Neutrino-Pair Bremsstrahlung in Dense Stars. III. Low-Temperature Quantum Corrections in the Liquid Metal Phase: Erratum

1993 ◽  
Vol 404 ◽  
pp. 418 ◽  
Author(s):  
Naoki Itoh ◽  
Yasuharu Kohyama ◽  
Noriyoshi Matsumoto ◽  
Midori Seki
Keyword(s):  
Low Temperature ◽  
Liquid Metal ◽  
Quantum Corrections ◽  
Metal Phase ◽  
Neutrino Pair ◽  
Dense Stars

A Shape‐Variable, Low‐Temperature Liquid Metal–Conductive Polymer Aqueous Secondary Battery

2021 ◽  
pp. 2107062
Author(s):  
Hao Fu ◽  
Guicheng Liu ◽  
Lingyun Xiong ◽  
Manxiang Wang ◽  
Jeongwoo Lee ◽  
...  
Keyword(s):  
Low Temperature ◽  
Liquid Metal ◽  
Conductive Polymer ◽  
Shape Variable ◽  
Secondary Battery ◽  
Temperature Liquid

Molten iodide salt electrolyte for low-temperature low-cost sodium-based liquid metal battery

2020 ◽  
Vol 475 ◽  
pp. 228674
Author(s):  
Qing Gong ◽  
Wenjin Ding ◽  
Alexander Bonk ◽  
Haomiao Li ◽  
Kangli Wang ◽  
...  
Keyword(s):  
Low Temperature ◽  
Liquid Metal ◽  
Low Cost ◽  
Liquid Metal Battery

scholarly journals Neutrino-pair bremsstrahlung in dense stars

1984 ◽  
Vol 105 ◽  
pp. 355-356
Author(s):  
Naoki Itoh ◽  
Yasuharu Kohyama
Keyword(s):  
Neutron Stars ◽  
Liquid State ◽  
White Dwarfs ◽  
Dense Matter ◽  
Waller Factor ◽  
Bcc Lattice ◽  
Debye Waller Factor ◽  
Lattice State ◽  
Neutrino Pair ◽  
Dense Stars

Neutrino-pair bremsstrahlung rate is calculated in the framework of the Weinberg-Salam theory for the dense matter relevant to the interior of white dwarfs and neutron stars. Ionic correlations both in the liquid state and in the bcc lattice state have been taken into account accurately. It is found that the ionic correlation in the liquid state reduces the neutrino-pair bremsstrahlung rate typically by a factor 2–20 depending on the element and temperature. It is also found that accurate inclusion of the Debye-Waller factor reduces the neutrino-pair bremsstrahlung rate in the lattice state typically by a factor 2.

scholarly journals Transport Processes in Dense Stellar Plasmas

1994 ◽  
Vol 147 ◽  
pp. 394-419
Author(s):  
Naoki Itoh
Keyword(s):  
Thermal Conductivity ◽  
Electrical Conductivity ◽  
Liquid Metal ◽  
Neutron Stars ◽  
Transport Properties ◽  
Dense Matter ◽  
Transport Processes ◽  
Crystalline Lattice ◽  
Metal Phase ◽  
Current Status

AbstractTransport processes in dense stellar plasmas which are relevant to the interiors of white dwarfs and neutron stars are reviewed. The emphasis is placed on the accuracy of the numerical results. In this review we report on the electrical conductivity and the thermal conductivity of dense matter. The methods of the calculations are different for the liquid metal phase and the crystalline lattice phase. We will broadly review the current status of the calculations of the transport properties of dense matter, and try to give the best instructions available at the present time to the readers.

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