Talk at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

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Expanding (3+1)-dimensional universe from a Lorentzian matrix model for superstring theory in (9+1)-dimensions Talk at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai) Ref.) Kim-J.N.-Tsuchiya arXiv:1108.1540

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Expanding (3+1)-dimensional universe from a Lorentzian matrix model for superstring theory in (9+1)-dimensions. Talk at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai) Ref.) Kim-J.N.-Tsuchiya arXiv:1108.1540. 1. Introduction. - PowerPoint PPT Presentation

Transcript of Talk at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Page 1: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Expanding (3+1)-dimensional universe from a Lorentzian matrix model for superstring theory in (9+1)-dimensions

Talk at KEK for String Advanced Lectures, 2011.9.12 (Tue.)Jun Nishimura (KEK, Sokendai)

Ref.) Kim-J.N.-Tsuchiya arXiv:1108.1540

Page 2: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)
Page 3: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Answers from a nonperturbative formulationof superstring theory in (9+1)-dimensions

fundamental questions concerning our universe

1.Why (3+1)-dimensions ?

2.Why expanding ?

Page 4: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Previous proposal

Euclideanized model with SO(10) symmetry

SSB of SO(10) studied by Gaussian Expansion Method J.N.-Okubo-Sugino, arXiv:1108.1293

free energy of SO(d) symmetric vacua (d=2,3,4,5,6,7) minimum at d=3 extent of space-time finite in all directions

motivated us to reconsider the formulation

Ishibashi-Kawai-Kitazawa-Tsuchiya (’96)

Page 5: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Our new proposal :

regularize SO(9,1) Lorentzian symmetric model without Wick rotation

Monte Carlo simulation

3 out of 9 spatial directions start to expand at some “critical time”

Page 6: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Comments on related works

Quantum Cosmology with minisuperspace approx.

Causal Dynamical Traingulation

Matrix Cosmology Freedman-Gibbons-Schnabl (’05) Matrix Big Bang Craps-Sethi-Verlinde (’05) Emergent gravity Steinacker (’11), Yang (’10)

Vilenkin (’82,’84), Hartle-Hawking (’83)

Ambjorn-Jurkiewicz-Loll (’05)

We expect that what we are doing is essentiallya first-principle calculation of the unified theory including quantum gravity.

Page 7: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Plan of the talk

1. Introduction2. Matrix model for superstrings3. Matrix model with SO(9,1) symmetry4. Monte Carlo results5. Mechanism of the SSB6. Removing the cutoffs7. Summary and discussions

Page 8: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)
Page 9: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

IKKT model

matrix regularization of the Green-Schwarz worldsheet action in the Schild gauge

interactions between D-branes

string field theory from SD eqs. for Wilson loops

Ishibashi-Kawai-Kitazawa-Tsuchiya (’96)

proposed as a nonperturbative definition of type IIB superstring theory in 10 dim.

Fukuma-Kawai-Kitazawa-Tsuchiya (’98)

c.f.) Matrix Theory Banks-Fischler-Shenker-Susskind (’96)

Page 10: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

10 D4 D

10   Hermitian matrices

Derivation of low-energy effective theory branched-polymer-like system Aoki-Iso-Kawai-Kitazawa-Tada (’99)

Explicit calculations by the Gaussian expansion methodJ.N.-Sugino (’02), J.N.-Okubo-Sugino,Kawai, Kawamoto, Kuroki, Matsuo, Shinohara, Aoyama, Shibusa,…

Does our 4-dimensional space-time appear from 10-dimensions ?

Page 11: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Results of the Gaussian expansion method J.N.-Okubo-Sugino (arXiv:1108.1293)

Minimum of the free energyoccurs at d=3

Extent of space-timefinite in all directions

SSB of SO(10) : interesting dynamical property of IKKT model,but we still seem to miss some important ingredient…

extended directions

shrunken directions

Page 12: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)
Page 13: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Matrix model with SO(9,1) symmetry

raised and lowered by the metric

  Hermitian matrices

Wick rotation

IKKT model SO(10) symmetry

Page 14: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Partition function of the Lorentzian model

connection to the worldsheet theory

opposite sign !Unlike IKKT model, the path integral is ill-defined !

c.f.) complex in the case of IKKT model the phase factor induces SSB of SO(10)

J.N.-Vernizzi (’00), Anagnostopoulos-J.N.(’02)

Krauth-Nicolai-Staudacher (’98), Austing-Wheater (’01)

Page 15: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Regularizing the Lorentzian model

In order to separate space and time,we “gauge fix” the boost invariance.

(1) IR cutoff in the temporal direction

SO(9) symmetry is still manifest.

Page 16: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Regularizing oscillating functions

inserting unity

convergence factor

Page 17: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Cure this divergence by imposing :

(2) IR cutoff in the spatial direction

Page 18: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Thus we arrive at

Yoneya ('97)

Monte Carlo simulation : Rational Hybrid Monte Carlo algorithm no sign problem unlike in IKKT model

Page 19: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)
Page 20: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Extracting time evolution

Page 21: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)
Page 22: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

“critical time”

SSB

Page 23: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)
Page 24: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Consider a simpler problem :

solution :

representation matrices ofa compact semi-simple Lie algebrawith d generators

Maximum is achieved for SU(2) algebra

Page 25: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)
Page 26: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

(continuum limit)

(infinite volume limit)

The theory thus obtained hasno parameters other than one scale paramter !

Page 27: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Clear large-N scaling behavior observed with

(continuum limit)

Page 28: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

The extent of time increases andthe size of the universe becomes very large at later time.

(infinite volume limit)

Page 29: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)
Page 30: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

A new proposal for the nonperturbative formulation of type IIB superstring theory in ten dimensions.

instead of making Wick rotation, we introduce the IR cutoffs for both temporal and spatial directions

after “gauge fixing” the boost symmetry

The two cutoffs can be removed in the large-N limit.

The theory thus obtained has no parameters other than one scale parameter.

Summary

Page 31: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Integrating over the scale factor first, we obtain a model without sign problem.

c.f.) Monte Carlo studies of IKKT model difficult due to sign problem

Monte Carlo simulation revealed SSB of SO(9) down to SO(3) at some critical time. mechanism is totally different from that for the SSB in the IKKT model

the size of the 3d space increases with time

Cosmological singularity is naturally avoided due to noncommutativity.

Page 32: Talk  at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)

Crucial role played by SUSY

c.f.) bosonic model

no expansion and no SSB !

Future directions Does a local field theory on a commutative space-time appear at later time ?

How do 4 fundamental interactions and the matter fields appear at later time ?