Talk at KEK for String Advanced Lectures, 2011.9.12 (Tue.) Jun Nishimura (KEK, Sokendai)
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Transcript of 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
Answers from a nonperturbative formulationof superstring theory in (9+1)-dimensions
fundamental questions concerning our universe
1.Why (3+1)-dimensions ?
2.Why expanding ?
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)
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”
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.
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
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)
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 ?
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
Matrix model with SO(9,1) symmetry
raised and lowered by the metric
Hermitian matrices
Wick rotation
IKKT model SO(10) symmetry
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)
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.
Regularizing oscillating functions
inserting unity
convergence factor
Cure this divergence by imposing :
(2) IR cutoff in the spatial direction
Thus we arrive at
Yoneya ('97)
Monte Carlo simulation : Rational Hybrid Monte Carlo algorithm no sign problem unlike in IKKT model
Extracting time evolution
“critical time”
SSB
Consider a simpler problem :
solution :
representation matrices ofa compact semi-simple Lie algebrawith d generators
Maximum is achieved for SU(2) algebra
(continuum limit)
(infinite volume limit)
The theory thus obtained hasno parameters other than one scale paramter !
Clear large-N scaling behavior observed with
(continuum limit)
The extent of time increases andthe size of the universe becomes very large at later time.
(infinite volume limit)
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
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.
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 ?