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相关论文: A topological approach to Neutrino masses by using…

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Usually, the topology of a 4-manifolds $M$ is restricted to admit a global hyperbolic structure $\Sigma\times\mathbb{R}$. The result was obtained by using two conditions: existence of a Lorentz structure and causality (no time-like closed…

广义相对论与量子宇宙学 · 物理学 2011-11-04 T. Asselmeyer-Maluga , R. Mader , J. Krol

We present a composite scotogenic model for neutrino masses, which are generated via loops of $\mathbb{Z}_2$-odd composite scalars. We consider three different approaches to the couplings of the neutrinos (including three right-handed…

高能物理 - 唯象学 · 物理学 2021-10-22 Giacomo Cacciapaglia , Martin Rosenlyst

We discuss non-perturbative corrections to the neutrino sector, in the context of a D-brane Pati-Salam-like model, that can be obtained as a simple alternative to $SO(10)$ GUT's in theories with open and unoriented strings. In such D-brane…

高能物理 - 唯象学 · 物理学 2016-02-09 Andrea Addazi , Massimo Bianchi , Giulia Ricciardi

We present a three-loop model of neutrino mass in which both the weak scale and neutrino mass arise as radiative effects. In this approach, the scales for electroweak symmetry breaking, dark matter, and the exotics responsible for neutrino…

高能物理 - 唯象学 · 物理学 2016-02-11 Amine Ahriche , Kristian L. McDonald , Salah Nasri

In the context of the supersymmetric flipped $SU(5)\otimes U(1)$ GUT model, we have studied in detail the neutrino mass spectrum, obtaining an approximate formula for the corresponding effective three-generation mass matrix. It is found…

高能物理 - 唯象学 · 物理学 2009-10-22 Stefano Ranfone

We present, theoretical predictions and Monte Carlo simulations, for a simple three matrix model that exhibits an exotic phase transition. The nature of the transition is very different if approached from the high or low temperature side.…

高能物理 - 理论 · 物理学 2010-01-15 Rodrigo Delgadillo-Blando , Denjoe O'Connor , Badis Ydri

The time evolution of a cosmological scalar field can be stopped by an increasing mass of the neutrinos. This leads to a transition from a cosmological scaling solution with dynamical dark energy at early time to a cosmological constant…

高能物理 - 唯象学 · 物理学 2008-11-26 C. Wetterich

Neutrino data lead via the see-saw mechanism to masses of the right handed neutrinos at the intermediate mass scale. Simple formalism is suggested which incorporates the quark - lepton symmetry and allows one to find properties of the…

高能物理 - 唯象学 · 物理学 2009-10-28 A. Yu. Smirnov

We study a six matrix model with global $SO(3)\times SO(3)$ symmetry containing at most quartic powers of the matrices. This theory exhibits a phase transition from a geometrical phase at low temperature to a Yang-Mills matrix phase with no…

高能物理 - 理论 · 物理学 2016-10-26 Badis Ydri , Ramda Khaled , Rouag Ahlam

Since the first work on exotic smoothness in physics, it was folklore to assume a direct influence of exotic smoothness to quantum gravity. Thus, the negative result of Duston (arXiv:0911.4068) was a surprise. A closer look into the…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Torsten Asselmeyer-Maluga

Since the first work on exotic smoothness in physics, it was folklore to assume a direct influence of exotic smoothness to quantum gravity. In the second paper, we calculate the "smoothness structure" part of the path integral in quantum…

广义相对论与量子宇宙学 · 物理学 2012-01-19 T. Asselmeyer-Maluga , J. Krol

I review promising approaches to neutrino mass models, focussing on three neutrino patterns of neutrino masses and mixing angles, and the corresponding Majorana mass matrices. I discuss the see-saw mechanism, and show how it may be applied…

高能物理 - 唯象学 · 物理学 2015-06-25 S. F. King

We analyse the phenomenology of a model of neutrino masses inspired by $\mathrm{E}_{6}$ GUT unification in which the exotic neutrinos can be present at low scales. The model introduces vector-like isosinglet down-type quarks, vector-like…

高能物理 - 唯象学 · 物理学 2017-11-22 Joshua P. Ellis , Raymond R. Volkas

Generating small sterile neutrino masses via the same seesaw mechanism that suppresses active neutrino masses requires a specific structure in the neutral fermion mass matrix. We present a model where this structure is enforced by a new…

高能物理 - 唯象学 · 物理学 2013-06-03 Julian Heeck , He Zhang

A mass-energy scale for neutrinos was calculated from the null cone curvature using geometric concepts. The scale is variable depending on the gravitational potential and the trajectory inclination with respect to the field direction. The…

综合物理 · 物理学 2014-05-22 Gustavo R. Gonzalez-Martin

We study a three matrix model with global SO(3) symmetry containing at most quartic powers of the matrices. We find an exotic line of discontinuous transitions with a jump in the entropy, characteristic of a 1st order transition, yet with…

高能物理 - 理论 · 物理学 2008-11-26 Rodrigo Delgadillo-Blando , Denjoe O'Connor , Badis Ydri

Using the concept of real tunneling configurations (classical signature change) and nucleation energy, we explore the consequences of an alternative minimization procedure for the Euclidean action in multiple-dimensional quantum cosmology.…

广义相对论与量子宇宙学 · 物理学 2009-10-28 Franz Embacher

We studied a left-right symmetric model that can accommodate the neutrino dark energy (\nd) proposal. Type III seesaw mechanism is implemented to give masses to the neutrinos. After explaining the model, we study the consistency of the…

高能物理 - 唯象学 · 物理学 2010-04-21 Jitesh R. Bhatt , Pei-Hong Gu , Utpal Sarkar , Santosh K. Singh

We study the formation and evolution of topological defects that arise in the post-recombination phase transition predicted by the gravitational neutrino mass model in [Dvali, Funcke, Phys. Rev. D 93, 113002 (2016)]. In the transition,…

高能物理 - 唯象学 · 物理学 2023-08-10 Gia Dvali , Lena Funcke , Tanmay Vachaspati

In this paper we consider the possibility of neutrino mass varying during the evolution of the Universe and study its implications on leptogenesis. Specifically, we take the minimal seesaw model of neutrino masses and introduce a coupling…

高能物理 - 唯象学 · 物理学 2009-11-10 Xiao-Jun Bi , Peihong Gu , Xiulian Wang , Xinmin Zhang
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