arXiv · 2001.09020
ν\barν -Pair Synchrotron Emission in Neutron-Star Matter based on a Relativistic Quantum Approach
Abstract
We study the neutrino anti-neutrino pair synchrotron emission from electrons and protons in a relativistic quantum approach. This process occurs only under a strong magnetic field, and it is considered to be one of effective processes for neutron star cooling. In this work we calculate the luminosity of the neutrino anti-neutrino pairs emitted from neutron-star-matter with a magnetic field of about 10^{15} G. We find that the energy loss is much larger than that of the modified Urca process. The neutrino anti-neutrino pair emission processes in strong magnetic fields is expected to contribute significantly to the cooling of the magnetars.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Tomoyuki Maruyama A. Baha Balantekin, Myung-Ki Cheoun, Toshitaka Kajino, Grant J. Mathews. 2020-04-03. ν\barν -Pair Synchrotron Emission in Neutron-Star Matter based on a Relativistic Quantum Approach. https://doi.org/10.1016/j.physletb.2020.135413
Cite the original work for its findings. Save a collection to share your selection of sources.