phase space integral
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scholarly journals ImprovedKL→π±e∓νform factor and phase space integral with reduced model uncertainty

2006 ◽  
Vol 74 (9) ◽  
Author(s):  
E. Abouzaid ◽  
M. Arenton ◽  
A. R. Barker ◽  
L. Bellantoni ◽  
A. Bellavance ◽  
...  
Keyword(s):  
Phase Space ◽  
Model Uncertainty ◽  
Reduced Model ◽  
Phase Space Integral

Law of large numbers and asymptotic behavior of phase-space integral

2004 ◽  
Vol 67 (1) ◽  
pp. 140-144
Author(s):  
J. Manjavidze ◽  
A. N. Sissakian ◽  
N. Shubitidze
Keyword(s):  
Asymptotic Behavior ◽  
Phase Space ◽  
Law Of Large Numbers ◽  
Large Numbers ◽  
Phase Space Integral

scholarly journals ON THE LIMITATIONS OF NEUTRINO EMISSIVITY FORMULA OF IWAMOTO

1994 ◽  
Vol 09 (19) ◽  
pp. 1717-1726 ◽  
Author(s):  
SANJAY K. GHOSH ◽  
S.C. PHATAK ◽  
PRADIP K. SAHU
Keyword(s):  
Phase Space ◽  
Quark Matter ◽  
Momentum Conservation ◽  
Severe Restriction ◽  
Alternative Formula ◽  
Neutrino Emissivity ◽  
Phase Space Integral

The neutrino emissivity from two- and three-flavor quark matter is numerically calculated and compared with Iwamoto’s formula. We find that the calculated emissivity is smaller than Iwamoto’s result by orders of magnitude when pf(u)+pf(e)−pf(d(s)) is comparable with the temperature. We attribute it to the severe restriction imposed by momentum conservation on the phase space integral. We obtain an alternative formula for the neutrino emissivity which is valid for any value of pf(u)+Pf(e)−Pf(d(s)) when the quarks and electrons are degenerate.

Multiparticle production in proton–proton collisions at high energies

1985 ◽  
Vol 63 (11) ◽  
pp. 1449-1452 ◽  
Author(s):  
M. T. Hussein ◽  
N. M. Hassan ◽  
M. K. Hegab
Keyword(s):  
Monte Carlo ◽  
Theoretical Model ◽  
Phase Space ◽  
Multiplicity Distribution ◽  
Proton Proton ◽  
Sequential Decay ◽  
Proton Collisions ◽  
High Energies ◽  
Proton Proton Collisions ◽  
Phase Space Integral

The multiplicity distribution and the inelasticity coefficient are studied for proton–proton collisions at incident energies of 6, 19, 25, and 69 GeV. A theoretical model is proposed, based on a sequential decay system formed by the two interacting protons. The Monte Carlo technique is used to calculate the phase-space integral and for simulation of events for the different reactions.

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