Results 171 to 180 of about 41,603 (215)

Multi-messenger gravitational lensing. [PDF]

Philos Trans A Math Phys Eng Sci
Smith GP, Baker T, Birrer S, Collins CE, Ezquiaga JM, Goyal S, Hannuksela OA, Hemanta P, Hendry MA, Janquart J, Keitel D, Levan AJ, Lo RKL, More A, Nicholl M, Pastor-Marazuela I, Ponte Pérez AI, Ubach H, Uronen LE, Wright M, Zumalacarregui M, Bianco F, Çalişkan M, Chan JCL, Colangeli E, Gompertz BP, Haines CP, Hayes EE, Hu B, Lamb GP, Liu A, Mandhai S, Narola H, Nguyen QL, Poon JSC, Ryczanowski D, Seo E, Shajib AJ, Shan X, Tanvir N, Vujeva L.   +40 more
europepmc   +1 more source

Photon strength functions and nuclear level densities: invaluable input for nucleosynthesis. [PDF]

Philos Trans A Math Phys Eng Sci
Wiedeking M, Goriely S.
europepmc   +1 more source

Overview of the ESCAPE Dark Matter Test Science Project for astronomers. [PDF]

Open Res Eur
Pearson J, Dickinson H, Sinha S, Serjeant S.   +3 more
europepmc   +1 more source

Gamma noise to non-invasively monitor nuclear research reactors. [PDF]

Sci Rep
Pakari O, Mager T, Frajtag P, Pautz A, Lamirand V.   +4 more
europepmc   +1 more source

Water can trigger nuclear reaction to produce energy and isotope gases. [PDF]

Sci Rep
Huang BJ, Pan YH, Wu PH, Yeh JF, Tso ML, Liu YH, Wu L, Huang CK, Chen IF, Lin CH, Tseng TR, Kang FW, Tsai TF, Lan KC, Chen YT, Liao MY, Xu L, Chen SL, Greenyer RW.   +18 more
europepmc   +1 more source

Micromegas with GEM preamplification for enhanced energy threshold in low-background gaseous time projection chambers. [PDF]

Open Res Eur
Castel Pablo JF, Cebrián Guajardo S, Dafni T, Díez Ibáñez D, Galán Lacarra J, García Pascual JA, Ezquerro Sastre Á, García Irastorza I, Luzón Marco G, Margalejo Blasco C, Mirallas Sánchez H, Obis Aparicio L, Ortiz de Solórzano A, Pérez Lázaro Ó, Porrón Lafuente J, Jiménez Puyuelo M.   +15 more
europepmc   +1 more source

The Solar Neutrino Problem [PDF]

Annual Review of Astronomy and Astrophysics, 1995
The solar neutrino problem has persisted for almost three decades. Recent results from Kamiokande, SAGE, and GALLEX indicate a pattern of neutrino fluxes that is very difficult to reconcile with plausible variations in standard solar models. This situation is reviewed, and suggested particle physics solutions are discussed.
W C Haxton
exaly   +3 more sources

Solar neutrinos and neutrino physics [PDF]

European Physical Journal A, 2016
Solar neutrino studies triggered and largely motivated the major developmentsin neutrino physics in the last 50 years. Theory of neutrino propagation indifferent media with matter and fields has been elaborated. It includesoscillations in vacuum and matter, resonance flavor conversion and resonanceoscillations, spin and spin-flavor precession, etc. LMA
Michele Maltoni, Alexei Yu Smirnov
exaly   +5 more sources

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Neutrino oscillations and the solar-neutrino problem

Physical Review D, 1987
The values of neutrino masses and mixing angles which are required by the Mikheyev-Smirnov-Wolfenstein (MSW) solution to the solar-neutrino problem are found from analytic solutions to the neutrino propagation equations in the Sun. They coincide with those obtained through extensive numerical computations by Rosen and Gelb.
, Dar, , Mann, , Melina, , Zajfman
openaire   +2 more sources