2000
DOI: 10.1103/physrevd.62.086006
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Adding matter to Poincaré invariant branes

Abstract: A solution to the cosmological constant problem has been proposed in which our universe is a 3-brane in a 5-dimensional spacetime. With a bulk scalar, the field equations admit a Poincare invariant brane solution regardless of the value of the cosmological constant (tension) on the brane. However, the solution does not include matter in the brane. We find new exact static solutions with matter density and pressure in the brane. We study small perturbations about these solutions. None seem consistent with obser… Show more

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Cited by 34 publications
(50 citation statements)
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“…This selftuning mechanism, first suggested in refs. [37,38], has been the subject of a great deal of debate in the context of supergravity models where U and V are derived from the same super-potential (see also [39,40]). Unfortunately, it appears [41] that no such supersymmetric model exists without the a naked singularity somewhere in the bulk.…”
Section: Effective 4d Equationsmentioning
confidence: 99%
“…This selftuning mechanism, first suggested in refs. [37,38], has been the subject of a great deal of debate in the context of supergravity models where U and V are derived from the same super-potential (see also [39,40]). Unfortunately, it appears [41] that no such supersymmetric model exists without the a naked singularity somewhere in the bulk.…”
Section: Effective 4d Equationsmentioning
confidence: 99%
“…In principle, photon emission from the initial light-quark is a non-perturbative, long-distance, contamination to the interesting signal of the short-distance dipole emission from H eff [76,77]. Fortunately, it can be shown [75] that predominantly these LD photons have the same helicity as those from H eff .…”
Section: G Time-dependent Cp Asymmetries In Exclusive Radiative B Dementioning
confidence: 99%
“…The reason for including this class of power corrections is that they come with numerical enhancement from the large Wilson coefficients C 1,2 (C 1 ≈ 3C 7 ) but are CKM suppressed and thus these contributions are expected to be very small for the decay under consideration. The amplitude for charged B meson decay in terms of Weak annihilation A, charmed penguin P c , gluonic penguin M and short distance amplitude P t can be written as [following the notation of [18]]…”
mentioning
confidence: 99%