Volume 281 - The 26th International Nuclear Physics Conference (INPC2016) - Neutrinos and Nuclei – Thursday 15
Asymmetric Neutrino Emissions In Strongly Magnetized Matter In Relativistic Quantum Approach
T. Maruyama*, T. Kajino, M.K. Cheoun and G.J. Mathews
*: corresponding author
Full text: pdf
Pre-published on: May 04, 2017
Published on: May 09, 2017
Abstract
We study a cooling process of magnetars through the neutrino-antineutrino pair emission from electron and proton,
which occurs only under the strong magnetic field, in the exact quantum calculation. Our results show that the luminosity is proportional to T**(0:95-1:7) when the magnetic fields are B = 10**15 -101**6G. The powers of the temperature are much smaller than those in the direct Urca and moderate Urca processes. Thus, the nu nubar -pair emission processes by the strong magnetic field is expected to
contribute very largely to the cooling process of the magnetar.
DOI: https://doi.org/10.22323/1.281.0252
How to cite

Metadata are provided both in article format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in proceeding format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.