A new equation of state for dense matter and fast rotating pulsars

Details A new equation of state for dense matter and fast rotating pulsars A new equation of state for dense matter and fast rotating pulsars

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...246..411w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 246, no. 2, June 1991, p. 411-416.

Physics

Condensed Matter

20

Condensed Matter Physics, Equations Of State, Neutron Stars, Pulsars, Stellar Models, Stellar Rotation, Angular Velocity, Momentum Transfer, Relativistic Effects, Stellar Mass

Scientific paper

A new equation of state (EOS) for condensed matter above nuclear density
is presented. Several arguments are brought forward why most EOS,
derived from laboratory data, might actually be too stiff. The new EOS
leads to neutron star models with an upper mass limit of 1.56 solar mass
and rotation periods less than 0.5 msec.

Affiliated with

Also associated with

No associations

Rating

A new equation of state for dense matter and fast rotating pulsars 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 A new equation of state for dense matter and fast rotating pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A new equation of state for dense matter and fast rotating pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1277741