Fundamentals of Neutrino Physics and Astrophysics
By C. Giunti, C. W. Kim. 2007
1,021 citations recorded by the source corpus.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/f4c407ae5af648e738be0bbf91c824dcfcb1bf33
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Citations in the corpus
- 2020 global reassessment of the neutrino oscillation picture (2020, background): “[91], isolating the individual neutrino masses from such observations is beyond the reach of present experiments.”
- Neutrino decoupling including flavour oscillations and primordial nucleosynthesis (2020, methodology): “with U the Pontercorvo-Maki-Nakagawa-Sakata (PMNS) mixing matrix [8].”
- From eV to EeV: Neutrino Cross Sections Across Energy Scales (2012, background): “We highlight (Giunti and Kim, 2007) as an excellent in-depth resource for the reader.”
- eV-Scale Sterile Neutrinos (2019, background): “The electron and muon neutrino and antineutrino appearance and disappearance in short-baseline experiments depend on |Ue4|(2) and |Uμ4|(2), which determine the amplitude sin(2) 2θeμ = 4|Ue4|(2)|Uμ4|(2) = sin(2) 2θ14 sin(2) θ24 (14)”
- Neutrino electromagnetic interactions: A window to new physics (2014, methodology): “The diagonal unitary matrix DM can be written as DM = diag ( 1 , eiλ21 , eiλ31 ) , (2.29) in terms of the two Majorana phases λ21 and λ31, All the phases in the mixing matrix violate the CP symmetry (see Giunti and Kim (2007); Branco et al. (2012)).”
- Neutrinoless double-beta decay. A brief review (2012, background): “rangeness. In terms of the quark fields, the current jα(x) has the form jα(x) = 2cosϑC¯uL(x)γαdL(x). (32) The mixed flavor field νeL(x) is given by the relation (28) with l = e: νeL(x) = X i Uei νiL(x), (33) where U is the PMNS mixing matrix and νi(x) is the field of the Majorana neutrino with mass mi, ”
- Challenges in Double Beta Decay (2013, background): “Massive neutrino phenomenology (see for example [8, 9, 10, 11]) is described in the framework of three distinguishable particles provided with their own leptonic number, flavor and mass eigenvalue.”
- IceCube sensitivity for low-energy neutrinos from nearby supernovae (2011, background): “A compilation in Giunti & Kim (2007) narrows the expected range to (1.7 − 2.5)/100 years by taking into account experimental and theoretical limits.”
- Neutrinoless Double-Beta Decay: a Probe of Physics Beyond the Standard Model (2014, background): “[46]), the Majorana nature of neutrinos is a sufficient and necessary condition for the existence of ββ0ν decay.”
- Neutrinoless Double Beta Decay and Heavy Sterile Neutrinos (2011, background): “On the theoretical side, accepting that neutrinos have masses, see [16, 17, 18, 19, 20, 21, 22, 23, 24] and [25, 26, 27, 28, 29, 30, 31, 32, 33, 34, 35, 36, 37, 38, 39, 40, 41, 42, 43], the investigation of 0ν2β becomes the most natural option; moreover, the observation of lepton-number violating pr”
- Reactor On-Off Antineutrino Measurement with KamLAND (2013, neutral): “(6) we have neglected matter effects, which modify the survival probability by 1% [14].”
- Neutrino oscillations (2013, neutral): “, [7, 9]) and the parameterF depends on the adopted electron density profile.”
- Current unknowns in the three-neutrino framework (2018, background): “Recent books with useful references on various aspects of our current understanding (and future prospects) of the neutrino mass-mixing phenomenology and its relation with astroparticle physics and cosmology include [67, 68, 69, 70, 71, 72, 73, 74, 75, 76, 77].”