Author pages are created from data sourced from our academic publisher partnerships and public sources.
- Publications
- Influence
Share This Author
Neutron Star Structure and the Equation of State(Nuclear Astrophysics,New Frontiers in QCD 2010-Exotic Hadron Systems and Dense Matter-)
- J. Lattimer, M. Prakash
- Physics
- 10 February 2000
The structure of neutron stars is considered from theoretical and observational perspectives. We demonstrate an important aspect of neutron star structure: the neutron star radius is primarily…
The Physics of Neutron Stars
- J. Lattimer, M. Prakash
- PhysicsScience
- 23 April 2004
TLDR
Evolution of Proto-Neutron Stars
- J. Pons, S. Reddy, M. Prakash, J. Lattimer, J. Miralles
- Physics
- 3 July 1998
We study the thermal and chemical evolution during the Kelvin-Helmholtz phase of the birth of a neutron star, employing neutrino opacities that are consistently calculated with the underlying…
The Equation of State of Hot, Dense Matter and Neutron Stars
- J. Lattimer, M. Prakash
- Physics
- 24 December 2015
Composition and structure of protoneutron stars
- M. Prakash, I. Bombaci, M. Prakash, P. Ellis, J. Lattimer, R. Knorren
- Physics
- 27 March 1996
Rapid Cooling and the Structure of Neutron Stars
- J. Lattimer, K. Riper, M. Prakash, M. Prakash
- Physics
- 1 April 1994
This report discusses the following topics on neutron stars: direct URCA neutrino emission; thermal evolution models; analytic model for diffusion through the crust; and core superfluidity. (LSP).
What a Two Solar Mass Neutron Star Really Means
- J. Lattimer, M. Prakash
- Physics
- 15 December 2010
The determination of neutron star masses is reviewed in light of a new measurement of 1.97 M$_\odot$ for PSR J1614-2230 and an estimate of 2.4 M$_\odot$ for the black widow pulsar. Using a simple…
Rapid cooling of neutron stars by hyperons and Delta isobars
- M. Prakash, M. Prakash, J. Lattimer, C. Pethick
- Physics
- 10 May 1992
It is shown that direct Urca processes with hyperons and/or nucleon isobars can occur in dense matter as long as the concentration of Λ hyperons exceeds a critical value that is less than 3% and is…
The Equation of State of Neutron Star Matter in Strong Magnetic Fields
- A. Broderick, M. Prakash, J. Lattimer
- Physics
- 31 January 2000
We study the effects of very strong magnetic fields on the equation of state (EOS) in multicomponent, interacting matter by developing a covariant description for the inclusion of the anomalous…
...
1
2
3
4
5
...