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相关论文: Supernovae as laboratories for neutrino properties

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We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through the detection of neutrinos produced in a future galactic supernova (SN).We consider the effect of NSI on the neutrino propagation through the…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Esteban-Pretel , R. Tomàs , J. W. F. Valle

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

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 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

Neutrinos emitted from a supernova encode useful information about neutrino physics and astrophysics. Interpreting the neutrino signal depends crucially on understanding neutrino production, flavor mixing during propagation, and detection.…

高能物理 - 唯象学 · 物理学 2011-04-22 Basudeb Dasgupta

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

I review the physics of the Diffuse Supernova Neutrino flux (or Background, DSNB), in the context of future searches at the next generation of neutrino observatories. The theory of the DSNB is discussed in its fundamental elements, namely…

宇宙学与河外天体物理 · 物理学 2016-05-24 Cecilia Lunardini

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

I shall review some of the recent results concerning the astrophysics of a core collapse supernova (SN) and neutrino oscillations. Neutrinos play an important role in the SN explosion, and they also carry most of the energy of the collapse.…

高能物理 - 唯象学 · 物理学 2009-11-10 Amol Dighe

Neutrinos, being elusive subatomic particles having only weak interactions, provide an ideal platform to look for physics beyond the Standard Model. In the present era of neutrino physics, various experiments are focusing towards the…

高能物理 - 唯象学 · 物理学 2025-03-18 Rukmani Mohanta

In dense environments, standard and non-standard neutrino interactions with the background particles trigger a variety of flavor mechanisms, which can impact r-process nucleosynthetic abundances. Future observations of a(n) (extra)galactic…

高能物理 - 唯象学 · 物理学 2021-11-17 Maria Cristina Volpe

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

We investigate the potential to probe new neutrino physics with future experiments measuring coherent neutrino-nucleus scattering. Experiments with high statistics should become feasible soon and allow to constrain parameters with…

高能物理 - 唯象学 · 物理学 2017-04-05 Manfred Lindner , Werner Rodejohann , Xun-Jie Xu

Neutrinos are amongst the most abundant particles in the universe. The fact that they are massive particles proves that the Standard Model is an incomplete theory and needs to be extended. This thesis focuses on the study of neutrino…

高能物理 - 唯象学 · 物理学 2023-09-28 Pablo Martínez-Miravé

This talk summarizes our recent work which studied the impact of resonant neutrino conversion induced by some non-standard neutrino properties beyond mass and mixing, such as neutrino magnetic moment, lepton-flavor non-universality as well…

高能物理 - 唯象学 · 物理学 2007-05-23 Hiroshi Nunokawa

Neutrino experiments study the least understood of the Standard Model particles by observing their direct interactions with matter or searching for ultra-rare signals. The study of neutrinos typically requires overcoming large backgrounds,…

计算物理 · 物理学 2020-12-30 Fernanda Psihas , Micah Groh , Christopher Tunnell , Karl Warburton

In most of the proposals for new physics beyond the standard model, neutrinos have new interactions and some of them have phenomenological consequences that, although at present they may seem purely academic, probably will have to be taken…

高能物理 - 唯象学 · 物理学 2022-07-05 Vicente Pleitez

Even the elusive neutrinos are trapped in matter, albeit transiently, in several astrophysical circumstances. Their interactions with the ambient matter not only reveal the properties of such exotic matter itself, but also shed light on the…

天体物理学 · 物理学 2009-11-06 M. Prakash , J. M. Lattimer , R. F. Sawyer , R. R. Volkas

We highlight the progress in our understanding of how neutrinos change their flavor in astrophysical environments, in particular effects from the neutrino self-interaction. We emphasize extended descriptions of neutrino propagation in…

高能天体物理现象 · 物理学 2016-06-22 Cristina Volpe

Presently, there are several experimental setups dedicated to rare event searches, such as dark matter interactions or double beta decay, in the building or commissioning phases. These experiments often use large mass detectors and have…

高能天体物理现象 · 物理学 2012-11-08 Carlos Martinez Amaya , Matteo Biassoni
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