Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-06-11
Phys.Rev.D76:125007,2007
Astronomy and Astrophysics
Astrophysics
11 pages, 6 figures
Scientific paper
10.1103/PhysRevD.76.125007
We derive the energy asymmetry given the proto-neutron star during the time when the neutrino sphere is near the surface of the proto-neutron star, using the modified URCA process. The electrons produced with the anti-neutrinos are in Landau levels due to the strong magnetic field, and this leads to asymmetry in the neutrino momentum, and a pulsar kick. The magnetic field must be strong enough for a large fraction of the eletrons to be in the lowest Landau level, however, there is no direct dependence of our pulsar velocity on the strength of the magnetic field. Our main prediction is that the large pulsar kicks start at about 10 s and last for about 10 s, with the corresponding neutrinos correlated in the direction of the magnetic field. We predict a pulsar velocity of 1.03 $\times 10^{-4} (T/10^{10}K)^7$ km/s, which reaches 1000 km/s if T $\simeq 9.96 \times 10^{10}$ K.
Henley Ernest M.
Johnson Mikkel B.
Kisslinger Leonard S.
No associations
LandOfFree
Pulsar Kicks With Modified URCA and Electrons in Landau Levels does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Pulsar Kicks With Modified URCA and Electrons in Landau Levels, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulsar Kicks With Modified URCA and Electrons in Landau Levels will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-179686