Stationary elastic rotational deformation of a relativistic neutron star model

Details Stationary elastic rotational deformation of a relativistic neutron star model Stationary elastic rotational deformation of a relativistic neutron star model

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...202..511c&link_type=abstract

Astrophysical Journal, vol. 202, Dec. 1, 1975, pt. 1, p. 511-522.

Astronomy and Astrophysics

Astrophysics

18

Astronomical Models, Elastic Deformation, Neutron Stars, Pulsars, Relativistic Theory, Stellar Rotation, Angular Momentum, Angular Velocity, Euler-Lagrange Equation, Mathematical Models, Relativistic Effects, Relativity, Starquakes, Tensor Analysis

Scientific paper

In order to predict pulsar glitch magnitudes in terms of the Ruderman starquake theory, it is necessary to calculate the deviation from perfect fluid behavior when a stationary rotating partly solid neutron star undergoes an elastic deformation due to a change in angular momentum. Previous calculations have been based on crude Newtonian or semi-Newtonian approximations. The present work describes the way to solve this problem exactly (in the small-deformation limit) using a fully relativistic treatment.

Affiliated with

Also associated with

No associations

Rating

Stationary elastic rotational deformation of a relativistic neutron star model 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 Stationary elastic rotational deformation of a relativistic neutron star model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stationary elastic rotational deformation of a relativistic neutron star model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1576767