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4801“…As no such increase is observed on cosmological scales, black hole formation requires strongly positive running n' of the spectral index n, though the running might only kick in below the `cosmological scales' probed by the CMB anisotropy and galaxy surveys. …”
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4802“…A new class of metastable de Sitter vacua is presented and analyzed in N =1 supergravity and string theory with tunable (infinitesimally small) value of the cosmological constant. They are based on a gauged R-symmetry and the minimal spectrum contains a vector and a linear multiplet of the string dilaton or of a compactification modulus. …”
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4803por Verde, Licia, Jimenez, Raul, Simpson, Fergus, Alvarez-Gaume, Luis, Heavens, Alan, Matarrese, Sabino“…We give an analytical form for the weighted correlation function of peaks in a Gaussian random field. In a cosmological context, this approach strictly describes the formation bias and is the main result here. …”
Publicado 2014
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4804“…Interactions of heavy Majorana neutrinos in the thermal phase of the early universe may be the origin of the cosmological matter-antimatter asymmetry. This mechanism of baryogenesis implies stringent constraints on light and heavy Majorana neutrino masses. …”
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4805“…Such a particle is shown to be consistent with all experimental data and with cosmological nucleosynthesis. There are difficulties with constraints from SN~1987A but these may be evaded if squarks are non-degenerate in mass.…”
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4806“…We also discuss briefly their application to a consistent treatment of cosmological constraints on $R$-parity violation.…”
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4807por Villadoro, Giovanni“…Supersymmetry is spontaneously broken to N=4,2,0 with vanishing cosmological constant. We discuss the gaugings of the broken phases, the scalar geometries and the spectrum. …”
Publicado 2004
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4808“…Specifically, the cosmological dark energy density measured at the present epoch may be linked to the apparent retardation of energetic photons propagating from nearby AGNs. …”
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info:eu-repo/semantics/article -
4809por Fraser, Sean, Hektor, Andi, Hütsi, Gert, Kannike, Kristjan, Marzo, Carlo, Marzola, Luca, Spethmann, Christian, Racioppi, Antonio, Raidal, Martti, Vaskonen, Ville, Veermäe, Hardi“…The recently claimed anomaly in the measurement of the 21 cm hydrogen absorption signal by EDGES at z∼17 , if cosmological, requires the existence of new physics. …”
Publicado 2018
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4810por Bondarenko, Kyrylo, Boyarsky, Alexey, Nikolic, Marco, Pradler, Josef, Sokolenko, Anastasia“…When the Dark Matter mass is below the eV-scale, its cosmological occupation number exceeds the ones of photons from the cosmic microwave background as well as of relic neutrinos. …”
Publicado 2020
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4811“…This reveals new cosmologically interesting parameter regions which have not attracted much attention so far. …”
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4812“…A critical review is given of the current status of cosmological nucleosynthesis. In the framework of the Standard Model with 3 types of relativistic neutrinos, the baryon-to-photon ratio, η, corresponding to the inferred primordial abundances of deuterium and helium-4 is consistent with the independent determination of η from observations of anisotropies in the cosmic microwave background. …”
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4813por Valle, José W F“…The topics include a basic discussion of the theory of neutrino mass and the corresponding extensions of the Standard Model that incorporate massive neutrinos; an overview of the present observational status of neutrino mass searches, with emphasis on solar neutrinos, as well the as cosmological data on the amplitude of primordial density fluctuations; the implications of neutrino mass in cosmological nucleosynthesis, non-accelerator, as well as in high energy particle collider experiments. …”
Publicado 1991
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4814“…The usual characterization of exact solutions of Einstein field equations, including cosmological solutions, is based on the symmetry properties of their corresponding metrics which is obviously mathematically involved. …”
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Online Artículo Texto -
4815“…We find that a collider with $E_{CM} = 500$ GeV or 1 TeV can only explore part of the cosmological region, and that a collider with $E_{CM} = 1.5$ TeV with sufficient luminosity can explore all of the supersymmetric dark matter region.…”
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4816por Gasperini, M.“…I discuss the status of present knowledge about a possible background of relic gravitons left by an early, pre-big bang cosmological epoch, whose existence in the past of our Universe is suggested by the duality symmetries of string theory.…”
Publicado 1996
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4817por Kusenko, Alexander“…They could be copiously produced in the early Universe as a by-product of the Affleck-Dine baryogenesis. I review the cosmological and astrophysical implications, methods of detection, and the present limits on this form of dark matter.…”
Publicado 1998
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4818“…Generalizing our previous work, we show how $O(d,d)$ transformations can be used to "boost away" in new dimensions the physical singularities that occur generically in cosmological and/or black-hole string backgrounds. As an example, we show how a recent model by Nappi and Witten can be made singularity-free via $O(3,3)$ boosts involving a fifth dimension.…”
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4819“…We also conclude that the rate of decreasing [Formula: see text] with increasing [Formula: see text] varies from epoch to epoch, at vanishing and finite cosmological constant. These results obviously help in improving our understanding of the nucleosynthesis and the cosmological large-scale structure.…”
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Online Artículo Texto -
4820por De Luca, Valerio, Mitridate, Andrea, Redi, Michele, Smirnov, Juri, Strumia, Alessandro“…Hybrid hadrons, made of Q and of standard model quarks and gluons, have large QCD cross sections, and do not reach underground detectors. Their cosmological abundance is 105 times smaller than DM, such that their unusual signals seem compatible with bounds. …”
Publicado 2018
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