Search results for "cosmological simulations"

showing 2 items of 2 documents

Thinking outside the box: effects of modes larger than the survey on matter power spectrum covariance

2012

Considering the matter power spectrum covariance matrix, it has recently been found that there is a potentially dominant effect on mildly non-linear scales due to power in modes of size equal to and larger than the survey volume. This {\it beat coupling} effect has been derived analytically in perturbation theory and while it has been tested with simulations, some questions remain unanswered. Moreover, there is an additional effect of these large modes, which has so far not been included in analytic studies, namely the effect on the estimated {\it average} density which enters the power spectrum estimate. In this article, we work out analytic, perturbation theory based expressions including…

Astrofísicadark matter simulationsCosmology and GravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesBeat (acoustics)Astrophysicspower spectrumAstrophysics01 natural sciences0103 physical sciencesStatistical physics010303 astronomy & astrophysics/dk/atira/pure/core/subjects/cosmologyPhysicsCosmologia010308 nuclear & particles physicsCovariance matrixMatter power spectrumcosmological simulationsSpectral densityFísicaAstronomy and AstrophysicsCovarianceRedshiftGalaxyCosmologyStepping stonegalaxy clusteringAstrophysics - Cosmology and Nongalactic Astrophysics
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Observational constraints on decoupled hidden sectors

2016

We consider an extension of the Standard Model with a singlet sector consisting of a real (pseudo)scalar and a Dirac fermion coupled with the Standard Model only via the scalar portal. We assume that the portal coupling is weak enough for the singlet sector not to thermalize with the Standard Model allowing the production of singlet particles via the freeze-in mechanism. If the singlet sector interacts with itself sufficiently strongly, it may thermalize within itself, resulting in dark matter abundance determined by the freeze-out mechanism operating within the singlet sector. We investigate this scenario in detail. In particular, we show that requiring the absence of inflationary isocurva…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterScalar (mathematics)FOS: Physical sciencesParameter space114 Physical sciences01 natural sciencesStandard Modeldecouplingsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)ABELL 38270103 physical sciencesSinglet state010306 general physicsdark matter abundanceInflation (cosmology)PhysicsINTERACTING DARK-MATTERta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyextensions of the Standard ModelHidden sectorHigh Energy Physics - Phenomenologysinglet sectorCOSMOLOGICAL SIMULATIONSDirac fermionGALAXY CLUSTER 1E-0657-56symbols3.5 KEV LINEINTERACTION CROSS-SECTIONAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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