Internal structure of cool superdense stars with a frozen-in magnetic field

Details Internal structure of cool superdense stars with a frozen-in magnetic field Internal structure of cool superdense stars with a frozen-in magnetic field

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976sva....19..698s&link_type=abstract

(Astronomicheskii Zhurnal, vol. 52, Nov.-Dec. 1975, p. 1166-1172.) Soviet Astronomy, vol. 19, no. 6, 1976, p. 698-702. Translat

Astronomy and Astrophysics

Astronomy

Magnetic Stars, Pulsars, Stellar Interiors, Stellar Magnetic Fields, Stellar Structure, Electron Density (Concentration), Pair Production, Proton Density (Concentration), Thermodynamic Equilibrium, Trapped Magnetic Fields

Scientific paper

It is shown that the concentration of protons (electrons) at the
densities near the nuclear density depends on magnetic field, the
strength of which has a value of at least ten to the eighteenth gs. The
limits of the applicability of anomalous magnetic moment of electron are
discussed.

Affiliated with

Also associated with

No associations

Rating

Internal structure of cool superdense stars with a frozen-in magnetic field 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 Internal structure of cool superdense stars with a frozen-in magnetic field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Internal structure of cool superdense stars with a frozen-in magnetic field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1785309