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1961
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1962por Joyce, Michael“…A homogeneous mode of a scalar field in a ``fast roll'' ( \dot{\phi}^2 >> V(\phi)), which has an energy density scaling as 1/a^6 in an expanding universe, could dominate the universe at the electroweak epoch. …”
Publicado 1996
Enlace del recurso
Enlace del recurso
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1963
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1964
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1965
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1966
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1967por De Rujula, Alvaro“…An elegantly symmetric Universe, consisting of large islands of matter and antimatter, is by no means obviously out of the question. …”
Publicado 1997
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1968
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1969
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1970
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1971
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1972“…It follows that under CH the remainder of the half line [0,infty) is universal among the continua of weight c. We complement this result by showing that 1) under MA every continuum of weight less than c is a continuous image of R^* 2) in the Cohen model the long segment of length omega_2+1 is not a continuous image of R^*, and 3) PFA implies that I_u is not a continuous image of R^*, whenever u is a c-saturated ultrafilter.…”
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1973
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1974
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1975
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1976“…We find that the transition falls into the 3d Ising universality class. The continuum limit extrapolation of the critical Higgs mass is $m_{H,c} = 72(2)$ GeV, which implies that there is no electroweak phase transition in the Standard Model.…”
Enlace del recurso
Enlace del recurso
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1977“…We make a detailed investigation of the critical properties of the electroweak theory at the critical point, and we find that the transition falls into the 3d Ising universality class. The continuum limit extrapolation of the critical Higgs mass is m_{H,c} = 72(2) GeV, which implies that there is no electroweak phase transition in the Standard Model.…”
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1978
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1979
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1980