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相关论文: Testing the see-saw mechanism at collider energies

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A gauged $U(1)_X$ extension of the Standard Model is a simple and consistent framework to naturally incorporate three right-handed neutrinos (RHNs) for generating the observed light neutrino masses and mixing by the type-I seesaw mechanism.…

高能物理 - 唯象学 · 物理学 2019-11-13 Arindam Das , P. S. Bhupal Dev , Nobuchika Okada

If neutrino masses are realized through the see-saw mechanism, can the right-handed neutrinos be produced and detected at present and future colliders? The answer is negative in the most popular see-saw scenarios for the simple reason that…

高能物理 - 唯象学 · 物理学 2008-11-26 P. Q. Hung

We discuss the scenario with TeV-scale right-handed neutrinos, which are accessible at future colliders, while holding down tiny seesaw-induced masses and sizable couplings to the standard-model particles. The signal with tri-lepton final…

高能物理 - 唯象学 · 物理学 2009-11-19 Naoyuki Haba , Shigeki Matsumoto , Koichi Yoshioka

We discuss phenomenology of the radiative seesaw model in which spontaneous breaking of the U(1)$_{B-L}$ gauge symmetry at the TeV scale gives the common origin for masses of neutrinos and dark matter (Kanemura et al., 2012). In this model,…

高能物理 - 唯象学 · 物理学 2013-05-30 Shinya Kanemura , Takehiro Nabeshima , Hiroaki Sugiyama

We review the low energy constraints on type I see-saw extensions of the Standard Model in which the scale of new physics, associated to lepton number violation, can be probed at current collider searches. In such scenarios, the flavour…

高能物理 - 唯象学 · 物理学 2011-11-15 Emiliano Molinaro

The fact that neutrinos are massive indicates that the Standard Model (SM) requires extension. We propose a low energy (<TeV) B-L extension of the SM, which is based on the gauge group SU(3)_C x SU(2)_L x U(1)_Y x U(1)_{B-L}. We show that…

高能物理 - 唯象学 · 物理学 2008-11-26 Shaaban Khalil

We study a type I see-saw scenario where the right-handed (RH) neutrinos, responsible for the light neutrino mass generation, lie at the electroweak scale. Under certain conditions, the strength of the charged and neutral current weak…

高能物理 - 唯象学 · 物理学 2011-08-08 A. Ibarra , E. Molinaro , S. T. Petcov

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

Seesaw mechanisms are the simplest and the most elegant way of generating small masses for the active neutrinos $(m_\nu)$. In these mechanisms $m_\nu$ is inversely proportional to the lepton number breaking scale $(M)$ that, in the…

高能物理 - 唯象学 · 物理学 2023-05-01 E. Cabrera , D. Cogollo , C. A. de S. Pires

We consider the Standard Model with right-handed neutrinos to explain the masses of active neutrinos by the seesaw mechanism. Since active neutrinos as well as heavy neutral leptons are Majorana fermions in this case, the lepton number…

高能物理 - 唯象学 · 物理学 2016-01-15 Takehiko Asaka , Takanao Tsuyuki

We study the possibility to test the Type I seesaw mechanism for neutrino masses at the CERN Large Hadron Collider. The inclusion of three generations of right-handed neutrinos (N_i) provides an attractive option of gauging the B-L…

高能物理 - 唯象学 · 物理学 2009-10-29 Pavel Fileviez Perez , Tao Han , Tong Li

We propose a gauged $U(1)_{B-L}$ extension of the standard model (SM) to explain simultaneously the light neutrino masses and dark matter (DM). The generation of neutrino masses occurs through a variant of type-II seesaw mechanism in which…

高能物理 - 唯象学 · 物理学 2020-02-18 Satyabrata Mahapatra , Nimmala Narendra , Narendra Sahu

In many models incorporating the type-I seesaw mechanism, the right-handed neutrino ($N$) couples to heavy vector/scalar bosons and thereby has resonant pair production. It barely receives attention thus far, however, it may provide the…

高能物理 - 唯象学 · 物理学 2016-05-04 Zhaofeng Kang , P. Ko , Jinmian Li

We re-examine the discovery potential at hadron colliders of high-mass right-handed (RH) gauge bosons $W_R$ - an inherent ingredient of Left-Right Symmetric Models (LRSM). We focus on the regime where the $W_R$ is very heavy compared to the…

高能物理 - 唯象学 · 物理学 2017-03-16 Manimala Mitra , Richard Ruiz , Darren J. Scott , Michael Spannowsky

We consider minimal $U(1)$ extensions of the Standard Model in which one of the right-handed neutrinos is charged under the new gauge symmetry and plays the role of dark matter. In particular, we perform a detailed phenomenological study…

高能物理 - 唯象学 · 物理学 2018-01-19 Peter Cox , Chengcheng Han , Tsutomu T. Yanagida

In this work, the standard model (SM) is extended with two right-handed (RH) neutrinos and two singlet neutral fermions to yield active neutrino masses via (2,2) inverse see-saw mechanism. We first validate the multi-dimensional model…

高能物理 - 唯象学 · 物理学 2023-04-26 Indrani Chakraborty , Himadri Roy , Tripurari Srivastava

We propose a modified version of the TeV scale B-L extension of the standard model, where neutrino masses are generated through the inverse seesaw mechanism. We show that heavy neutrinos associated with this model can be accessible via…

高能物理 - 唯象学 · 物理学 2013-05-29 Shaaban Khalil

The Standard Model extended with right-handed neutrinos whose masses are below the electroweak scale provides a simultaneous solution for the origin of neutrino masses and of the baryon asymmetry of the Universe, that can be tested in…

高能物理 - 唯象学 · 物理学 2019-07-01 Michele Lucente

We extend the Type I and Type III seesaw mechanisms to generate neutrino masses within the left-right symmetric theories where parity is spontaneously broken. We construct a next to minimal left-right symmetric model where neutrino masses…

高能物理 - 唯象学 · 物理学 2010-03-17 Joydeep Chakrabortty

We investigate the pair-production of right-handed neutrinos via the Standard Model (SM) Higgs boson in a gauged $B-L$ model. The right-handed neutrinos with a mass of few tens of GeV generating viable light neutrino masses via the seesaw…

高能物理 - 唯象学 · 物理学 2018-09-13 Frank F. Deppisch , Wei Liu , Manimala Mitra
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