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Related papers: Neutrino Oscillations in Deconstructed Dimensions

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Low-scale models of neutrino mass generation often feature sterile neutrinos with masses in the GeV-TeV range, which can be produced at colliders through their mixing with the Standard Model neutrinos. We consider an alternative scenario in…

High Energy Physics - Phenomenology · Physics 2021-02-24 Stéphane Lavignac , Anibal D. Medina

In this paper, we study the effect of the minimal length on neutrino oscillation in a static magnetic field. In the framework of the generalized uncertainty principle, we reformulate the Hamiltonian for a relativistic neutrino moving in a…

High Energy Physics - Phenomenology · Physics 2023-05-31 Fidele J. Twagirayezu

We investigate the formation of dynamical gaugino condensates and supersymmetry breaking in the compactifications of Horava-Witten theory with perturbative nonstandard embeddings. Specific models are considered where the underlying massless…

High Energy Physics - Theory · Physics 2009-10-31 Zygmunt Lalak , Steven Thomas

We propose a new framework for solving the hierarchy problem which does not rely on either supersymmetry or technicolor. In this framework, the gravitational and gauge interactions become united at the weak scale, which we take as the only…

High Energy Physics - Phenomenology · Physics 2008-11-26 Nima Arkani-Hamed , Savas Dimopoulos , Gia Dvali

The clustering properties of sterile neutrinos are studied within an extension of the minimal standard model, where these are produced via the decay of a gauge singlet scalar. The distribution function after decoupling is strongly out of…

Astrophysics · Physics 2008-12-18 D. Boyanovsky

We study neutrino spin oscillations in background matter under the influence of strong electromagnetic and gravitational fields. The neutrino spin evolution is treated quasiclassically. We derive the effective Hamiltonian governing spin…

High Energy Physics - Phenomenology · Physics 2018-01-09 Maxim Dvornikov

This article summarises a talk given at the 2014 Palermo workshop on Astrophysics. It covers a short review on the neutrino physics status and the potential physics opportunities of future experiments. During the last year our knowledge on…

High Energy Physics - Experiment · Physics 2015-03-20 Thomas Strauss

We propose a ultraviolet complete theory for cold dark matter(CDM) and sterile neutrino that can accommodate both cosmological data and neutrino oscillation experiments at $1\sigma$ level. A new $U(1)_X$ dark gauge symmetry is introduced,…

High Energy Physics - Phenomenology · Physics 2014-10-29 P. Ko , Yong Tang

We propose a new pattern of the neutrino mixing matrix which can be parametrized as the product of an arbitrary Hermitian matrix and the well-known tri-bimaximal mixing matrix. In this scenario, nontrivial values of the smallest neutrino…

High Energy Physics - Phenomenology · Physics 2008-11-26 Shu Luo

We consider a class of models in which the neutrinos acquire Majorana masses through mixing with singlet neutrinos that emerge as composite states of a strongly coupled hidden sector. In this framework, the light neutrinos are partially…

High Energy Physics - Phenomenology · Physics 2021-03-16 Zackaria Chacko , Patrick J. Fox , Roni Harnik , Zhen Liu

We study nonlinear gravitational perturbations of vacuum Einstein equations, with $\Lambda<0$ in $(n+2)$ dimensions, with $n>2$, generalizing previous studies for $n=2$. We follow the formalism by Ishibashi, Kodama and Seto to decompose the…

General Relativity and Quantum Cosmology · Physics 2020-11-18 Dhanya S. Menon , Vardarajan Suneeta

We consider the effect of three species of neutrinos with nearly degenerate mass on the cosmic structure formation in a low matter-density universe within a hierarchical clustering scenario with a flat initial perturbation spectrum. The…

High Energy Physics - Phenomenology · Physics 2008-11-26 Masataka Fukugita , Guo-Chin Liu , Naoshi Sugiyama

We propose structures of size between $\sim 1$ meter to 100 meters that drastically alter the local distribution of the Cosmic Neutrino Background ($C\nu B$). These structures have a shape reminiscent of a sea urchin: They consist of rods…

High Energy Physics - Phenomenology · Physics 2024-01-01 Asimina Arvanitaki , Savas Dimopoulos

Our understanding of neutrino flavor conversion in the innermost regions of core-collapse supernovae and neutron star mergers is mostly limited to spherically symmetric configurations that facilitate the numerical solution of the quantum…

High Energy Astrophysical Phenomena · Physics 2024-11-28 Marie Cornelius , Shashank Shalgar , Irene Tamborra

A quintessence scalar field or cosmon interacting with neutrinos can have important effects on cosmological structure formation. Within growing neutrino models the coupling becomes effective only in recent times, when neutrinos become…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-29 Nico Wintergerst , Valeria Pettorino , David F. Mota , Christof Wetterich

Neutrino physics in the early Universe is key to our understanding of later cosmological stages, such as primordial nucleosynthesis (BBN) or the formation of large-scale structures. The coming decade promises new experimental results to…

Cosmology and Nongalactic Astrophysics · Physics 2022-09-15 Julien Froustey

An upper limit to distillable entanglement between two disconnected regions of massless non-interacting scalar field theory has an exponential decay defined by a geometric decay constant. When regulated at short distances with a spatial…

Quantum Physics · Physics 2021-03-31 Natalie Klco , Martin J. Savage

In a previous paper, we gave a new theoretical framework in which three neutrino mixing in matter are discussed. Rigorous analytical solutions are obtained. In present paper an approximate method is developed for studying three flavor…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Cheng

The case for small neutrino mass differences from atmospheric and solar neutrino oscillation experiments has become compelling, but leaves the overall neutrino mass scale m_nu undetermined. The most restrictive limit of m_nu < 0.8 eV arises…

Astrophysics · Physics 2009-11-07 G. G. Raffelt

Searches for modified gravity in the large-scale structure try to detect the enhanced amplitude of density fluctuations caused by the fifth force present in many of these theories. Neutrinos, on the other hand, suppress structure growth…

Cosmology and Nongalactic Astrophysics · Physics 2019-09-04 Steffen Hagstotz , Max Gronke , David Mota , Marco Baldi