2006
DOI: 10.1103/physrevd.74.124004
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Brane cosmology in an arbitrary number of dimensions

Abstract: We derive the effective cosmological equations for a non-Z 2 symmetric codimension one brane embedded in an arbitrary D-dimensional bulk spacetime, generalizing the D = 5, 6 cases much studied previously. As a particular case, this may be considered as a regularized codimension (D-4) brane avoiding the problem of curvature divergence on the brane. We apply our results to the case of spherical symmetry around the brane and to partly compactified AdS-Schwarzschild bulks.

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Cited by 18 publications
(26 citation statements)
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“…The study of the fission of the neutron-deficient Thorium isotopes, which are analyzed in this paper, has been motivated by the experimental data obtained during the 2012 SOFIA campaign at GSI Darmstadt [58,59]. The measurements concern the thorium isotopes 230 Th, 229 Th, 226 Th, 225 Th, 223 Th, 222 Th and 221 Th.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…The study of the fission of the neutron-deficient Thorium isotopes, which are analyzed in this paper, has been motivated by the experimental data obtained during the 2012 SOFIA campaign at GSI Darmstadt [58,59]. The measurements concern the thorium isotopes 230 Th, 229 Th, 226 Th, 225 Th, 223 Th, 222 Th and 221 Th.…”
Section: Resultsmentioning
confidence: 99%
“…The tensor interaction rearranges the position of the single particle orbitals changing the shell effects responsible for many of the properties of the quantities relevant to fission. In fact, it could be the missing ingredient required to explain a symmetric bimodal fission mode recently found in some neutron-deficient thorium isotopes [56][57][58][59]. Recent experimental data provided by the experiments of the SOFIA collaboration have revealed the existence of such a symmetric bimodal mode, composed of the standard super-long mode and a new compact mode.…”
Section: Introductionmentioning
confidence: 95%
“…The equilibrium points are then given by (z a = 0, y = y o ). The nature as well as the stability of these equilibrium points can be obtained by linearising equations (9) and studying the eigenvalues of the corresponding Jacobian matrix about the equilibrium points. In this case this is a 2n × 2n matrix given by…”
Section: Motion Of Massive Particles In the Neighbourhood Of The Submmentioning
confidence: 99%
“…Consequently, it is necessary to review the development of the relativity and gravity in higher dimensional wave equations for completeness. These contributions can be summarized as follows: the brane models [119], scalar field contribution to rotating black hole entropy [120], brane cosmology [121], N -dimensional Vaidya metric with a cosmological constant in double-null coordinates [122], the spherical gravitational collapse in N dimensions [123], the motion of a dipole in a cosmic string background [124], repulsive Casimir effect from extra dimensions and Robin boundary conditions [125], extremal black hole/CFT correspondence in gauged supergravity [126], massive fermion emission from higher dimensional black holes [127], magnetic and electric black holes [128], fermion families from two layer warped extra dimensions [129], quasinormal behavior of the D-dimensional Schwarzschild black hole [130], the study of the Schrödinger-Newton equations in D dimensions [131], rotating Einstein-Maxwell-Dilaton black holes in D dimensions [132], the Kaluza-Klein theory in the limit of large number of extra dimensions [133], gauge invariance of the one-loop effective potential in (d + 1)-dimensional Kaluza-Klein theory [134] and the multicentered solution for maximally charged dilaton black holes in arbitrary dimensions [135]. Such method was also generalized to quantum modes of the scalar field on AdS d+1 space-time [117] as well as geometric models of the (d + 1)-dimensional relativistic rotating oscillators [118].…”
Section: Introduction 1 Basic Reviewmentioning
confidence: 99%