Abstract
Relativistic equations of structure are solved using Lamb's equations of state for warm neutron degenerate matter. The stability of isothermal cores in neutron stars is discussed and also the possible compatibility of the results obtained with experimental evidence is shown.
Ibanez Cabanell, J M
[1]
- Departamento de Mecanica y Astronomia, Facultad de Matematicas, Burjasot-Valencia (Spain)
Citation Formats
Ibanez Cabanell, J M.
Structure and stability of warm cores in neutron stars.
United Kingdom: N. p.,
1981.
Web.
Ibanez Cabanell, J M.
Structure and stability of warm cores in neutron stars.
United Kingdom.
Ibanez Cabanell, J M.
1981.
"Structure and stability of warm cores in neutron stars."
United Kingdom.
@misc{etde_5385309,
title = {Structure and stability of warm cores in neutron stars}
author = {Ibanez Cabanell, J M}
abstractNote = {Relativistic equations of structure are solved using Lamb's equations of state for warm neutron degenerate matter. The stability of isothermal cores in neutron stars is discussed and also the possible compatibility of the results obtained with experimental evidence is shown.}
journal = []
volume = {197:3}
journal type = {AC}
place = {United Kingdom}
year = {1981}
month = {Dec}
}
title = {Structure and stability of warm cores in neutron stars}
author = {Ibanez Cabanell, J M}
abstractNote = {Relativistic equations of structure are solved using Lamb's equations of state for warm neutron degenerate matter. The stability of isothermal cores in neutron stars is discussed and also the possible compatibility of the results obtained with experimental evidence is shown.}
journal = []
volume = {197:3}
journal type = {AC}
place = {United Kingdom}
year = {1981}
month = {Dec}
}