A causal alternative to the c=0 string Jan AmbjornNiels Bohr and Univ. Utrecht W.W.Univ. Of Iceland Stefan Zohren Imperial College London Renate LollUniv.

Slides:



Advertisements
Similar presentations
Stokes Phenomena and Non-perturbative Completion in the multi-cut matrix models Hirotaka Irie (NTU) A collaboration with Chuan-Tsung Chan (THU) and Chi-Hsien.
Advertisements

Theories of gravity in 5D brane-world scenarios
Brane-World Inflation
Cosmic Billiards are fully integrable: Tits Satake projections and Kac Moody extensions Talk by Pietro Frè at Corfu 2005”
A journey inside planar pure QED CP3 lunch meeting By Bruno Bertrand November 19 th 2004.
Lattice Spinor Gravity Lattice Spinor Gravity. Quantum gravity Quantum field theory Quantum field theory Functional integral formulation Functional integral.
A causal alternative to the c=0 string Jan AmbjornNiels Bohr and Univ. Utrecht Willem Westra Univ. Of Iceland Stefan Zohren Imperial College London Renate.
Gerard ’t Hooft Berlin November 1, 2007 Utrecht University of the.
Tomographic approach to Quantum Cosmology Cosimo Stornaiolo INFN – Sezione di Napoli Fourth Meeting on Constrained Dynamics and Quantum Gravity Cala Gonone.
Space-time Lego Willem Westra And Stefan Zohren. Our goal Find a theory of Gravity for very, very small scales Einstein’s theory of gravity: works well.
Quintessence from time evolution of fundamental mass scale.
Large spin operators in string/gauge theory duality M. Kruczenski Purdue University Based on: arXiv: (L. Freyhult, A. Tirziu, M.K.) Miami 2009.
Entanglement in Quantum Critical Phenomena, Holography and Gravity Dmitri V. Fursaev Joint Institute for Nuclear Research Dubna, RUSSIA Banff, July 31,
The causal matrix model Willem Westra and Stefan Zohren Leipzig
Spiky Strings in the SL(2) Bethe Ansatz
AdS4/CFT3+gravity for Accelerating Conical Singularities arXiv: arXiv: Mohamed Anber HET Bag Lunch Novemberr 12th.
Gerard ’t Hooft Chennai, November 17, 2009 Utrecht University.
A new continuum limit for the one matrix model
The causal matrix model Willem Westra and Stefan Zohren Leipzig
Self Sustained Wormholes Remo Garattini Università di Bergamo I.N.F.N. - Sezione di Milano MG 11 Berlin,
Quintessence from time evolution of fundamental mass scale.
Field Theory: The Past 25 Years Nathan Seiberg (IAS) The Future of Physics October, 2004 A celebration of 25 Years of.
EDUARDO GUENDELMAN, PHYSICS DEPARTMENT, BEN GURION UNIVERSITY, BEER SHEVA, ISRAEL. WITH EMIL NISSIMOV, SVETLANA PACHEVA PEDRO LABRANA AND RAMON HERRERA.
Infra-red Quantum Effects in de Sitter Space Yoshihisa Kitazawa KEK Theory Center and Sokendai H. Kitamoto and Y.K. arXiv:1012:5930.
Fermion Generations from “Apple Shaped” Extra Dimensions* Douglas Singleton CSU Fresno QUARKS 2008 Sergiev Posad, Russia May 23-29, 2008 *Work in collaboration.
Yugo Abe (Shinshu University) July 10, 2015 In collaboration with T. Inami (NTU), Y. Kawamura (Shinshu U), Y. Koyama (NCTS) YA, T. Inami,
P-adic Strings: Thermal Duality & the Cosmological Constant Tirthabir Biswas Loyola University, New Orleans PRL 104, (2010) JHEP 1010:048, (2010)
Yuya Sasai (Yukawa Institute for Theoretical Physics, Kyoto University) in collaboration with N. Sasakura (YITP) JHEP 0906, 013 (2009) [arXiv: ]
The relationship between a topological Yang-Mills field and a magnetic monopole RCNP, Osaka, 7 Dec Nobuyuki Fukui (Chiba University, Japan) Kei-Ichi.
Gravitational Physics: Quantum Gravity and Other Theoretical Aspects Luca BombelliTibor Torma Arif Caixia Gao Brian Mazur approaches to quantum gravity:
Dimensionalities of Space-Time Yu, Hoi-Lai 16 th Oct NTHU.
The false vacuum bubble : - formation and evolution - in collaboration with Bum-Hoon Lee, Chul H. Lee, Siyong Nam, and Chanyong Park Based on PRD74,
The false vacuum bubble, the true vacuum bubble, and the instanton solution in curved space 1/23 APCTP 2010 YongPyong : Astro-Particle and Conformal Topical.
The false vacuum bubble : - formation and evolution - in collaboration with Chul H. Lee(Hanyang), Wonwoo Lee, Siyong Nam, and Chanyong Park (CQUeST) Based.
Tachyon-Dilaton driven Inflation as an α'-non perturbative solution in first quantized String Cosmology Anna Kostouki, King’s College London DISCRETE ’08,
Uniform discretizations: the continuum limit of consistent discretizations Jorge Pullin Horace Hearne Institute for Theoretical Physics Louisiana State.
Random volumes from matrices Sotaro Sugishita (Kyoto Univ.) Masafumi Fukuma & Naoya Umeda (Kyoto Univ.) arXiv: (accepted in JHEP)
Background Independent Matrix Theory We parameterize the gauge fields by M transforms linearly under gauge transformations Gauge-invariant variables are.
Expanding (3+1)-dimensional universe from a Lorentzian matrix model for superstring theory in (9+1)-dimensions Talk at KEK for String Advanced Lectures,
Quantum Gravity and emergent metric Quantum Gravity and emergent metric.
Higgs branch localization of 3d theories Masazumi Honda Progress in the synthesis of integrabilities arising from gauge-string Hotel Biwako.
Expanding (3+1)-dimensional universe from a Lorentzian matrix model for superstring theory in (9+1)-dimensions Seminar at University of Tokyo,
Quantum cosmology with nontrivial topologies T. Vargas Center for Mathematics and Theoretical Physics National Central University.
Comments on entanglement entropy in the dS/CFT correspondence Yoshiki Sato ( Kyoto U. ) PRD 91 (2015) 8, [arXiv: ] 9th July.
Emergence of space, general relativity and gauge theory from tensor models Naoki Sasakura Yukawa Institute for Theoretical Physics.
Can observations look back to the beginning of inflation ?
Wilsonian approach to Non-linear sigma models Etsuko Itou (YITP, Japan) Progress of Theoretical Physics 109 (2003) 751 Progress of Theoretical Physics.
A.Sako S.Kuroki T.Ishikawa Graduate school of Mathematics, Hiroshima University Graduate school of Science, Hiroshima University Higashi-Hiroshima ,Japan.
Strong coupling problems in condensed matter and the AdS/CFT correspondence HARVARD arXiv: Reviews: Talk online: sachdev.physics.harvard.edu arXiv:
Effective Action on Manifolds with Branes and Boundaries Lebedev Physics Institute, Moscow Quarks-2008 Andrei Barvinsky Dmitry Nesterov Effective action.
Holomorphic Anomaly Mediation Yu Nakayama (Caltech) arXiv: and to appear.
Three dimensional conformal sigma models Collaborated with Takeshi Higashi and Kiyoshi Higashijima (Osaka U.) Etsuko Itou (Kyoto U. YITP) hep-th/
Random volumes from matrices Based on the work with Masafumi Fukuma and Sotaro Sugishita (Kyoto Univ.) Naoya Umeda (Kyoto Univ.) [arXiv: ][JHEP.
Supersymmetric three dimensional conformal sigma models Collaborated with Takeshi Higashi and Kiyoshi Higashijima (Osaka U.) Etsuko Itou (Kyoto U. YITP)
The nonperturbative analyses for lower dimensional non-linear sigma models Etsuko Itou (Osaka University) 1.Introduction 2.The WRG equation for NLσM 3.Fixed.
1 Bhupendra Nath Tiwari IIT Kanpur in collaboration with T. Sarkar & G. Sengupta. Thermodynamic Geometry and BTZ black holes This talk is mainly based.
Causal Space-Time on a Null Lattice with Hypercubic Coordination Martin Schaden Rutgers University - Newark Department of Physics.
Geometric Monte Carlo and Black Janus Geometries
Joe Kapusta* University of Minnesota
Zong-Kuan Guo Department of Physics, Kinki University
A rotating hairy BH in AdS_3
Opening remarks ---- Monte Carlo studies of Large N and SUSY
Quantized K
Why concave rather than convex
Based on the work submitted to EPJC
Gravity from Entanglement and RG Flow
Gauge invariant computable quantities in Timelike Liouville theory
Supersymmetry and Lorentz Invariance as Low-Energy Symmetries
Based on collaboration with Y. Kitazawa (KEK, SOKENDAI)
Bianchi type-III quantum cosmology T Vargas National Central University I.-Introduction In the standard cosmological model, the universe is described by.
Presentation transcript:

A causal alternative to the c=0 string Jan AmbjornNiels Bohr and Univ. Utrecht W.W.Univ. Of Iceland Stefan Zohren Imperial College London Renate LollUniv. Utrecht Yoshiyuki WatabikiTokyo Inst. Tech. Zakopane

Publications and preprints Putting a cap on causality violations in CDT arXiv: JHEP 0712:017,2007 A String Field Theory based on Causal Dynamical Triangulations arXiv: JHEP 0805:032,2008 Topology change in causal quantum gravity arXiv: Conf. Proc. JGRG17 Nagoya, Japan A Matrix Model for 2D Quantum Gravity defined by Causal Dynamical Triangulations arXiv: t.a. Phys. Lett. B provisional titles for papers to come that are covered in this talk: Loop equations for CDT The causal continuum limit for matrix model quantum gravity

What and Why? Two dimensional quantum gravity Non critical (bosonic) string theory = Strings living in target space with D≠26 Toy model for 4d quantum gravity Talks by J. Ambjorn and A. Goerlich

How? Dynamical triangulations (DT): Path integral over geometries  Discrete statistical sum over triangulations  Manifold is discretized with equilateral triangles  Geometry is encoded in the way triangles are glued together

Geometry of DT Flat space: Positively curved space: a

Two different theories? Euclidean 2D quantum gravity Causal 2D quantum gravity

Causal 2D quantum gravity Euclidean 2D quantum gravity Not on the discrete level

Causal 2D quantum gravity Euclidean 2D quantum gravity On the discrete level: Euclidean DT  Causal DT

Discrete: Euclidean DT  Causal DT On the discrete level: EDT = CDT + spatial topology change

In the continuum: EDT ≠CDT + spatial topology change Continuum: Euclidean DT ≠ Causal DT

EDT Hausdorff dimension = 4 Time scales non canonically Spatial topology changes are everywhere and dominate the dynamics No single string states Continuum: CDT is better behaved CDT Hausdorff dimension = 2 Time is measured in seconds as should be Spatial topology changes controlled by a coupling constant Fock space of multistring states can be explicitly defined

The Transfer matrix The old construction of CDT

Causal quantum gravity What do we compute? The disc function W(Z,T) Z T Probability amplitude

Causal Dynamical Triangulations Discrete path integral Transfer matrix The disc function T=1

Causal Dynamical Triangulations Discrete path integral Transfer matrix The disc function T=2

Causal Dynamical Triangulations Discrete path integral Transfer matrix The disc function T=3

Causal Dynamical Triangulations Discrete path integral Transfer matrix The disc function T=4

Causal Dynamical Triangulations Discrete path integral Transfer matrix The disc function T=5

Causal Dynamical Triangulations Discrete path integral Transfer matrix The disc function T=6

NEW for CDT: Loop equations

The new CDT loop equations N NN

N N+1

An example

CDT with spatial topology change N N+1 N

The coupling constant N N+1 g Coupling constant important to obtain CDT N

The “old” EDT matrix model N N+1 N

Our new CDT matrix model N N+1 N g

Solution of the disc-function

Continuum limit

Very different from EDT! Here both factors under square root contribute to the continuum limit: No non scaling contributions in the continuum!

Looks familiar?!

Continuum Matrix Model Close to ’t Hooft’s original idea: N controls the topological expansion only

Conclusions We have generalized CDT to include spatial topology changes String coupling constant controls spatial topology fluctuations too We have introduced more powerful techniques to derive CDT amplitudes: loop equations matrix models Our matrix model makes the relation between EDT and CDT very clear

Outlook The more powerful methods allow us to study matter coupling to CDT analytically Ising model Minimal models Scalar fields.... Coupling scalar field = adding a target space what are the implications to noncritical string theory? Gauge-string duality at N=2?

To be continued...