Expanding (3+1)-dimensional universe from a lorentzian matrix model for superstring theory in (9+1) dimensions.
نویسندگان
چکیده
We reconsider the matrix model formulation of type IIB superstring theory in (9+1)-dimensional space-time. Unlike the previous works in which the Wick rotation was used to make the model well defined, we regularize the Lorentzian model by introducing infrared cutoffs in both the spatial and temporal directions. Monte Carlo studies reveal that the two cutoffs can be removed in the large-N limit and that the theory thus obtained has no parameters other than one scale parameter. Moreover, we find that three out of nine spatial directions start to expand at some "critical time," after which the space has SO(3) symmetry instead of SO(9).
منابع مشابه
Local field theory from the expanding universe at late times in the IIB matrix model
Recently we have shown that (3+1)-dimensional expanding universe appears dynamically and uniquely from the Lorentzian version of the IIB matrix model, which is considered as a nonperturbative formulation of superstring theory. Similarly, it is possible that the Standard Model appears uniquely at the electroweak scale from the same model at late times. In order to pursue such a possibility, we d...
متن کاملLate time behaviors of the expanding universe in the IIB matrix model
Recently we have studied the Lorentzian version of the IIB matrix model as a nonperturbative formulation of superstring theory. By Monte Carlo simulation, we have shown that the notion of time —as well as space—emerges dynamically from this model, and that we can uniquely extract the real-time dynamics, which turned out to be rather surprising: after some “critical time”, the SO(9) rotational s...
متن کاملMonte Carlo studies on the expanding behavior of the early universe in the Lorentzian type IIB matrix model
The type IIB matrix model is a conjectured nonperturbative formulation of superstring theory. Recently the Lorentzian version of the model has been studied by Monte Carlo simulation, and it has been shown that only three out of nine spatial directions start to expand after a critical time. We extend this work by investigating the expanding behavior for much longer time. We find that the 3d spac...
متن کاملAccelerating cosmologies from exponential potentials
It is learnt that exponential potentials of the form V ∼ exp(−2cφ/Mp) arising from the hyperbolic compactification of higher-dimensional theories are of interest for getting short periods of accelerated cosmological expansions. Using such a potential derived for the combined case of hyperbolic-flux compactification, we study a fourdimensional flat (or open) FRW cosmolgy and give analytic (and n...
متن کاملChallenges for Superstring Cosmology
We consider whether current notions about superstring theory below the Planck scale are compatible with cosmology. We find that the anticipated form for the dilaton interaction creates a serious roadblock for inflation and makes it unlikely that the universe ever reaches a state with zero cosmological constant and time-independent gravitational constant. Superstring theories have been extensive...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
- Physical review letters
دوره 108 1 شماره
صفحات -
تاریخ انتشار 2012