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Иш: Rotating stars in relativity
Dark energy or modified gravity? An effective field theory approach
Jolyon Bloomfield, Éanna É. Flanagan, Minjoon Park +1
Мақола20132 иқтибосABICONSTRAINING THE SYMMETRY PARAMETERS OF THE NUCLEAR INTERACTION
James M. Lattimer, Yeunhwan Lim
Мақола20132 иқтибосABIOn the Nature of Core-Collapse Supernova Explosions
Adam Burrows, John Hayes, Bruce A. Fryxell
Мақола19952 иқтибосABILedoux convection in protoneutron stars - a clue to supernova nucleosynthesis?
Keil, W., Janka, H.T., Mueller, E. +1
Мақола19962 иқтибосABIOn the nature of core-collapse supernova explosions
Burrows, A, Hayes, J, Fryxell, B
Мақола19952 иқтибосABIGravitational waves from the collapse of rotating stellar cores
R. Moênchmeyer, G. Schaêfer, E. Müeller +1
Мақола19912 иқтибосABIStability of nonradial oscillations of cold nonrotating neutron stars
L. Battiston, P. Cazzola, L. Lucaroni
Мақола19712 иқтибосABIRotational modes of relativistic stars: Numerical results
Keith H. Lockitch, John L. Friedman, Nils Andersson
Мақола20032 иқтибосABIDOUBLE COMPACT OBJECTS. III. GRAVITATIONAL-WAVE DETECTION RATES
Michal Dominik, Emanuele Berti, Richard O’Shaughnessy +6
Мақола20152 иқтибосABIRelativistic g-modes in rapidly rotating neutron stars
Erich Gaertig, Kostas D. Kokkotas
Мақола20092 иқтибосABI