NSR Query Results

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NSR database version of April 11, 2024.

Search: Author = P.Krastev

Found 19 matches.

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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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2010JO04      Phys.Rev. C 81, 054303 (2010)

C.W.Johnson, P.G.Krastev

Sensitivity analysis of random two-body interactions

doi: 10.1103/PhysRevC.81.054303
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2007KR16      Phys.Rev. C 76, 055804 (2007)

P.G.Krastev, B.-A.Li

Constraining a possible time variation of the gravitational constant G with terrestrial nuclear laboratory data

doi: 10.1103/PhysRevC.76.055804
Citations: PlumX Metrics

2007SA15      Phys.Rev. C 75, 034315 (2007)

F.Sammarruca, P.G.Krastev

Spin polarized neutron matter within the Dirac-Brueckner-Hartree-Fock approach

doi: 10.1103/PhysRevC.75.034315
Citations: PlumX Metrics

2006KR05      Phys.Rev. C 74, 025808 (2006); Erratum Phys.Rev. C 74, 039901 (2006)

P.G.Krastev, F.Sammarruca

Neutron star properties and the equation of state of neutron-rich matter

doi: 10.1103/PhysRevC.74.025808
Citations: PlumX Metrics

2006SA02      Phys.Rev. C 73, 014001 (2006)

F.Sammarruca, P.Krastev

Effective nucleon-nucleon cross sections in symmetric and asymmetric nuclear matter

doi: 10.1103/PhysRevC.73.014001
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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 T_1/2, 0ν-accompanied 2β-decay T_1/2 lower limit.

doi: 10.1016/S0920-5632(02)01514-1
Citations: PlumX Metrics

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
Citations: PlumX Metrics

1998BA84      Phys.Lett. 436B, 243 (1998)

J.N.Bahcall, P.I.Krastev

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

1997BA11      Phys.Rev. C55, 929 (1997)

J.N.Bahcall, P.I.Krastev

What Can Be Learned by Measuring the Fluxes of the ⁷Be and the pep Solar Neutrino Lines ( Question )

doi: 10.1103/PhysRevC.55.929
Citations: PlumX Metrics

1997BA73      Phys.Rev. C56, 2839 (1997)

J.N.Bahcall, P.I.Krastev

Does the Sun Appear Brighter at Night in Neutrinos ( Question )

doi: 10.1103/PhysRevC.56.2839
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

1995EN03      Phys.Rev. C51, 2837 (1995)

J.Engel, P.I.Krastev, K.Lande

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
Citations: PlumX Metrics

Note: The following list of authors and aliases matches the search parameter P.Krastev: , P.G.KRASTEV, P.I.KRASTEV