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2101por Thoma, Markus H.“…Then the possible presence of quark matter in a neutron star core and finally the interaction of light with the Cosmic Microwave Background will be considered.…”
Publicado 2001
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Enlace del recurso
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2102“…In generic domains of the CMSSM parameter space with a relic density in the preferred range 0.1 < Omega-hsquared < 0.3, the sensitivities to all these parameters are moderate, so an interesting amount of supersymetric dark matter is a natural and robust prediction. Within these domains, the accuracy in measuring the CMSSM and other input parameters at the LHC may enable the relic density to be predicted quite precisely. …”
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2103por Dighe, Amol S.“…We explore the earth matter effects on the energy spectra of neutrinos from a supernova. …”
Publicado 2001
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2104
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2105
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2106
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2107
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2108
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2109“…We conclude the quark impact (estimated in the tadpole approximation) on the instanton liquid could shift color superconducting phase transition to higher values of the chemical potential bringing critical quark matter density to the values essentially higher than conventional nuclear one.…”
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2110
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2111
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2112
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2113
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2114
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2115
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2116
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2117
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2118por Lourenço, Carlos“…The first goal of these experimental attempts, which started in 1986, with the AGS and SPS fixed-target programs, is the discovery of the phase transition from confined hadronic matter to deconfined partonic matter. The idea that such a phase transition should exist, between hadronic and quark matter, has been around since the first models of the quark structure of hadrons. …”
Publicado 2002
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2119por Schrödinger, Erwin“…It appears here together with Mind and Matter, his essay investigating a relationship which has eluded and puzzled philosophers since the earliest times. …”
Publicado 1992
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2120