finite Temperature in TFD

D-Branes at Finite Temperature in TFD D-Branes at Finite Temperature in TFD arxiv:hep-th/0308114v1 18 Aug 2003 M. C. B. Abdalla a, A. L. Gadelha a, I. V. Vancea b January 8, 2014 a Instituto de Física Teórica, Universidade Estadual Paulista

More information

PHYS 4390: GENERAL RELATIVITY NON-COORDINATE BASIS APPROACH

PHYS 4390: GENERAL RELATIVITY NON-COORDINATE BASIS APPROACH PHYS 4390: GENERAL RELATIVITY NON-COORDINATE BASIS APPROACH 1. Differential Forms To start our discussion, we will define a special class of type (0,r) tensors: Definition 1.1. A differential form of order

More information

arxiv:hep-th/ v1 21 Apr 1995

arxiv:hep-th/ v1 21 Apr 1995 CERN-TH/95-78 arxiv:hep-th/950408v 2 Apr 995 A GAS OF D-INSTANTONS Michael B. Green, Theory Division, CERN, CH-2, Geneva 23, Switzerland ABSTRACT A D-instanton is a space-time event associated with world-sheet

More information

Gauge Theory of Gravitation: Electro-Gravity Mixing

Gauge Theory of Gravitation: Electro-Gravity Mixing Gauge Theory of Gravitation: Electro-Gravity Mixing E. Sánchez-Sastre 1,2, V. Aldaya 1,3 1 Instituto de Astrofisica de Andalucía, Granada, Spain 2 Email: sastre@iaa.es, es-sastre@hotmail.com 3 Email: valdaya@iaa.es

More information

Continuity Equations and the Energy-Momentum Tensor

Continuity Equations and the Energy-Momentum Tensor Physics 4 Lecture 8 Continuity Equations and the Energy-Momentum Tensor Lecture 8 Physics 4 Classical Mechanics II October 8th, 007 We have finished the definition of Lagrange density for a generic space-time

More information

Quantum Field Theory Example Sheet 4 Michelmas Term 2011

Quantum Field Theory Example Sheet 4 Michelmas Term 2011 Quantum Field Theory Example Sheet 4 Michelmas Term 0 Solutions by: Johannes Hofmann Laurence Perreault Levasseur Dave M. Morris Marcel Schmittfull jbh38@cam.ac.uk L.Perreault-Levasseur@damtp.cam.ac.uk

More information

Théorie des cordes: quelques applications. Cours IV: 11 février 2011

Théorie des cordes: quelques applications. Cours IV: 11 février 2011 Particules Élémentaires, Gravitation et Cosmologie Année 2010-11 Théorie des cordes: quelques applications Cours IV: 11 février 2011 Résumé des cours 2009-10: quatrième partie 11 février 2011 G. Veneziano,

More information

8.821 String Theory Fall 2008

8.821 String Theory Fall 2008 MIT OpenCourseWare http://ocw.mit.edu 8.8 String Theory Fall 008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 8.8 F008 Lecture 0: CFTs in D > Lecturer:

More information

Tutorial 5 Clifford Algebra and so(n)

Tutorial 5 Clifford Algebra and so(n) Tutorial 5 Clifford Algebra and so(n) 1 Definition of Clifford Algebra A set of N Hermitian matrices γ 1, γ,..., γ N obeying the anti-commutator γ i, γ j } = δ ij I (1) is the basis for an algebra called

More information

Exercises Symmetries in Particle Physics

Exercises Symmetries in Particle Physics Exercises Symmetries in Particle Physics 1. A particle is moving in an external field. Which components of the momentum p and the angular momentum L are conserved? a) Field of an infinite homogeneous plane.

More information

Spinning strings and QED

Spinning strings and QED Spinning strings and QED James Edwards Oxford Particles and Fields Seminar January 2015 Based on arxiv:1409.4948 [hep-th] and arxiv:1410.3288 [hep-th] Outline Introduction Various relationships between

More information

1.7 Plane-wave Solutions of the Dirac Equation

1.7 Plane-wave Solutions of the Dirac Equation 0 Version of February 7, 005 CHAPTER. DIRAC EQUATION It is evident that W µ is translationally invariant, [P µ, W ν ] 0. W is a Lorentz scalar, [J µν, W ], as you will explicitly show in homework. Here

More information

Scalar Fields and Gauge

Scalar Fields and Gauge Physics 411 Lecture 23 Scalar Fields and Gauge Lecture 23 Physics 411 Classical Mechanics II October 26th, 2007 We will discuss the use of multiple fields to expand our notion of symmetries and conservation.

More information

Chapter 2: Deriving AdS/CFT

Chapter 2: Deriving AdS/CFT Chapter 8.8/8.87 Holographic Duality Fall 04 Chapter : Deriving AdS/CFT MIT OpenCourseWare Lecture Notes Hong Liu, Fall 04 Lecture 0 In this chapter, we will focus on:. The spectrum of closed and open

More information

TOPIC VII ADS/CFT DUALITY

TOPIC VII ADS/CFT DUALITY TOPIC VII ADS/CFT DUALITY The conjecture of AdS/CFT duality marked an important step in the development of string theory. Quantum gravity is expected to be a very complicated theory. String theory provides

More information

Übungen zur Elektrodynamik (T3)

Übungen zur Elektrodynamik (T3) Arnold Sommerfeld Center Ludwig Maximilians Universität München Prof. Dr. Ivo Sachs SoSe 08 Übungen zur Elektrodynamik (T3) Lösungen zum Übungsblatt 7 Lorentz Force Calculate dx µ and ds explicitly in

More information

1 Covariant quantization of the Bosonic string

1 Covariant quantization of the Bosonic string Covariant quantization of the Bosonic string The solution of the classical string equations of motion for the open string is X µ (σ) = x µ + α p µ σ 0 + i α n 0 where (α µ n) = α µ n.and the non-vanishing

More information

Massive gravitons in arbitrary spacetimes

Massive gravitons in arbitrary spacetimes Massive gravitons in arbitrary spacetimes Mikhail S. Volkov LMPT, University of Tours, FRANCE Kyoto, YITP, Gravity and Cosmology Workshop, 6-th February 2018 C.Mazuet and M.S.V., Phys.Rev. D96, 124023

More information

Parity P : x x, t t, (1.116a) Time reversal T : x x, t t. (1.116b)

Parity P : x x, t t, (1.116a) Time reversal T : x x, t t. (1.116b) 4 Version of February 4, 005 CHAPTER. DIRAC EQUATION (0, 0) is a scalar. (/, 0) is a left-handed spinor. (0, /) is a right-handed spinor. (/, /) is a vector. Before discussing spinors in detail, let us

More information

Dirac Equation with Self Interaction Induced by Torsion

Dirac Equation with Self Interaction Induced by Torsion Advanced Studies in Theoretical Physics Vol. 9, 2015, no. 12, 587-594 HIKARI Ltd, www.m-hikari.com http://dx.doi.org/10.12988/astp.2015.5773 Dirac Equation with Self Interaction Induced by Torsion Antonio

More information

Quantization of the open string on exact plane waves and non-commutative wave fronts

Quantization of the open string on exact plane waves and non-commutative wave fronts Quantization of the open string on exact plane waves and non-commutative wave fronts F. Ruiz Ruiz (UCM Madrid) Miami 2007, December 13-18 arxiv:0711.2991 [hep-th], with G. Horcajada Motivation On-going

More information

This document is downloaded from DR-NTU, Nanyang Technological University Library, Singapore.

This document is downloaded from DR-NTU, Nanyang Technological University Library, Singapore. This document is downloaded from DR-NTU, Nanyang Technological University Library, Singapore. Title A doubled discretization of Abelian Chern-Simons theory Author(s) Adams, David H. Citation Adams, D.

More information

MIFPA PiTP Lectures. Katrin Becker 1. Department of Physics, Texas A&M University, College Station, TX 77843, USA. 1

MIFPA PiTP Lectures. Katrin Becker 1. Department of Physics, Texas A&M University, College Station, TX 77843, USA. 1 MIFPA-10-34 PiTP Lectures Katrin Becker 1 Department of Physics, Texas A&M University, College Station, TX 77843, USA 1 kbecker@physics.tamu.edu Contents 1 Introduction 2 2 String duality 3 2.1 T-duality

More information

Non-associative Deformations of Geometry in Double Field Theory

Non-associative Deformations of Geometry in Double Field Theory Non-associative Deformations of Geometry in Double Field Theory Michael Fuchs Workshop Frontiers in String Phenomenology based on JHEP 04(2014)141 or arxiv:1312.0719 by R. Blumenhagen, MF, F. Haßler, D.

More information