Open String Tachyon in Supergravity Solution

Slides:



Advertisements
Similar presentations
Based on arXiv:1107.xxxx with G. Mandal (TIFR) What is the gravity dual of the confinement/deconfinement transportation in holographic QCD Takeshi Morita.
Advertisements

Brane-World Inflation
Summing planar diagrams
Construction of BPS Solitons via Tachyon Condensation So RIKEN based on the work with T. Asakawa and K. Ohta hep-th/0603***
String Theory A picture book.
Solitons in Matrix model and DBI action Seiji Terashima (YITP, Kyoto U.) at KEK March 14, 2007 Based on hep-th/ , and hep-th/ ,
Holographic Superconductors with Higher Curvature Corrections Sugumi Kanno (Durham) work w/ Ruth Gregory (Durham) Jiro Soda (Kyoto) arXiv: , to.
Making Precise the Nothing at the Beginning of the Universe Yu Nakayama, hep-th/ (Collaboration with S.J. Rey, Y. Sugawara)
Intersecting membrane and an anisotropic models of dark energy Dmitry G. Orlov (NCU, Taiwan; VNIIMS, Russia) 1st June, 2008NDHU, Taiwan.
ASYMPTOTIC STRUCTURE IN HIGHER DIMENSIONS AND ITS CLASSIFICATION KENTARO TANABE (UNIVERSITY OF BARCELONA) based on KT, Kinoshita and Shiromizu PRD
Giant Magnon and Spike Solutions in String Theories Bum-Hoon Lee Center for Quantum SpaceTime(CQUeST)/Physics Dept. Sogang University, Seoul, Korea PAQFT08,
U(1) Breakdown in Super Yang-Mills and Cascade of Gregory-Laflamme Transitions Masanori Hanada (RIKEN) With Tatsuma Nishioka (Kyoto U., D1 ) Weizmann inst.
Unruh effect and Holography
Extremal Single-charge Small Black holes Aninda Sinha DAMTP, Cambridge University, UK hep-th/ (to appear in CQG) with Nemani Suryanarayana(Perimeter),
3rd International Workshop On High Energy Physics In The LHC Era.
E. Rakhmetov, S. Keyzerov SINP MSU, Moscow QFTHEP 2011, September, Luchezarny, Russia.
Supersymmetry and Gauge Symmetry Breaking from Intersecting Branes A. Giveon, D.K. hep-th/
Shan-Shan Xu University of Science and Technology of China Remarks on Dp & Dp−2 with each carrying a flux Interdisciplinary Center for Theoretical Study.
Elcio Abdalla Perturbations around Black Hole solutions.
AdS/CFT-QCD-CMT Yi NTHU April 8 th, 2010.
Coupled Dark Energy and Dark Matter from dilatation symmetry.
Planar diagrams in light-cone gauge hep-th/ M. Kruczenski Purdue University Based on:
Equations of state and compact stars in gauge/gravity duality
Dynamical solutions in intersecting brane systems Kunihito Uzawa Osaka City University Advanced Mathematical Institute.
Holographic Description of Quantum Black Hole on a Computer Yoshifumi Hyakutake (Ibaraki Univ.) Collaboration with M. Hanada ( YITP, Kyoto ), G. Ishiki.
Emergent Universe Scenario
Rolling D-brane in Lorentzian 2D-black Yu Nakayama, S. J. Rey and Y. Sugawara hep-th/ , JHEP09(2005)020 hep-th/ , JHEP08(2006)014.
Boundary States and Black p-branes Shinpei Kobayashi ( RESCEU ) in collaboration with Tsuguhiko Asakawa (RIKEN) Tsuguhiko Asakawa (RIKEN) So Matsuura (RIKEN)
Stabilizing moduli with flux in brane gas cosmology Jin Young Kim (Kunsan National Univ.) CosPA 2009, Melbourne Based on arXiv: [hep-th]; PRD 78,
String solitons in the M5-brane worldvolume with a Nambu-Poisson structure and Seiberg-Witten map Tomohisa Takimi (NTU) Ref ) Kazuyuki Furuuchi, T.T JHEP08(2009)050.
Black Holes, Entropy, and Information Gary Horowitz UCSB.
“Einstein Gravity in Higher Dimensions”, Jerusalem, Feb., 2007.
“Models of Gravity in Higher Dimensions”, Bremen, Aug , 2008.
A New Endpoint for Hawking Evaporation Gary Horowitz UCSB hep-th/ Gary Horowitz UCSB hep-th/
Gaussian Brane and Open String Tachyon Condensation Shinpei Kobayashi ( RESCEU, The University of Tokyo ) Tateyama, Chiba Yoshiaki Himemoto.
Brane Gravity and Cosmological Constant Tetsuya Shiromizu Tokyo Institute of Technology Tokyo Institute of Technology 白水 White Water.
Localization of gravity on Higgs vortices with B. de Carlos Jesús M. Moreno IFT Madrid Hanoi, August 7th hep-th/
Domain-wall/QFT correspondence Wen-Yu Wen Academia Sinica Feb 24, 2006 A Bridge Connecting Gravity and Gauge Theory.
Matrix Cosmology Miao Li Institute of Theoretical Physics Chinese Academy of Science.
Hawking radiation for a Proca field Mengjie Wang (王梦杰 ) In collaboration with Carlos Herdeiro & Marco Sampaio Mengjie Wang 王梦杰 Based on: PRD85(2012)
Schwarzschild Radius and Black Hole Thermodynamics with Corrections from Simulations of SUSY Matrix Quantum Mechanics Talk at “Black Holes and Quantum.
GASYUKU2002,Kyoto-U @ KAGA 1 Computing Feynman Graphs in MSFT Isao Kishimoto (Univ. of Tokyo) based on Collaboration with I.Bars and Y.Matsuo [ hep-th/ ]
Black holes sourced by a massless scalar KSM2105, FRANKFURT July, 21th 2015 M. Cadoni, University of Cagliari We construct asymptotically flat black hole.
Brane-Antibrane at Finite Temperature in the Framework of Thermo Field Dynamics Hokkaido Univ. Kenji Hotta.
Introduction to Strings Yoshihisa Kitazawa KEK Nasu lecture 9/25/06.
STRING FIELD THEORY EFFECTIVE ACTION FORTHE TACHYON AND GAUGE FIELDS FOR THE TACHYON AND GAUGE FIELDS secondo incontro del P.R.I.N. “TEORIA DEI CAMPI SUPERSTRINGHE.
Higher spin AdS 3 holography and superstring theory Yasuaki Hikida (Rikkyo University) Based on collaborations with T. Creutzig (U. of Alberta) & P. B.
Simulating Superstrings inside a Black Hole Nov.1, ’08, RIKEN workshop “New Developments in Gauge Theory Driven by Numerical Simulation” Jun Nishimura.
Heidelberg, June 2008 Volker Schomerus - DESY Hamburg - Of Mesons and Metals – Bethe & the 5th Dimension.
Precision test of the gauge/gravity duality from first principles IPMU Focus Week “Condensed Matter Physics Meets High Energy Physics”, IPMU, Univ. of.
알기 쉬운 초끈 이론 박 재모 (Postech). Outline 1. Partcle physics 2. Black holes 3. String theory 4. M theory 5. D branes 6. Gauge/Gravity theory correspondence.
Yoshinori Matsuo (KEK) in collaboration with Hikaru Kawai (Kyoto U.) Yuki Yokokura (Kyoto U.)
On String Theory Duals of Lifshitz-like Fixed Point Tatsuo Azeyanagi (Kyoto University) Based on work arXiv: (to appear in JHEP) with Wei Li (IPMU)
Creation of D9-brane — anti-D9-brane Pairs from Hagedorn Transition of Closed Strings Hokkaido Univ. Kenji Hotta.
Heavy quarkonia in AdS/QCD Y. Kim (KIAS) YK, J.-P. Lee, S. H. Lee, Phys. Rev. D75:114008, YK, B.-H. Lee, C. Park, and S.-J. Sin, hep-th/
Univ.1 Idempotency Equation and Boundary States in Closed String Field Theory Isao Kishimoto (Univ. of Tokyo → KEK) Collaboration.
Microscopic entropy of black holes : a two-dimensional approach M. Cadoni, Capri 2004 Abstract Two-dimensional gravity models allow in many situations.
Holographic Description of Quantum Black Hole on a Computer Yoshifumi Hyakutake (Ibaraki Univ.) Collaboration with M. Hanada ( YITP, Kyoto ), G. Ishiki.
B.-H.L, R. Nayak, K. Panigrahi, C. Park On the giant magnon and spike solutions for strings on AdS(3) x S**3. JHEP 0806:065,2008. arXiv: J. Kluson,
Collider Signals of Extra Dimension Scenarios
Innermost stable circular orbits around squashed Kaluza-Klein black holes Ken Matsuno & Hideki Ishihara ( Osaka City University ) 1.
Ramond-Ramond Couplings of D-branes Collaborators: Koji Hashimoto (Osaka Univ.) Seiji Terashima (YITP Kyoto) Sotaro Sugishita (Kyoto Univ.) JHEP1503(2015)077.
Gauge/gravity duality in Einstein-dilaton theory Chanyong Park Workshop on String theory and cosmology (Pusan, ) Ref. S. Kulkarni,
Bum-Hoon Lee Sogang University, Seoul, Korea D-branes in Type IIB Plane Wave Background 15th Mini-Workshop on Particle Physics May 14-15, 2006, Seoul National.
ADHM is a Tachyon Condensation --- Stringy Derivation of the ADHM Construction --- Koji Hashimoto (U. of Tokyo, Komaba) 30 Oct Hawaii meeting hep-th/ ,
Dept.of Physics & Astrophysics
A rotating hairy BH in AdS_3
Charged black holes in string-inspired gravity models
Gravity from Entanglement and RG Flow
Hysteresis Curves from 11 dimensions
Presentation transcript:

Open String Tachyon in Supergravity Solution Shinpei Kobayashi ( Research Center for the Early Universe, The University of Tokyo ) Based on hep-th/0409044 in collaboration with Tsuguhiko Asakawa and So Matsuura ( RIKEN ) 2005/01/18 at KEK

Motivation We would like to apply the string theory to the analyses of the gravitational systems. We have to know how we should apply string theory to realistic gravitational systems, or what stringy (non-perturbative) effects are, or what stringy counterparts of the BHs or Universe in the general relativity are. → D-branes may be a clue to tackle such problems (BH entropy, D-brane inflation, etc.)

Contents D-branes and Classical Descriptions D/anti D-brane system Three-parameter solution Conclusions Discussions and Future Works

1. D-branes and Classical descriptions String Field Theory Supergravity low energy limit α’ → 0 classical description ( Black p-brane ) low energy limit D-brane ( Boundary State )

D-brane ( BPS case ) Open string endpoints stick to a D-brane Properties SO(1,p)×SO(9-p) ( BPS case ), RR-charged (mass)  1/(string coupling) Dp-brane X0 Xμ Xi open string

BPS black p-brane solution Symmetry : SO(1,p)×SO(9-p), RR-charged setup : SUGRA action ansatz :

BPS black p-brane solution (D=10) ・ SO(1,p)×SO(9-p), ・ (mass)=(RR-charge), which are the same as D-branes it must be large for the validity of SUGRA Di Vecchia et al. suggested more direct method to check the correspondence between a Dp-brane and a black p-brane solution using the boundary state.

coincide Relation between the D-brane ( the boundary state) and the black p-brane solution (Di Vecchia et al. (1997)) asymptotic behavior of the black p-brane = difference from the flat background = graviton, dilaton, RR-potential in SUGRA massless modes of the closed strings from the boundary state ( D-brane in closed string channel ) = graviton, dilaton, RR-potential in string theory ( string field theory ) coincide

Boundary State ( = D-brane) Boundary states are defined as sources of closed strings ( = D-branes in closed string channel ). As closed strings include gravitons, the boundary state directly relates to a black p-brane solution.

e.g. ) asymptotic behavior of Φ of black p-brane leading term at infinity coincident <B|  |φ> We can reproduce the leading term of a black p-brane solution ( asymptotic behavior ) via the boundary state.

String Field Theory Supergravity eom eom D-brane ( Boundary State ) low energy limit α’ → 0 eom eom D-brane ( Boundary State ) classical solution ( Black p-brane ) low energy limit BPS case → OK (Di Vecchia et al. (1997)) non-BPS case → ? We study non-BPS systems ( e.g. D/anti D-brane system ). non-BPS cases are more realistic in GR sense

We verify their claim using the boundary state. BPS case Dp-brane    black p-brane Non-BPS case D/anti D-brane system with a constant tachyon vev Three-parameter solution ? ( guessed by Brax-Mandal-Oz (2000)) ( other non-BPS system corresponding classical solution ?) We verify their claim using the boundary state.

2. D/anti D-brane system tachyon condensation closed string emission D-branes and anti D-branes attracts together Unstable multiple branes Open string tachyon represents its instability Stable D-branes are left   case 

Boundary State with boundary interaction

open string

Boundary state for D/anti D-brane with a constant tachyon vev RR-charge mass

Change of the Mass during the tachyon condensation D-branes,   anti D-branes coincide with each other. ( t = 0 )   During the tachyon condensation ( t = t0 ) tachyon vev is included in the mass. Final state ( t = ∞ ) The mass will decrease through the closed string emission, and the value of the mass will coincide with that of the RR-charge (BPS).

Boundary state for D/anti D-brane constant tachyon RR-charge mass

3. Three-parameter solution ( Zhou & Zhu (1999) ) SUGRA action ansatz : SO(1, p)×SO(9-p) ( D=10 ) same symmetry as the D/anti D-brane system

tachyon vev ? charge ? mass ?

Property of the three-parameter solution ADM mass RR charge We can extend it to an arbitrary dimensionality. We re-examine the correspondence between the D/anti D-brane system and the three-parameter solution using the boundary state. ~ ? ~ ? From the form of the boundary state, Brax-Mandal-Oz claimed that c_1 corresponds to the tachyon vev.

New parametrization   → During the tachyon condensation, the RR-charge does not change its value. → We need a new parametrization suitable for t.c.

Asymptotic behavior of the three-parameter solution (= graviton, dilaton, RR-potential in SUGRA )

graviton, dilaton, RR-potential in string theory <B|  |physical field>

Using the boundary state, we obtain

Results and Comparison asymptotic behavior of the three-parameter solution massless modes via the boundary state

Results and Comparison asymptotic behavior of the three-parameter solution massless modes via the boundary state

We find that they coincide with each other under the following identification, RR-charge, constant during the tachyon condensation v ^2 ~ M^2 – Q^2 : non-extremality → tachyon vev can be seen as a part of the ADM mass c_1 does not corresponds to the vev of the open string tachyon. The three-parameter solution with c_1=0 does correspond to the D/anti D-brane system.

Conclusions Using the boundary state, we find that the three-parameter solution with c_1=0 corresponds to the D/anti D-brane system with a constant tachyon vev. New parametrization is needed to keep the RR-charge constant during the tachyon condensation. The vev of the open string tachyon is only seen as a part of the ADM mass. c_1 does not corresponds to the tachyon vev as opposed to the proposal made so far. We find that we can extend the correspondence between D-branes and classical solutions to non-BPS case. First discovery of the correspondence in non-BPS case. It may be a clue to describe “realistic” gravitational systems which are generally non-BPS.

Discussion : Why was c_1 thought to be the open string tachyon vev ? Parametrization → during the t.c., the RR-charge does not change its value. → The relation between the mass and the scalar charge → cf. Wyman solution in D=4 case c_1 corresponds to the dilaton charge.

Wyman solution in Schwarzschild gauge Static, spherically symmetric, with a free scalar

Wyman solution in isotropic gauge r → R In this gauge, we can compare it with the 3-para. sln.

Three-parameter solution case   corresponds to the dilaton charge.

Discussion : Stringy counterpart of c_1 ? has something to do with the -brane. We can not relate these parts with an ordinary boundary state counterpart of the D/anti D-brane system

We can not relate these parts with an ordinary boundary state counterpart of the D/anti D-brane system

Do we have such a deformation in string theory ? Deformation of the boundary state Do we have such a deformation in string theory ? →    with open string tachyon We can reproduce the 3-para. sln with non-zero by adjusting α・β

Construction of (Asakawa-Sugimoto-Terashima, JHEP 0302 (2003) 011) boundary interaction

→ordinary boundary state δ-function with t → ∞ →ordinary boundary state

From Gaussian Boundary State to BPS Dp-brane lower-dimensional BPS D-brane t → ∞ tachyon has some configuration

-direction infinitely extend to -direction infinitely Gaussian in -direction localized at

Consider that each or is made from So far, we treat          Consider that each   or is made from boundary state is deformed as follows: ordinary Deformed origin Gaussian brane origin

Gaussian boundary state D9-tachyon Mixture of Neumann b.c. and Dirichlet b.c. → smeared boundary condition

Oscillator picture boundary condition in the oscillator picture

cf. ordinary boundary state open string σ τ closed string closed tree graph τ σ boundary state D-brane open 1-loop graph

boundary conditions Longitudinal to the D-brane Transverse to the D-brane

Gaussian boundary state case ・ Longitudinal to the Dp-brane ・Transverse to the Dp-brane

Oscillator part 0-mode part combine them to ordinary boundary state with t→∞ combine them

thus, in the limit (D9-tachyon vanishes) tension part via SFT (Kraus-Larsen, PRD63 (2001) 106004) From a to one thus, in the limit (D9-tachyon vanishes)

integrate with finite finally, we obtain origin Gaussian brane origin

     tachyon origin      tachyon origin

graviton, dilaton via Gaussian boundary state

graviton, dilaton via three-parameter solution

constant criterion : RR charge Q keeps its value

Thus, we compare them as → The effect of can be interpreted as D9-tachyon t.

Future Work c_1 and a Gaussian brane (SK, Asakawa & Matsuura, hep-th/0502XXX ) Entropy counting via non-BPS boundary state Construction of a time-dependent solution feedback to SFT Solving δB|B>=0 ( E-M conservation law in SFT ) (Asakawa, SK & Matsuura, JHEP 0310 (2003) 023) Application to cosmology (SK, K. Takahashi & Himemoto) Stability analysis ( K. Takahashi & SK)