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相关论文: Resonance refraction and neutrino oscillations

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We consider in detail a possibility that the observed neutrino oscillations are due to refraction on ultralight scalar boson dark matter. We introduce the refractive mass squared, $\tilde{m}^2$, and study its properties: dependence on…

高能物理 - 唯象学 · 物理学 2023-11-13 Manibrata Sen , Alexei Y. Smirnov

We have determined the dispersion relation of a neutrino test particle propagating in the cosmic neutrino background. Describing the relic neutrinos and antineutrinos from the hot big bang as a dense medium, a matter potential or refractive…

高能物理 - 唯象学 · 物理学 2016-03-09 J. S. Diaz , F. R. Klinkhamer

We investigate resonant active-sterile neutrino oscillations emergent from the interplay between matter, CPT- and Lorentz-violating coefficients with different energy dependences. Novel and experimentally accessible resonant neutrino…

高能物理 - 唯象学 · 物理学 2010-06-17 Sebastian Hollenberg , Heinrich Päs

We present the results of a new analysis of the data of the MiniBooNE experiment taking into account the additional background of photons from $\Delta^{+/0}$ decay proposed in arXiv:1909.08571 and additional contributions due to coherent…

高能物理 - 唯象学 · 物理学 2020-12-30 C. Giunti , A. Ioannisian , G. Ranucci

The impact of neutrino mixing, refraction and absorption on high-energy neutrino propagation through a thick medium is studied using the MSW evolution equation with complex indices of refraction. It is found that, owing to the mixing with…

高能物理 - 唯象学 · 物理学 2009-11-07 Vadim A. Naumov

We consider a class of theories in which neutrino masses depend significantly on environment, as a result of interactions with the dark sector. Such theories of mass varying neutrinos (MaVaNs) were recently introduced to explain the origin…

高能物理 - 唯象学 · 物理学 2009-11-10 David B. Kaplan , Ann E. Nelson , Neal Weiner

Neutrino self-interactions beyond the standard model have profound implications in astrophysics and cosmology. In this Letter, we study an uncharted scenario in which one of the three neutrino species has a mass smaller than the temperature…

高能物理 - 唯象学 · 物理学 2025-10-30 Isaac R. Wang , Xun-Jie Xu , Bei Zhou

Heavy neutrinos with additional interactions have recently been proposed as an explanation to the MiniBooNE excess. These scenarios often rely on marginally boosted particles to explain the excess angular spectrum, thus predicting large…

高能物理 - 唯象学 · 物理学 2020-01-17 Carlos A. Argüelles , Matheus Hostert , Yu-Dai Tsai

We present a theory of neutrino oscillations in a dense medium which goes beyond the effective matter potential used in the description of the MSW effect. We show how the purity of the neutrino state is degraded by neutrino interactions…

高能物理 - 唯象学 · 物理学 2021-07-20 Antonio Capolupo , Salvatore Marco Giampaolo , Aniello Quaranta

The MiniBooNE excess persists as a significant puzzle in particle physics. Given that the MiniBooNE detector cannot discriminate between electron-like signals and backgrounds due to photons, the goal of this work is to study photon…

高能物理 - 唯象学 · 物理学 2023-05-31 Kevin J. Kelly , Joachim Kopp

The bounds on neutrino masses and mixing that follows from the data on light element abundances, large scale structure formation, and angular fluctuations of cosmic microwave background radiation are analyzed. The role of neutrino…

高能物理 - 唯象学 · 物理学 2017-08-23 A. D. Dolgov

The neutrino flux close to a supernova core contributes substantially to neutrino refraction so that flavor oscillations become a nonlinear phenomenon. One unexpected consequence is efficient flavor transformation for anti-neutrinos in a…

天体物理学 · 物理学 2009-11-07 Sergio Pastor , Georg Raffelt

We investigate the resonant interaction of neutrinos in matter in the presence of mixing. At energies near the W resonance, oscillations are absent; the survival probability of electron antineutrinos is suppressed due to the presence of…

高能物理 - 唯象学 · 物理学 2009-10-28 G. Domokos , S. Kovesi-Domokos

We consider the neutrino self-energy in a background composed of a scalar particle and a fermion using a simple model for the coupling of the form $\lambda\bar f_R\nu_L\phi$. The results are useful in the context of Dark Matter-neutrino…

高能物理 - 唯象学 · 物理学 2022-01-17 José F. Nieves , Sarira Sahu

We study the RH neutrino properties from the low energy neutrino data in the seesaw mechanism. Reonance behavior is found for the right-handed (RH) mixing angle as a function of light neutrino mass ratios in two favored region of the solar…

高能物理 - 唯象学 · 物理学 2007-05-23 Haijun Pan , G. Cheng

If there is a hidden photon -- i.e. a light abelian gauge boson in the hidden sector -- its kinetic mixing with the standard photon can produce a hidden cosmic microwave background (hCMB). For meV masses, resonant photon-hidden photon…

天体物理学 · 物理学 2009-06-23 Joerg Jaeckel , Javier Redondo , Andreas Ringwald

The mechanism of resonance enhancement of neutrino oscillations in matter and some critical remarks to this mechanism are considered. Using of this resonance mechanism is very important to examine the model of electroweak interactions since…

高能物理 - 唯象学 · 物理学 2009-01-01 Kh. M. Beshtoev

Consequences of a new force mediated by a light scalar particle for neutrino oscillation experiments are considered. Such a force could give rise to neutrino masses and mixings whose matter dependence is much more significant than the MSW…

高能物理 - 唯象学 · 物理学 2008-11-26 Kathryn M. Zurek

Parametric enhancement of the appearance probability of the neutrino oscillation under the inhomogeneous matter is studied. Fourier expansion of the matter density profile leads to a simple resonance condition and manifests that each…

高能物理 - 唯象学 · 物理学 2009-10-16 Masafumi Koike , Toshihiko Ota , Masako Saito , Joe Sato

The MiniBooNE low-energy excess stands as an unexplained anomaly in short-baseline neutrino oscillation experiments. It has been shown that it can be explained in the context of dark sector models. Here, we provide an overview of the…

高能物理 - 唯象学 · 物理学 2025-01-31 Asli M. Abdullahi , Jaime Hoefken Zink , Matheus Hostert , Daniele Massaro , Silvia Pascoli
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