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相关论文: How can we test seesaw experimentally?

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The recently proposed "mini-seesaw mechanism" combines naturally suppressed Dirac and Majorana masses to achieve light Standard Model neutrinos via a low-scale seesaw. A key feature of this approach is the presence of multiple light (order…

高能物理 - 唯象学 · 物理学 2011-11-15 Michael Duerr , Damien P. George , Kristian L. McDonald

A summary of neutrino oscillation results is given along with a discussion of neutrino mass generation mechanisms, including high and low-scale seesaw, with and without supersymmetry, as well as recent attempts to understand flavor. I argue…

高能物理 - 唯象学 · 物理学 2010-01-30 J. W. F. Valle

Heavy neutrinos with masses below the electroweak scale can simultaneously generate the light neutrino masses via the seesaw mechanism and the baryon asymmetry of the universe via leptogenesis. The requirement to explain these phenomena…

高能物理 - 唯象学 · 物理学 2017-09-13 Marco Drewes , Bjorn Garbrecht , Dario Gueter , Juraj Klaric

With a mass at least six orders of magnitudes smaller than the mass of an electron -- but non-zero -- neutrinos are a clear misfit in the Standard Model of Particle Physics. On the one hand, its tiny mass makes the neutrino one of the most…

核实验 · 物理学 2016-06-22 Susanne Mertens

If there is no new physics beyond the TeV energy scale, such as in a theory of large extra dimensions, the smallness of the seesaw neutrino mass, i.e. $m_\nu = m_D^2/m_N$, cannot be explained by a very large $m_N$. In contrast to previous…

高能物理 - 唯象学 · 物理学 2009-10-31 Ernest Ma

On fitting the type II seesaw mechanism into the type I seesaw mechanism, we obtain a formula to the neutrino masses which get suppressed by high-scale $M^3$ in its denominator. As a result, light neutrinos are naturally obtained with new…

高能物理 - 唯象学 · 物理学 2010-04-30 D. Cogollo , H. Diniz , C. A. de S. Pires

Recent (first or/and the best) results from the neutrino experiments are reviewed and their implications for the theory are discussed. The sense of the experiments is the searching for neutrino masses, mixing and interactions beyond the…

高能物理 - 唯象学 · 物理学 2009-09-25 Alexei Yu. Smirnov

If the canonical seesaw mechanism alone is responsible for neutrino mass, i.e. m_nu = -m_D^2/m_N, it can neither be proved nor disproved at the TeV energy scale. A new verifiable mechanism of neutrino mass is proposed, using the "inverse"…

高能物理 - 唯象学 · 物理学 2009-09-02 Ernest Ma

We discuss neutrino mass and mixing in the framework of the classic seesaw mechanism, involving right-handed neutrinos with large Majorana masses, which provides an appealing way to understand the smallness of neutrino masses. However, with…

高能物理 - 唯象学 · 物理学 2016-06-22 Stephen F. King

The simplest possibility to generate small Majorana neutrino masses is the seesaw mechanism. However, the smallness of the observed neutrino masses can also be understood, if neutrino masses are generated by higher-dimensional operators…

高能物理 - 唯象学 · 物理学 2020-05-20 Ricardo Cepedello , Renato Fonseca , Martin Hirsch

Superheavy neutrinos can, via the seesaw model, provide a mechanism for lepton number violation. If they are combined with flavor violation as characterized by the Froggatt-Nielsen mechanism, then the phenomenology for the neutrinos in…

高能物理 - 唯象学 · 物理学 2019-07-24 Micheal S. Berger , Maria Dawid

In a recent Letter we presented a systematic way of testing the seesaw origin of neutrino mass in the context of the Minimal Left-Right Symmetric Model. The essence of the program is to exploit lepton number violating decays of doubly…

高能物理 - 唯象学 · 物理学 2019-12-25 Goran Senjanovic , Vladimir Tello

We discuss the prospects for detecting right-handed neutrinos which are introduced in the see-saw mechanism at future colliders. This requires a very accurate cancellation between contributions from different right-handed neutrinos to the…

高能物理 - 唯象学 · 物理学 2011-11-10 Joern Kersten

Knowledge of the mechanism of neutrino mass generation would help understand a lot more about Lepton Number Violation (LNV), the cosmological evolution of the Universe, or the evolu tion of astronomical objects. Here we propose a verifiable…

高能物理 - 唯象学 · 物理学 2020-03-18 Claudio Dib , Sergey Kovalenko , Ivan Schmidt , Adam Smetana

A minimal extension of the Standard Model is proposed, where the observed left-handed neutrinos obtain naturally small Majorana masses from a one-loop radiative seesaw mechanism. This model has two candidates (one bosonic and one fermionic)…

高能物理 - 唯象学 · 物理学 2010-04-06 Ernest Ma

Within type-I seesaw mechanism it is possible to have large (order one) light-heavy neutrino mixing even in case of low right-handed neutrino mass scale (of the order of GeV). This implies large lepton flavor violation. As example we…

高能物理 - 唯象学 · 物理学 2024-03-05 Stefano Morisi

The seesaw mechanism is the most popular explanation for the smallness of neutrino masses. However, its high scale makes direct tests impossible and only indirect signals at low energies are reachable for collider experiments. One of these…

高能物理 - 唯象学 · 物理学 2015-03-17 Avelino Vicente

A Standard Model extension with two Majorana neutrinos can explain the measured neutrino masses and mixings, and also account for the matter-antimatter asymmetry in a region of parameter space that could be testable in future experiments.…

高能物理 - 唯象学 · 物理学 2017-08-02 A. Caputo , P. Hernandez , J. Lopez-Pavon , J. Salvado

If neutrino masses are obtained via the canonical seesaw mechanism, based on an underlying 2X2 mass matrix, unitarity violation of the neutrino mixing matrix is unavoidable, but its effect is extremely small. On the other hand, in the…

高能物理 - 唯象学 · 物理学 2010-11-15 Ernest Ma

The seesaw mechanism is attractive not only because it "explains'' small neutrino mass, but also because of its packaging with the SUSY-GUT, leptogenesis, Dark Matter, and electroweak symmetry breaking. However, this package has the flavor,…

高能物理 - 唯象学 · 物理学 2009-09-29 Hitoshi Murayama