Results 221 to 230 of about 44,435 (241)
Mathematical Modeling of Physical Reality: From Numbers to Fractals, Quantum Mechanics and the Standard Model. [PDF]
Entropy (Basel)Kupczynski M.
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The waning of the WIMP: endgame? [PDF]
Eur Phys J C Part FieldsArcadi G +9 more
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International Journal of Modern Physics A, 1998
The current status of solar neutrino experiments is reviewed. All the experimental measurements show deficits of solar neutrinos. Non monotonic suppression indicates that the problem may naturally be explained by neutrino oscillations, but not by modifying solar models. A new experiment shows very promising results.
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The current status of solar neutrino experiments is reviewed. All the experimental measurements show deficits of solar neutrinos. Non monotonic suppression indicates that the problem may naturally be explained by neutrino oscillations, but not by modifying solar models. A new experiment shows very promising results.
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Nuclear Instruments and Methods, 1973
The observed capture rate for solar neutrinos in the 37Cl detector is lower than the predicted capture rate. This discrepancy between theory and observation is known as the ‘solar neutrino problem’. I review the basic elements in this problem: the detector efficiency, the theory of stellar (solar) evolution, the nuclear physics of energy generation ...
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The observed capture rate for solar neutrinos in the 37Cl detector is lower than the predicted capture rate. This discrepancy between theory and observation is known as the ‘solar neutrino problem’. I review the basic elements in this problem: the detector efficiency, the theory of stellar (solar) evolution, the nuclear physics of energy generation ...
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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.
Lawrence M. Krauss, Frank 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.
Lawrence M. Krauss, Frank Wilczek
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Nonaccelerator Astroparticle Physics, 2002
Neutrinos have been and are abundantly produced in the Universe and neutrino astronomy provides very rich information either in astrophysics or in particle physics. We focus in this review on neutrinos as witnesses of the life of stars (solar neutrinos) and on neutrinos as messengers of the death of stars (supernov= neutrinos).
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Neutrinos have been and are abundantly produced in the Universe and neutrino astronomy provides very rich information either in astrophysics or in particle physics. We focus in this review on neutrinos as witnesses of the life of stars (solar neutrinos) and on neutrinos as messengers of the death of stars (supernov= neutrinos).
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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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