scholarly journals Exact monopole instantons and cosmological solutions in string theory from Abelian dimensional reduction

1997 ◽  
Vol 55 (10) ◽  
pp. 6394-6402 ◽  
Author(s):  
Adrián R. Lugo
1999 ◽  
Vol 14 (26) ◽  
pp. 4121-4142 ◽  
Author(s):  
H. LÜ ◽  
S. MUKHERJI ◽  
C. N. POPE

We study the relationship between static p-brane solitons and cosmological solutions of string theory or M theory. We discuss two different ways in which extremal p-branes can be generalized to nonextremal ones, and show how wide classes of recently discussed cosmological models can be mapped into nonextremal p-brane solutions of one of these two kinds. We also extend previous discussions of cosmological solutions to include some that make use of cosmological-type terms in the effective action that can arise from the generalized dimensional reduction of string theory or M theory.


2001 ◽  
Vol 16 (10) ◽  
pp. 1679-1701 ◽  
Author(s):  
B. SATHIAPALAN

We continue the discussion of our previous paper on writing down gauge-invariant interacting equations for a bosonic string using the loop variable approach. In the earlier paper the equations were written down in one higher dimension where the fields are massless. In this paper we describe a procedure for dimensional reduction that gives interacting equations for fields with the same spectrum as in bosonic string theory. We also argue that the on-shell scattering amplitudes implied by these equations for the physical modes are the same as for the bosonic string. We check this explicitly for some of the simpler equations. The gauge transformation of space–time fields induced by gauge transformations of the loop variables are discussed in some detail. The unintegrated (i.e. before the Koba–Nielsen integration), regularized version of the equations, are gauge invariant off-shell (i.e. off the free mass shell).


2004 ◽  
Vol 19 (10) ◽  
pp. 1499-1509
Author(s):  
THIBAULT DAMOUR

We briefly review two aspects of string cosmology: (1) the presence of chaos in the generic cosmological solutions of the tree-level low-energy effective actions coming out of string theory, and (2) the remarkable link between the latter chaos and the Weyl groups of some hyperbolic Kac–Moody algebras.


2008 ◽  
Vol 77 (12) ◽  
Author(s):  
Simeon Hellerman ◽  
Ian Swanson

2016 ◽  
Vol 25 (12) ◽  
pp. 1644018 ◽  
Author(s):  
Samir D. Mathur

It is conventionally believed that if a ball of matter of mass [Formula: see text] has a radius close to [Formula: see text][Formula: see text]GM then it must collapse to a black hole. But string theory microstates (fuzzballs) have no horizon or singularity, and they do not collapse. We consider two simple examples from classical gravity to illustrate how this violation of our intuition happens. In each case, the ‘matter’ arises from an extra compact dimension, but the topology of this extra dimension is not trivial. The pressure and density of this matter diverge at various points, but this is only an artifact of dimensional reduction; thus, we bypass results like Buchadahl’s theorem. Such microstates give the entropy of black holes, so these topologically nontrivial constructions dominate the state space of quantum gravity.


1999 ◽  
Vol 60 (4) ◽  
Author(s):  
Nemanja Kaloper ◽  
Ian I. Kogan ◽  
Keith A. Olive

2005 ◽  
Vol 2005 (05) ◽  
pp. 016-016
Author(s):  
Makoto Tanabe ◽  
Shuntaro Mizuno

2011 ◽  
Vol 01 ◽  
pp. 189-194 ◽  
Author(s):  
MASATO MINAMITSUJI

We derive the brane cosmological solutions in the six-dimensional Einstein-Maxwell-dilaton theory, via dimensional reduction from the higher-dimensional Einstein-Maxwell theory. Two extra dimensions are compactified by a magnetic flux and two codimension-two branes are located at the boundaries. All the cosmological solutions approach an attractor in the later times. The attractor represents a simple power-law inflationary Universe whose power is simply given by the dilatonic coupling in the theory. Then, we discuss the properties of our solutions and deduce the cosmological implications.


2020 ◽  
Vol 8 (1) ◽  
Author(s):  
Sara Pasquetti ◽  
Shlomo Razamat ◽  
Matteo Sacchi ◽  
Gabi Zafrir

We discuss compactifications of rank QQ E-string theory on a torus with fluxes for abelian subgroups of the E_8E8 global symmetry of the 6d6d SCFT. We argue that the theories corresponding to such tori are built from a simple model we denote as E[USp(2Q)]E[USp(2Q)]. This model has a variety of non trivial properties. In particular the global symmetry is USp(2Q)\times USp(2Q)\times U(1)^2USp(2Q)×USp(2Q)×U(1)2 with one of the two USp(2Q)USp(2Q) symmetries emerging in the IR as an enhancement of an SU(2)^QSU(2)Q symmetry of the UV Lagrangian. The E[USp(2Q)]E[USp(2Q)] model after dimensional reduction to 3d3d and a subsequent Coulomb branch flow is closely related to the familiar 3d3dT[SU(Q)]T[SU(Q)] theory, the model residing on an S-duality domain wall of 4d4d\mathcal{N}=4𝒩=4SU(Q)SU(Q) SYM. Gluing the E[USp(2Q)]E[USp(2Q)] models by gauging the USp(2Q)USp(2Q) symmetries with proper admixtures of chiral superfields gives rise to systematic constructions of many examples of 4d4d theories with emergent IR symmetries. We support our claims by various checks involving computations of anomalies and supersymmetric partition functions. Many of the needed identities satisfied by the supersymmetric indices follow directly from recent mathematical results obtained by E. Rains.


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