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We consider the effect of non-standard neutrino interactions (NSI, for short) on the propagation of neutrinos through the supernova (SN) envelope within a three-neutrino framework and taking into account the presence of a neutrino…

高能物理 - 唯象学 · 物理学 2010-04-06 A. Esteban-Pretel , R. Tomas , J. W. F. Valle

Nonstandard interactions (NSI) of neutrinos with matter can significantly alter neutrino flavor evolution in supernovae with the potential to impact explosion dynamics, nucleosynthesis, and the neutrinos signal. In this paper, we explore,…

高能物理 - 唯象学 · 物理学 2016-12-07 Charles J. Stapleford , Daavid J. Väänänen , James P. Kneller , Gail C. McLaughlin , Brandon T. Shapiro

We analyze the prospects for studying scalar non-standard interactions (SNSI) using the neutrino burst from a Galactic supernova. SNSI modify the resonant flavor conversion and, correspondingly, the neutronization burst signal, and may be…

高能物理 - 唯象学 · 物理学 2025-08-25 Bhaskar Dutta , Aparajitha Karthikeyan , Nityasa Mishra , Yago Porto , Louis E. Strigari

Non-standard neutrino self interactions (NSSI) could be stronger than Fermi interactions. We investigate the ability to constrain these four-neutrino interactions by their effect on the flux of neutrinos originating from a galactic…

高能物理 - 唯象学 · 物理学 2020-02-19 Minjie Lei , Noah Steinberg , James D. Wells

Neutrino non-standard interactions (NSI), previously introduced for the sun, are studied in the supernova context. For normal hierarchy the probability for electron neutrinos and antineutrinos at low energy ($E\lesssim 0.8-0.9 MeV$) is…

高能物理 - 唯象学 · 物理学 2013-04-10 C. R. Das , Joao Pulido

The present thesis aims to be an analysis of various aspects of neutrino phenomenology in two different scenarios. On the one hand, we address the study of non-standard neutrino interactions (NSI) in accelerator and reactor terrestrial…

高能物理 - 唯象学 · 物理学 2009-12-11 Andreu Esteban-Pretel

Neutrino nonstandard interactions (NSI) were investigated earlier in the solar case and were shown to reduce the tensions between the data and the large mixing angle solution predictions. We extend the previous framework to the supernova…

高能物理 - 唯象学 · 物理学 2013-05-29 C. R. Das , Joao Pulido

We show that non-standard neutrino interactions (NSI) can notably modify the pattern of resonant flavor conversion of neutrinos within supernovae and significantly impact the neutronization burst signal in forthcoming experiments such as…

高能物理 - 唯象学 · 物理学 2025-03-25 Sudip Jana , Yago Porto

We introduce the first oscillation-independent astrophysical method to probe non-standard neutrino interactions (NSI) in core-collapse supernovae. Using a self-consistent treatment of NSI effects in both supernova neutrino emission…

高能物理 - 唯象学 · 物理学 2025-09-10 Angela R. Beatty , Anna M. Suliga , Volodymyr Takhistov

Non-standard neutrino interactions with a massive boson can produce the bosons in the core of core-collapse supernovae (SNe). After the emission of the bosons from the SN core, their subsequent decays into neutrinos can modify the SN…

高能物理 - 唯象学 · 物理学 2022-12-28 Kensuke Akita , Sang Hui Im , Mehedi Masud

Non-standard neutrino interactions (NSI) affect both their propagation through matter and their detection, with bounds on NSI parameters coming from various astrophysical and terrestrial neutrino experiments. In this paper, we show that NSI…

高能物理 - 唯象学 · 物理学 2017-08-31 Bhaskar Dutta , Shu Liao , Louis E. Strigari , Joel W. Walker

Observing a high-statistics neutrino signal from a galactic supernova (SN) would allow one to test the standard delayed explosion scenario and may allow one to distinguish between the normal and inverted neutrino mass ordering due to the…

高能物理 - 唯象学 · 物理学 2009-11-11 Georg G. Raffelt

Future dark matter (DM) direct detection searches will be subject to irreducible neutrino backgrounds that will challenge the identification of an actual WIMP signal in experiments without directionality sensitivity. We study the impact of…

高能物理 - 唯象学 · 物理学 2017-12-29 D. Aristizabal Sierra , N. Rojas , M. H. G. Tytgat

Neutrino self-interactions are known to lead to non-linear collective flavor oscillations in a core-collapse supernova. We point out new possible effects of non-standard self-interactions (NSSI) of neutrinos on flavor conversions in a…

高能物理 - 唯象学 · 物理学 2017-06-05 Anirban Das , Amol Dighe , Manibrata Sen

We present a new analysis of non-universal and flavor changing non-standard neutrino interactions (NSI) in \nu_e e or \bar{\nu}_e e scattering. Our global analysis of these process includes all relevant experiments, such as the most recent…

高能物理 - 唯象学 · 物理学 2009-09-17 J. Barranco , O. G. Miranda , C. A. Moura , J. W. F. Valle

Future galactic supernovae will provide an extremely long baseline for studying the properties and interactions of neutrinos. In this paper, we discuss the possibility of using such an event to constrain (or discover) the effects of exotic…

高能天体物理现象 · 物理学 2010-10-01 Chris Kelso , Dan Hooper

We discuss the sensitivity reach of a neutrino factory measurement to non-standard neutrino interactions (NSI), which may exist as a low-energy manifestation of physics beyond the Standard Model. We use the muon appearance mode \nu_e -->…

高能物理 - 唯象学 · 物理学 2009-01-06 N. Cipriano Ribeiro , H. Minakata , H. Nunokawa , S. Uchinami , R. Zukanovich Funchal

Neutrino non-standard interactions (NSI) play a crucial role in neutrino oscillations and can provide valuable insights for constructing models of neutrino masses and mixing. While NSI have been widely explored through oscillation and…

高能物理 - 唯象学 · 物理学 2025-07-16 Sudip Jana , Saumyen Kundu , Santosh Kumar Rai

Non-standard interactions (NSI) between neutrinos and electrons can significantly modify the decoupling of neutrinos from the plasma. These interactions have two effects on the overall picture: (i) they alter neutrino oscillations though…

高能物理 - 唯象学 · 物理学 2022-03-02 Pablo Martínez-Miravé

We investigate non-standard neutrino interactions (NSIs) in the triplet seesaw model featuring non-trivial correlations between NSI parameters and neutrino masses and mixing parameters. We show that sizable NSIs can be generated as a…

高能物理 - 唯象学 · 物理学 2009-02-18 Michal Malinsky , Tommy Ohlsson , He Zhang
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