Results 41 to 50 of about 239,431 (169)
Just-So Oscillation: as Just as MSW?
, 1995 The neutrino long wavelength (just-so) oscillation is reconsidered as a solution to the solar neutrino problem. In the light of the presently updated results of the four solar neutrino experiments, the data fit in the just-so scenario substantially ...
Acker +47 more
core +1 more source
Human‐AI Co‐Creativity: Does ChatGPT Make Us More Creative?
The Journal of Creative Behavior, Volume 59, Issue 2, June 2025.ABSTRACT Much has been made of the apparent capacity for creativity of generative AI. However, as research expands the knowledge base regarding the capabilities and performance of this technology, the prevailing view is shifting away from “AI is creative” and towards a more balanced model of Human‐AI co‐creativity.
Kelsey Medeiros +3 more
wiley +1 more source
Fingerprint of GeV scale right-handed neutrinos on inflationary gravitational waves and PTA data [PDF]
, 2023 Satyabrata Datta, Rome Samanta
openalex +1 more source
Theoretical Prospects of Neutrinoless Double Beta Decay
, 2005 The compelling experimental evidences for oscillations of solar and atmospheric neutrinos imply the existence of 3-neutrino mixing in vacuum. We briefly review the phenomenology of 3-neutrino mixing, and the current data on the 3-neutrino mixing ...
Aalseth C +43 more
core +1 more source
Neutrinoloser Doppelbetazerfall: Der Gral der Neutrinophysik
Physik in unserer Zeit, Volume 56, Issue 3, Page 132-137, May 2025.Die Entschlüsselung der Neutrinoeigenschaften ist auch siebzig Jahre nach ihrer Entdeckung noch nicht abgeschlossen. Es wäre eine spektakuläre Entdeckung, sollten Neutrinos ihre eigenen Antiteilchen sein und sich folglich als Majorana‐Teilchen entpuppen. Mehrere Experimente untersuchen diese Möglichkeit.
Bernhard Schwingenheuer
wiley +1 more source
The Cosmological Energy Density of Neutrinos from Oscillation Measurements
, 2003 The emerging structure of the neutrino mass matrix, when combined with the primordial element abundances, places the most stringent constraint on the flavor asymmetries in the cosmological neutrino background and therefore its energy density.
Abazajian, Kevork
core +2 more sources
Effect of Matter Motion and Polarization in Neutrino Flavour Oscillations
, 2002 The Lorentz invariant formalism for description of neutrino flavor oscillation in moving and polarized matter is developed. It is shown that the neutrino effective potential, which determines the effective mass difference between neutrinos in matter can ...
A. Grigoriev +17 more
core +1 more source
Neutrino Properties Before and After KamLAND [PDF]
, 2003 We review neutrino oscillation physics, including the determination of mass splittings and mixings from current solar, atmospheric, reactor and accelerator neutrino data. A brief discussion is given of cosmological and astrophysical implications.
Pakvasa, S., Valle, J. W. F.
core +4 more sources
Diffuse neutrino flux measurements with the Baikal-GVD neutrino telescope [PDF]
, 2023 E. Eckerová
openalex +1 more source