1999 European School of High-Energy Physics: Časta-Papiernička, Slovak Republic, 22 August-4 September 1999 : ProceedingsA. Olchevski |
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Page 112
... energy density of the fluid at a given time in the expansion , and U " is the comoving four - velocity , satisfying ... energy of quantum field theory , although we still do not understand why should it have such a small value ( 120 ...
... energy density of the fluid at a given time in the expansion , and U " is the comoving four - velocity , satisfying ... energy of quantum field theory , although we still do not understand why should it have such a small value ( 120 ...
Page 276
... energy densities we have to observe a drop of about 40 % , and , eventually , at even higher energy densities J / has ... density of these comovers [ 19 ] . Another increase of the J / absorption could be produced if , before the J / is ...
... energy densities we have to observe a drop of about 40 % , and , eventually , at even higher energy densities J / has ... density of these comovers [ 19 ] . Another increase of the J / absorption could be produced if , before the J / is ...
Page 283
... energy density of about 2.1 GeV / fm3 and the second at about 3.2 GeV / fm3 . Thermal model analyses of strange particle yields have shown that the system approaches thermal and chemical equilibrium [ 52 ] . The different features ...
... energy density of about 2.1 GeV / fm3 and the second at about 3.2 GeV / fm3 . Thermal model analyses of strange particle yields have shown that the system approaches thermal and chemical equilibrium [ 52 ] . The different features ...
Contents
Field Theory and the Standard Model | 1 |
Astrophysics and cosmology | 109 |
Determination of cosmological parameters | 126 |
39 other sections not shown
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