Results 141 to 150 of about 67,992 (214)

Scientific program for the Forward Physics Facility. [PDF]

Eur Phys J C Part Fields
Adhikary J, Anchordoqui LA, Ariga A, Ariga T, Barr AJ, Batell B, Bian J, Boyd J, Citron M, De Roeck A, Diwan MV, Feng JL, Hill CS, Jeong YS, Kling F, Linden S, Mäkelä T, Mavrokoridis K, McFayden J, Otono H, Rojo J, Soldin D, Stasto A, Trojanowski S, Vicenzi M, Wu W.   +25 more
europepmc   +1 more source

The Revised Solar Abundance of Iron and the Solar Neutrino Flux

, 1969
W. D. Watson
openalex   +1 more source

Particle swarm optimization based analysis to unlocking the neutrino mass puzzle using [Formula: see text] flavor symmetry. [PDF]

Sci Rep
Aslam MW, Zafar AA, Aslam MN, Bhatti AA, Hussain T, Iqbal M, Abdo MS.   +6 more
europepmc   +1 more source

Neutrino Emission and a Possible Model for Pre-White Dwarf Stars.

, 1962
Hong‐Yee Chiu, P. Morrison, H. Reeves
openalex   +2 more sources

Direct experimental constraints on the spatial extent of a neutrino wavepacket. [PDF]

Nature
Smolsky J, Leach KG, Abells R, Amaro P, Andoche A, Borbridge K, Bray C, Cantor R, Diercks D, Fretwell S, Friedrich S, Gillespie A, Guerra M, Hall A, Harris CN, Harris JT, Hayen LM, Hervieux PA, Hinkle C, Kim GB, Kim I, Lamm A, Lennarz A, Lordi V, Machado J, Marino A, McKeen D, Mougeot X, Ponce F, Ruiz C, Samanta A, Santos JP, Stone-Whitehead C, Taylor J, Templet J, Upadhyayula S, Wagner L, Warburton WK.   +37 more
europepmc   +1 more source

Observation of an ultra-high-energy cosmic neutrino with KM3NeT. [PDF]

Nature
KM3NeT Collaboration.
europepmc   +1 more source

Charge Ratio of Produced Pions in Neutrino Inelastic Scattering [PDF]

, 1965
M. Fukawa
openalex   +1 more source

Sensitivity Challenge of the Next-Generation Bolometric Double-Beta Decay Experiment. [PDF]

Research (Wash D C)
Ma L, Huang HZ, Ma YG.
europepmc   +1 more source

Flavored resonant leptogenesis in the U(1)X model

Nuclear Physics B
We study the generation of baryon asymmetry through the flavored resonant leptogenesis in the U(1)X extension of the Standard Model. Being a generalization of the U(1)B-L, U(1)X is an ultraviolet-complete model of the right-handed neutrinos (RHNs), whose
Garv Chauhan
doaj  

Pre-White Dwarf Evolution and Neutrino Emission

, 1966
Chao-Wen Chin, Hong‐Yee Chiu, Richard B. Stothers   +2 more
openalex   +2 more sources