Evolve
发表于 2025-3-28 18:00:35
Mass Spectrum of ,-Deformed Dual String Theoryeter . a root of unity, in addition to the relation of such values of . with the rational conformai field theory, the Fock space of each oscillator mode in the Fubini-Veneziano operator formulation becomes truncated. Thus, based on general physical grounds, the resulting spin-(mass). relation is exp
Irremediable
发表于 2025-3-28 19:20:45
Hagedorn’s Reincarnation in String Theoryry are discussed, as well as the possible transition to a new phase beyond the string Hagedorn temperature. Studies of string black holes suggest that the concepts of space and time are likely to disappear in this reincarnation of Hagedorn.
Systemic
发表于 2025-3-29 01:45:09
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粉笔
发表于 2025-3-29 04:37:57
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exceptional
发表于 2025-3-29 10:26:16
Crystalline Quark-Hadron Phase in Neutron Starsnt component. The constancy of the pressure throughout the mixed phase independent of the proportion of the two phases is its most special feature, and one that has noticeable consequences under many circumstances. For example, if a neutron star underwent such a constant pressure phase transition, t
反应
发表于 2025-3-29 13:55:55
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BOOST
发表于 2025-3-29 16:00:14
Hadronic Matter with Internal Symmetries and its Consequences: An Expanding Hadronic Gashis matter can be considered as a gas which expands longitudinally according to a hydrodynamical evolution. In the simplest case the hadronic matter is supposed to be made of non — interacting massless pions.. However an assumption of a thermodynamical equilibrium leads to the conclusions that a sys
讨厌
发表于 2025-3-29 20:56:30
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outer-ear
发表于 2025-3-30 00:00:54
Fluctuation Corrections to Bubble Nucleationuch a computation I will consider the bubble nucleation rate in the context of the electroweak phase transition. Some of the material presented here is based on work done in collaboration with V. G. Kiselev.
面包屑
发表于 2025-3-30 05:07:42
A Finite Temperature String Phase Transition a la Volume Exclusiontribution to In . (β) in d-dimension, apart from the numerical factors, becomes.where ..(.β) is the bessel function of second kind. For temperatures β. > .. , the integral is divergent and it simply becomes impossible to have strings in thermal equilibrium. For if one had a string gas at this temper