Results 161 to 170 of about 41,366 (209)
Photon strength functions and nuclear level densities: invaluable input for nucleosynthesis. [PDF]
Wiedeking M, Goriely S.
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Gamma noise to non-invasively monitor nuclear research reactors. [PDF]
Pakari O +4 more
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Water can trigger nuclear reaction to produce energy and isotope gases. [PDF]
Huang BJ +18 more
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Micromegas with GEM preamplification for enhanced energy threshold in low-background gaseous time projection chambers. [PDF]
Castel Pablo JF +15 more
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Primordial black holes and their gravitational-wave signatures. [PDF]
Bagui E +20 more
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Evaluation of Daughter Radionuclide Release from the 103Pd/103mRh In Vivo Generator for Targeted Auger Therapy. [PDF]
Laouameria AN +6 more
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Reviews of Modern Physics, 1978
New results are presented for absorption cross sections of nine possible detectors of solar neutrinos ($^{7}\mathrm{Li}$, $^{37}\mathrm{Cl}$, $^{51}\mathrm{V}$, $^{55}\mathrm{Mn}$, $^{71}\mathrm{Ga}$, $^{81}\mathrm{Br}$, $^{87}\mathrm{Rb}$, $^{115}\mathrm{In}$, and $^{205}\mathrm{Tl}$). Special attention is given to nuclear physics uncertainties.
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New results are presented for absorption cross sections of nine possible detectors of solar neutrinos ($^{7}\mathrm{Li}$, $^{37}\mathrm{Cl}$, $^{51}\mathrm{V}$, $^{55}\mathrm{Mn}$, $^{71}\mathrm{Ga}$, $^{81}\mathrm{Br}$, $^{87}\mathrm{Rb}$, $^{115}\mathrm{In}$, and $^{205}\mathrm{Tl}$). Special attention is given to nuclear physics uncertainties.
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Physical Review Letters, 1985
The theory of oscillations of solar neutrinos is developed as it applies to the electron-recoil spectrum in neutrino-electron scattering. The spectral information obtained by such measurements (as opposed to counting total event rates) is crucial for allowing observation of neutrino oscillations for masses down to 500 neV.
, Krauss, , Wilczek
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The theory of oscillations of solar neutrinos is developed as it applies to the electron-recoil spectrum in neutrino-electron scattering. The spectral information obtained by such measurements (as opposed to counting total event rates) is crucial for allowing observation of neutrino oscillations for masses down to 500 neV.
, Krauss, , Wilczek
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