Abstract
The role of neutrinos in the core of a star that has undergone a supernova explosion is discussed. The existence of neutron stars, the Schwarzchild singularity in general relativity, and the meaning of conservation of baryons in the neighborhood of a Schwarzchild singularity are also considered. The problem of detection of neutron stars is discussed. It is concluded that neutron stars are the most plausible alternative for the remnant of the core of a supernova. The neutrino emission processes are divided into two groups: the neutrino associated with the meson (mu) and the production of electron neutrinos. (C.E.S.)
Citation Formats
Chiu, H Y.
SUPERNOVAE, NEUTRON STARS, AND TWO KINDS OF NEUTRINO.
United States: N. p.,
1962.
Web.
Chiu, H Y.
SUPERNOVAE, NEUTRON STARS, AND TWO KINDS OF NEUTRINO.
United States.
Chiu, H Y.
1962.
"SUPERNOVAE, NEUTRON STARS, AND TWO KINDS OF NEUTRINO."
United States.
@misc{etde_4875515,
title = {SUPERNOVAE, NEUTRON STARS, AND TWO KINDS OF NEUTRINO}
author = {Chiu, H Y}
abstractNote = {The role of neutrinos in the core of a star that has undergone a supernova explosion is discussed. The existence of neutron stars, the Schwarzchild singularity in general relativity, and the meaning of conservation of baryons in the neighborhood of a Schwarzchild singularity are also considered. The problem of detection of neutron stars is discussed. It is concluded that neutron stars are the most plausible alternative for the remnant of the core of a supernova. The neutrino emission processes are divided into two groups: the neutrino associated with the meson (mu) and the production of electron neutrinos. (C.E.S.)}
place = {United States}
year = {1962}
month = {Aug}
}
title = {SUPERNOVAE, NEUTRON STARS, AND TWO KINDS OF NEUTRINO}
author = {Chiu, H Y}
abstractNote = {The role of neutrinos in the core of a star that has undergone a supernova explosion is discussed. The existence of neutron stars, the Schwarzchild singularity in general relativity, and the meaning of conservation of baryons in the neighborhood of a Schwarzchild singularity are also considered. The problem of detection of neutron stars is discussed. It is concluded that neutron stars are the most plausible alternative for the remnant of the core of a supernova. The neutrino emission processes are divided into two groups: the neutrino associated with the meson (mu) and the production of electron neutrinos. (C.E.S.)}
place = {United States}
year = {1962}
month = {Aug}
}