Thermodynamically Consistent Description of One-Phonon States Fragmentation in Hot Nuclei

2021 ◽  
Vol 18 (6) ◽  
pp. 629-639
Author(s):  
A. A. Dzhioev ◽  
A. I. Vdovin
Keyword(s):  
Consistent Description ◽  
Hot Nuclei

MULTIFRAGMENTATION OF HOT NUCLEI

1986 ◽  
Vol 47 (C4) ◽  
pp. C4-263-C4-274
Author(s):  
J. P. BONDORF
Keyword(s):  
Hot Nuclei

Influence of nuclear thermometers and hot nuclei properties on nuclear temperature isospin effect measurement

2021 ◽  
Vol 1009 ◽  
pp. 122156
Author(s):  
Hui-Xiao Duan ◽  
Dong-Hai Zhang ◽  
Fan Zhang ◽  
Hai-Shun Wu
Keyword(s):  
Effect Measurement ◽  
Hot Nuclei ◽  
Nuclear Temperature

Production and deexcitation of hot nuclei in collisions of 27 MeV/nucleon 40Ar with 238U

1990 ◽  
Vol 511 (1) ◽  
pp. 195-220 ◽  
Author(s):  
D. Jacquet ◽  
G.F. Peaslee ◽  
J.M. Alexander ◽  
B. Borderie ◽  
E. Duek ◽  
...  
Keyword(s):  
Hot Nuclei

scholarly journals ON VACUUM-ENERGY DECAY FROM PARTICLE PRODUCTION

2012 ◽  
Vol 27 (25) ◽  
pp. 1250150 ◽  
Author(s):  
F. R. KLINKHAMER
Keyword(s):  
Vacuum Energy ◽  
Particle Production ◽  
Energy Decay ◽  
Back Reaction ◽  
De Sitter Spacetime ◽  
De Sitter ◽  
Consistent Description ◽  
Sitter Spacetime

A simplified (but consistent) description of particle-production back-reaction effects in de Sitter spacetime is given.

A consistent description of the iron dimer spectrum with a correlated single-determinant wave function

2009 ◽  
Vol 477 (4-6) ◽  
pp. 255-258 ◽  
Author(s):  
Michele Casula ◽  
Mariapia Marchi ◽  
Sam Azadi ◽  
Sandro Sorella
Keyword(s):  
Wave Function ◽  
Consistent Description

scholarly journals The limiting Temperature of hot nuclei from microscopic Equation of State

2005 ◽  
Vol 749 ◽  
pp. 118-121 ◽  
Author(s):  
O.E. Nicotra ◽  
M. Baldo ◽  
L.S. Ferreira
Keyword(s):  
Equation Of State ◽  
Hot Nuclei

scholarly journals Bargmann–Wigner formulation and superradiance problem of bosons and fermions in Kerr space–time

2015 ◽  
Vol 30 (11) ◽  
pp. 1550052 ◽  
Author(s):  
Masakatsu Kenmoku ◽  
Y. M. Cho
Keyword(s):  
Negative Energy ◽  
Space Time ◽  
The Other ◽  
Positive Energy ◽  
Independent Components ◽  
Consistent Description ◽  
Other Hand ◽  
Kerr Space

The superradiance phenomena of massive bosons and fermions in the Kerr space–time are studied in the Bargmann–Wigner formulation. In case of bi-spinor, the four independent components spinors correspond to the four bosonic freedom: one scalar and three vectors uniquely. The consistent description of the Bargmann–Wigner equations between fermions and bosons shows that the superradiance of the type with positive energy (0 < ω) and negative momentum near horizon (p H < 0) is shown not to occur. On the other hand, the superradiance of the type with negative energy (ω < 0) and positive momentum near horizon (0 < p H ) is still possible for both scalar bosons and spinor fermions.

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