Results 51 to 60 of about 241,450 (255)
Cosmological neutrino mass detection: The best probe of neutrino lifetime [PDF]
, 2007 Future cosmological data may be sensitive to the effects of a finite sum of neutrino masses even as small as ~0.06 eV, the lower limit guaranteed by neutrino oscillation experiments.
Serpico, Pasquale D.
core +2 more sources
Symmetry Finder applied to the 1–3 mass eigenstate exchange symmetry
European Physical Journal C: Particles and Fields, 2021 In a previous paper, Symmetry Finder (SF) method is proposed to find the reparametrization symmetry of the state-exchange type in neutrino oscillation in matter.
Hisakazu Minakata
doaj +1 more source
Investigation of the Hue–Wavelength Response of a CMOS RGB-Based Image Sensor
Sensors, 2022 In this study, a non-linear hue–wavelength (H-W) curve was investigated from 400 to 650 nm. To date, no study has reported on H-W relationship measurements, especially down to the 400 nm region.
Hyeon-Woo Park +4 more
doaj +1 more source
Tachyonic neutrinos and the neutrino masses [PDF]
Astroparticle Physics, 2013 18 pages, 2 ...
openaire +3 more sources
Journal of High Energy Physics, 2019 Abstract Clockwork (CW) mechanism can explain the smallness of neutrino masses without introducing unnaturally small input parameters. In this paper we study the simplest CW neutrino model, the “uniform” clockwork, as well as a broader class of “generalized” clockwork models.
Hong, Sungwoo +2 more
openaire +4 more sources
Solar Neutrinos Before and After Neutrino 2004 [PDF]
, 2004 We compare, using a three neutrino analysis, the allowed neutrino oscillation parameters and solar neutrino fluxes determined by the experimental data available Before and After Neutrino 2004. New data available after Neutrino2004 include refined KamLAND
Bahcall, John N. +2 more
core +4 more sources
Astronomische Nachrichten, EarlyView.ABSTRACT We investigate the effects of a minimal measurable length on neutron stars, within the quantum hadrodynamics (QHD‐I) model modified by the Generalized Uncertainty Principle (GUP). Working in a deformed Poisson algebra framework, we incorporate GUP effects via a time‐invariant transformation of the phase space volume, effectively reducing the ...
João Gabriel Galli Gimenez +2 more
wiley +1 more source
Journal of High Energy Physics, 2014 The Standard Model of particle physics fails to explain the important pieces in the standard cosmology, such as inflation, baryogenesis, and dark matter of the Universe. We consider the possibility that the sector to generate small neutrino masses is responsible for all of them; the inflation is driven by the Higgs field to break $B-L$ gauge symmetry ...
Higaki, Tetsutaro +2 more
openaire +2 more sources
, 2011 Core-collapse supernova neutrinos undergo a variety of phenomena when they travel from the high neutrino density region and large matter densities to the Earth.
+28 more
core +3 more sources
Thermal neutrinos from pre-supernova [PDF]
, 2006 We would like to discuss prospects for neutrino observations of the core-collapse supernova progenitor during neutrino-cooled stage. We will present new theoretical results on thermal neutrino and antineutrino spectra produced deep inside the pre ...
A. Odrzywolek +6 more
core +3 more sources