scholarly journals Feasibility of using neutrino intensity interferometry to measure protoneutron star radii

2018 ◽  
Vol 98 (4) ◽  
Author(s):  
Warren P. Wright ◽  
James P. Kneller
Keyword(s):  
Intensity Interferometry ◽  
Protoneutron Star

scholarly journals Entanglement Enabled Intensity Interferometry of different wavelengths of light

2021 ◽  
Vol 424 ◽  
pp. 168346
Author(s):  
Jordan Cotler ◽  
Frank Wilczek ◽  
Victoria Borish
Keyword(s):  
Intensity Interferometry

Protoneutron Star Formation

1988 ◽  
Vol 7 (4) ◽  
pp. 371-381
Author(s):  
Adam Burrows
Keyword(s):  
Star Formation ◽  
Neutron Star ◽  
General Analysis ◽  
Sn 1987A ◽  
Supernova Neutrino ◽  
Neutrino Theory ◽  
Protoneutron Star

AbstractThe theory of neutron star formation is addressed in the light of the detected neutrino burst from SN 1987A. A brief review of how supernova neutrino theory has evolved over the last 30 years and a general analysis of the SN 1987A detections is presented.

A NUCLEAR MANY-BODY THEORY AT FINITE TEMPERATURE APPLIED TO A PROTONEUTRON STAR

2002 ◽  
Vol 11 (02) ◽  
pp. 83-104 ◽  
Author(s):  
GUILHERME F. MARRANGHELLO ◽  
CESAR A. Z. VASCONCELLOS ◽  
MANFRED DILLIG ◽  
J. A. DE FREITAS PACHECO
Keyword(s):  
Phase Transition ◽  
Nuclear Matter ◽  
Finite Temperature ◽  
Degrees Of Freedom ◽  
Many Body ◽  
Many Body Theory ◽  
The Masses ◽  
Protoneutron Stars ◽  
Protoneutron Star

Thermodynamical properties of nuclear matter are studied in the framework of an effective many-body field theory at finite temperature, considering the Sommerfeld approximation. We perform the calculations by using the nonlinear Boguta and Bodmer model, extended by the inclusion of the fundamental baryon octet and leptonic degrees of freedom. Trapped neutrinos are also included in order to describe protoneutron star properties through the integration of the Tolman–Oppenheimer–Volkoff equations, from which we obtain, beyond the standard relations for the masses and radii of protoneutron stars as functions of the central density, new results of these quantities as functions of temperature. Our predictions include: the determination of an absolute value for the limiting mass of protoneutron stars; new structural aspects on the nuclear matter phase transition via the behavior of the specific heat and, through the inclusion of quark degrees of freedom, the properties of a hadron-quark phase transition and hybrid protoneutron stars

Characterization of nuclear sources via two-neutron intensity interferometry

1999 ◽  
Vol 660 (1) ◽  
pp. 20-40 ◽  
Author(s):  
R. Ghetti ◽  
N. Colonna ◽  
J. Helgesson ◽  
E. De Filippo ◽  
G. Tagliente ◽  
...  
Keyword(s):  
Neutron Intensity ◽  
Intensity Interferometry

A new analytical approach to study chaos fraction characterization by using intensity interferometry

2021 ◽  
Vol 152 ◽  
pp. 111414
Author(s):  
Ghulam Bary ◽  
Waqar Ahmed ◽  
Muhammad Sajid ◽  
Riaz Ahmad ◽  
Ilyas Khan ◽  
...  
Keyword(s):  
Analytical Approach ◽  
Intensity Interferometry

Hard Photon Intensity Interferometry in Heavy-Ion Collisions at Intermediate Energies

1996 ◽  
pp. 91-98
Author(s):  
A. Badalà ◽  
R. Barbera ◽  
A. Palmeri ◽  
G. S. Pappalardo ◽  
F. Riggi ◽  
...  
Keyword(s):  
Heavy Ion Collisions ◽  
Heavy Ion ◽  
Hard Photon ◽  
Intensity Interferometry ◽  
Intermediate Energies ◽  
Ion Collisions ◽  
Photon Intensity

scholarly journals Improved Spatial Resolution Achieved by Chromatic Intensity Interferometry

2021 ◽  
Vol 127 (10) ◽  
Author(s):  
Lu-Chuan Liu ◽  
Luo-Yuan Qu ◽  
Cheng Wu ◽  
Jordan Cotler ◽  
Fei Ma ◽  
...  
Keyword(s):  
Spatial Resolution ◽  
Intensity Interferometry
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