NSR Query Results

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NSR database version of April 29, 2024.

Search: Author = P.I.Krastev

Found 7 matches.

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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
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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
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