Higher-dimensional Einstein-Maxwell theory with inflation

1985 ◽  
Vol 32 (4) ◽  
pp. 1011-1013 ◽  
Author(s):  
Y. S. Myung ◽  
B. H. Cho ◽  
Yongduk Kim ◽  
Young-Jai Park
Keyword(s):  
Maxwell Theory ◽  
Higher Dimensional

scholarly journals Critical Combinations of Higher-Order Terms in Einstein-Maxwell Theory and Compactification

2015 ◽  
Vol 2015 ◽  
pp. 1-10 ◽  
Author(s):  
Nahomi Kan ◽  
Kiyoshi Shiraishi
Keyword(s):  
Higher Order ◽  
De Sitter ◽  
Spontaneous Compactification ◽  
Maxwell Theory ◽  
Higher Derivative ◽  
Higher Dimensional ◽  
Inflationary Phase ◽  
Expansion Time ◽  
Higher Order Terms

We discuss the role of a particular combination of higher derivative terms in higher dimensional theories, particularly in the background of spontaneous compactification. Two classes of theories are proposed in this paper. The first model as a generalization of the critical gravity with the Maxwell field could have a de Sitter solution. We consider the Lanczos-Lovelock term and Horndeski term as well as the higher-order Maxwell term for the second model, which contains a possible longer expansion time for the inflationary phase. It is interesting that both models can be regarded as the generalization of the Randjbar-Daemi, Salam and Strathdee (RSS) model and give the well behavior for inflation stage under the specific assumptions.

scholarly journals Thin shell wormholes in higher dimensional Einstein–Maxwell theory

2006 ◽  
Vol 38 (11) ◽  
pp. 1687-1695 ◽  
Author(s):  
F. Rahaman ◽  
M. Kalam ◽  
S. Chakraborty
Keyword(s):  
Thin Shell ◽  
Maxwell Theory ◽  
Higher Dimensional ◽  
Thin Shell Wormholes

scholarly journals Quasinormal Modes of Charged Black Holes in Higher-Dimensional Einstein-Power-Maxwell Theory

Axioms ◽  
2020 ◽  
Vol 9 (1) ◽  
pp. 33 ◽  
Author(s):  
Grigoris Panotopoulos
Keyword(s):  
Black Holes ◽  
Scalar Field ◽  
Electric Charge ◽  
Quasinormal Modes ◽  
Space Time ◽  
Maxwell Theory ◽  
Charged Black Holes ◽  
Higher Dimensional ◽  
The Impact ◽  
Scalar Perturbations

We compute the quasinormal frequencies for scalar perturbations of charged black holes in five-dimensional Einstein-power-Maxwell theory. The impact on the spectrum of the electric charge of the black holes, of the angular degree, of the overtone number, and of the mass of the test scalar field is investigated in detail. The quasinormal spectra in the eikonal limit are computed as well for several different space-time dimensionalities.

scholarly journals All Higher-Dimensional Majumdar–Papapetrou Black Holes

2021 ◽  
Author(s):  
James Lucietti
Keyword(s):  
Black Holes ◽  
Careful Analysis ◽  
Positive Mass Theorem ◽  
Maxwell Theory ◽  
Asymptotically Flat ◽  
Extreme Black Hole ◽  
Higher Dimensional ◽  
Manifolds With Conical Singularities ◽  
Regular Event ◽  
Horizon Geometry

AbstractWe prove that the only asymptotically flat spacetimes with a suitably regular event horizon, in a generalised Majumdar–Papapetrou class of solutions to higher-dimensional Einstein–Maxwell theory, are the standard multi-black holes. The proof involves a careful analysis of the near-horizon geometry and an extension of the positive mass theorem to Riemannian manifolds with conical singularities. This completes the classification of asymptotically flat, static, extreme black hole solutions in this theory.

Lovelock black holes in the presence of nonlinear electrodynamics

2015 ◽  
Vol 24 (06) ◽  
pp. 1550040 ◽  
Author(s):  
Seyed Hossein Hendi
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Nonlinear Electrodynamics ◽  
Thermodynamic Quantities ◽  
De Sitter ◽  
Maxwell Theory ◽  
Hole Radius ◽  
Higher Dimensional ◽  
Effective Cosmological Constant ◽  
Black Hole Solutions

In this paper, we consider third-order Lovelock–Maxwell gravity with additional (Fμν Fμν)2 term as a nonlinearity correction of the Maxwell theory. We obtain black hole solutions with various horizon topologies (and various number of horizons) in which their asymptotical behavior can be flat or anti-de Sitter with an effective cosmological constant. We investigate the effects of Lovelock and electrodynamic corrections on properties of the solutions. Then, we restrict ourselves to asymptotically flat solutions and calculate the conserved and thermodynamic quantities. We check the first law of thermodynamics for these black hole solutions and calculate the heat capacity to analyze stability. Although higher dimensional black holes in Einstein gravity are unstable, here we look for suitable constraints on the black hole radius to find thermally stable black hole solutions.

SIX-DIMENSIONAL BRANEWORLD COSMOLOGY

2011 ◽  
Vol 01 ◽  
pp. 189-194 ◽  
Author(s):  
MASATO MINAMITSUJI
Keyword(s):  
Magnetic Flux ◽  
Power Law ◽  
Dimensional Reduction ◽  
Extra Dimensions ◽  
Inflationary Universe ◽  
Maxwell Theory ◽  
Braneworld Cosmology ◽  
Codimension Two ◽  
Higher Dimensional ◽  
Cosmological Solutions

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.

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