The role of the equation of state in the structure of neutron stars is summarized. At densities beyond a few times the normal nuclear saturation density, the neutron-proton-electron sea can be supplemented with more exotic matter, usually involving strangeness, such as hyperons, kaon or pion condens
β¦ LIBER β¦
Equation of state of the alpha and epsilon phases of iron
β Scribed by D.J. Andrews
- Publisher
- Elsevier Science
- Year
- 1972
- Tongue
- English
- Weight
- 71 KB
- Volume
- 11
- Category
- Article
- ISSN
- 0038-1098
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Equation of state, neutron stars and exo
β
James M. Lattimer; Madappa Prakash
π
Article
π
2006
π
Elsevier Science
π
English
β 580 KB
Thermal equation of state of iron and Fe
β
J. Zhang; F. Guyot
π
Article
π
1999
π
Springer-Verlag
π
English
β 105 KB
Schiestel's derivation of the epsilon eq
β
R. Rubinstein; Ye Zhou
π
Article
π
2003
π
Elsevier Science
π
English
β 391 KB
As part of a more general program of developing multiple-scale models of turbulence, Schiestel suggested a derivation of the homogeneous part of the dissipation rate transport equation. Schiestel's approach is generalized to rotating turbulence. The resulting model reproduces the main features obser
An equation of state for methane in the
β
A. J. Vennix; Riki Kobayashi
π
Article
π
1969
π
American Institute of Chemical Engineers
π
English
β 716 KB
RedlichβKwong equation of state: an anal
β
A.L. Horvath
π
Article
π
1972
π
Elsevier Science
π
English
β 326 KB
a position of moving boundary b constant defined by Eq. ( 12) c concentration D diffisivity K constant defined by Eq. ( 9)
Equation of State and Phase Diagram of Q
β
A. V. Petrovtsev; V. V. Dremov; V. G. Vildanov; M. M. Gorshkov; V. T. Zahikin; Y
π
Article
π
2006
π
John Wiley and Sons
β 8 KB
π 1 views