NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = P.Krastev Found 19 matches. 2019LI39 Eur.Phys.J. A 55, 117 (2019) B.-A.Li, P.G.Krastev, D.-H.Wen, N.-B.Zhang Towards understanding astrophysical effects of nuclear symmetry energy
doi: 10.1140/epja/i2019-12780-8
2011LI54 J.Phys.:Conf.Ser. 312, 042006 (2011) B.-A.Li, L.-W.Chen, M.Gearheart, J.Hooker, C.M.Ko, P.G.Krastev, W.-K.Lin, W.G.Newton, D.-H.Wen, C.Xu, J.Xu Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars
doi: 10.1088/1742-6596/312/4/042006
2010JO04 Phys.Rev. C 81, 054303 (2010) Sensitivity analysis of random two-body interactions
doi: 10.1103/PhysRevC.81.054303
2009WE03 Phys.Rev. C 80, 025801 (2009) D.-H.Wen, B.-A.Li, P.G.Krastev Imprints of the nuclear symmetry energy on gravitational waves from the axial w-modes of neutron stars
doi: 10.1103/PhysRevC.80.025801
2008LI09 J.Phys.(London) G35, 014044 (2008) B.-A.Li, L.-W.Chen, C.M.Ko, P.G.Krastev, A.W.Steiner, G.-C.Yong Constraining properties of neutron stars with heavy-ion reactions in terrestrial laboratories
doi: 10.1088/0954-3899/35/1/014044
2007KR16 Phys.Rev. C 76, 055804 (2007) Constraining a possible time variation of the gravitational constant G with terrestrial nuclear laboratory data
doi: 10.1103/PhysRevC.76.055804
2007SA15 Phys.Rev. C 75, 034315 (2007) Spin polarized neutron matter within the Dirac-Brueckner-Hartree-Fock approach
doi: 10.1103/PhysRevC.75.034315
2006KR05 Phys.Rev. C 74, 025808 (2006); Erratum Phys.Rev. C 74, 039901 (2006) Neutron star properties and the equation of state of neutron-rich matter
doi: 10.1103/PhysRevC.74.025808
2006SA02 Phys.Rev. C 73, 014001 (2006) Effective nucleon-nucleon cross sections in symmetric and asymmetric nuclear matter
doi: 10.1103/PhysRevC.73.014001
2005SA36 Phys.Rev. C 71, 064306 (2005) F.Sammarruca, W.Barredo, P.Krastev Predicting the single-proton and single-neutron potentials in asymmetric nuclear matter
doi: 10.1103/PhysRevC.71.064306
2002EJ05 Nucl.Phys. B(Proc.Supp.) S110, 375 (2002) H.Ejiri, J.Engel, K.Fushimi, K.Hayashi, R.Hazama, T.Kishimoto, P.Krastev, N.Kudomi, K.Kume, H.Kuramoto, K.Matsuoka, R.G.H.Robertson, K.Takahisa, S.Yoshida Double Beta Decays of 100Mo and Molybdenum Observatory of Neutrinos RADIOACTIVITY 100Mo(2β-); measured β-spectra, 2ν-accompanied 2β-decay T1/2, 0ν-accompanied 2β-decay T1/2 lower limit.
doi: 10.1016/S0920-5632(02)01514-1
2000EJ01 Phys.Rev.Lett. 85, 2917 (2000) H.Ejiri, J.Engel, R.Hazama, P.Krastev, N.Kudomi, R.G.H.Robertson Spectroscopy of Double-Beta and Inverse-Beta Decays from 100Mo for Neutrinos RADIOACTIVITY 100Mo(2β-); calculated 0ν-, 2ν-accompanied 2β decay spectra, correlation features. Detector design, solar neutrino detection discussed.
doi: 10.1103/PhysRevLett.85.2917
1998BA84 Phys.Lett. 436B, 243 (1998) Do hep Neutrinos Affect the Solar Neutrino Energy Spectrum ? NUCLEAR REACTIONS 3He(p, e+ν), E=low; analyzed σ, relationship to solar neutrino flux.
doi: 10.1016/S0370-2693(98)00920-4
1997BA03 Phys.Rev. C55, 494 (1997) J.N.Bahcall, P.I.Krastev, E.Lisi Neutrino Oscillations and Moments of Electron Spectra NUCLEAR STRUCTURE 8B; calculated neutrino oscillations effects on solar neutrino; deduced energy distribution first two moments to be sufficient.
doi: 10.1103/PhysRevC.55.494
1997BA11 Phys.Rev. C55, 929 (1997) What Can Be Learned by Measuring the Fluxes of the 7Be and the pep Solar Neutrino Lines ( Question )
doi: 10.1103/PhysRevC.55.929
1997BA73 Phys.Rev. C56, 2839 (1997) Does the Sun Appear Brighter at Night in Neutrinos ( Question )
doi: 10.1103/PhysRevC.56.2839
1996BA30 Phys.Lett. 374B, 1 (1996) J.N.Bahcall, M.Fukugita, P.I.Krastev How Does the Sun Shine ( Question )
doi: 10.1016/0370-2693(96)00187-6
1995BA31 Phys.Lett. 348B, 121 (1995) J.N.Bahcall, P.I.Krastev, E.Lisi Limits on Electron-Neutrino Oscillations from the GALLEX 51Cr Source Experiment
doi: 10.1016/0370-2693(95)00111-W
1995EN03 Phys.Rev. C51, 2837 (1995) What Can be Learned with an Iodine Solar-Neutrino Detector ( Question ) NUCLEAR REACTIONS 127I(ν, e-), E=solar; calculated Iso-SNU contours for Iodine detector, event rates; deduced Δm2-Sin22θ parameter space allowed region distinguishing possibility.
doi: 10.1103/PhysRevC.51.2837
Back to query form Note: The following list of authors and aliases matches the search parameter P.Krastev: , P.G.KRASTEV, P.I.KRASTEV |