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相关论文: Dark Matter from the vector of SO(10)

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In constrained minimal supersymmetry the lightest neutralino of bino-type is the only neutral candidate for dark matter. As a result, one is typically able to restrict all the supersymmetric mass spectra below roughly 1-2\tev\ {\em without}…

高能物理 - 唯象学 · 物理学 2008-02-03 G. L. Kane , Chris Kolda , Leszek Roszkowski , James D. Wells

We show how the Higgs boson mass is protected from the potentially large corrections due to the introduction of minimal dark matter if the new physics sector is made supersymmetric. The fermionic dark matter candidate (a 5-plet of…

高能物理 - 唯象学 · 物理学 2016-03-23 Marco Fabbrichesi , Alfredo Urbano

The existence of the neutrino mass and flavor mixing have been experimentally verified. These phenomena strongly motivate to extend the Standard Model (SM). Amongst many possibilities, a simple and interesting extension of the SM can be…

高能物理 - 唯象学 · 物理学 2020-12-01 Arindam Das , Kazuki Enomoto , Shinya Kanemura

The hypothesis that Dark Matter is one electroweak multiplet leads to predictive candidates with multi-TeV masses that can form electroweak bound states. Bound states with the same quantum numbers as electroweak vectors are found to be…

高能物理 - 唯象学 · 物理学 2021-06-28 Salvatore Bottaro , Alessandro Strumia , Natascia Vignaroli

We propose a dark matter model in which the dark sector is gauged under a new SU(2) group. The dark sector consists of SU(2) dark gauge fields, two triplet dark Higgs fields, and two dark fermion doublets (dark matter candidates in this…

高能物理 - 唯象学 · 物理学 2014-11-20 Hao Zhang , Chong Sheng Li , Qing-Hong Cao , Zhao Li

We present a simple and natural dark sector model in which dark matter particles arise as composite states of hidden strong dynamics and their stability is ensured by accidental symmetries. The model has only a few free parameters. In…

高能物理 - 唯象学 · 物理学 2017-03-15 Raymond T. Co , Keisuke Harigaya , Yasunori Nomura

In a recent paper, we proposed a new class of supersymmetric SO(10) models for neutrino masses where the TeV scale electroweak symmetry is SU(2)_L\times SU(2)_R\times U(1)_{B-L} making the associated gauge bosons W_R and Z' accessible at…

高能物理 - 唯象学 · 物理学 2015-03-13 P. S. Bhupal Dev , R. N. Mohapatra

We present a new model of "Stealth Dark Matter": a composite baryonic scalar of an $SU(N_D)$ strongly-coupled theory with even $N_D \geq 4$. All mass scales are technically natural, and dark matter stability is automatic without imposing an…

We construct supersymmetric models of SO(10) unification in which the gauge symmetry is broken by orbifold compactification. We find that using boundary conditions to break the gauge symmetry down to $SU(3)_C \otimes SU(2)_L \otimes U(1)_Y…

高能物理 - 唯象学 · 物理学 2008-11-26 Lawrence Hall , Yasunori Nomura , Takemichi Okui , David Smith

Self-interacting dark matter (SIDM) is a simple and well-motivated scenario that could explain long-standing puzzles in structure formation on small scales. If the required self-interaction arises through a light mediator (with mass $\sim…

高能物理 - 唯象学 · 物理学 2015-11-04 Eugenio Del Nobile , Manoj Kaplinghat , Hai-Bo Yu

We propose a class of dark matter models based on a chiral $U(1)$ gauge symmetry acting on a dark sector. The chiral $U(1)$ protects the masses of the dark sector fermions, and also guarantees the stability of the dark matter particle by…

高能物理 - 唯象学 · 物理学 2025-02-07 K. S. Babu , Shreyashi Chakdar , Vishnu P. K

In this work, we study an extension of the Standard Model which includes a new massive vector field in the fundamental representation of SU(2)_L. The neutral component of the new vector field is a natural dark matter candidate. We compute…

高能物理 - 唯象学 · 物理学 2024-12-11 Sebastian Acevedo , Alfonso R. Zerwekh

To explain the dark matter and the baryon asymmetry of the Universe, the parameters of the $\nu$MSM (an extension of the Minimal Standard Model by three singlet neutrinos with masses smaller than the electroweak scale) must be fine-tuned:…

高能物理 - 唯象学 · 物理学 2008-11-26 Mikhail Shaposhnikov

We investigate and compare two simple models of dark matter (DM): a vector and a scalar DM model. Both models require the presence of two physical Higgs bosons $h_1$ and $h_2$ which come from mixed components of the standard Higgs doublet…

高能物理 - 唯象学 · 物理学 2019-01-16 Duarte Azevedo , Mateusz Duch , Bohdan Grzadkowski , Da Huang , Michal Iglicki , Rui Santos

We propose the existence of a hidden or dark sector besides the standard model (SM) of particle physics, whose members (both fermionic and bosonic) obey a local SU(2)$_{\rm H}$ gauge symmetry while behaving like a singlet under the SM gauge…

高能物理 - 唯象学 · 物理学 2016-07-12 Amit Dutta Banik , Debasish Majumdar , Anirban Biswas

We propose a simple non-supersymmetric grand unified theory (GUT) based on the gauge group $SO(10) \times U(1)_\psi$. The model includes 3 generations of fermions in ${\bf 16}$ ($+1$), ${\bf 10}$ ($-2$) and ${\bf 1}$ ($+4$) representations.…

高能物理 - 唯象学 · 物理学 2019-07-01 Nobuchika Okada , Digesh Raut , Qaisar Shafi

We study a renormalizable model of Dirac fermion dark matter (DM) that communicates with the Standard Model (SM) through a pair of mediators -- one scalar, one fermion -- in the representation $(\boldsymbol{6},\boldsymbol{1}, \tfrac{4}{3})$…

高能物理 - 唯象学 · 物理学 2022-09-27 Linda M. Carpenter , Taylor Murphy , Tim M. P. Tait

The minimal $SO(10)$ grand unified theory, augmented by higher-dimensional operators, is based on the following Higgs representations: adjoint $45_{\rm H}$, spinor $16_{\rm H}$ and complex vector $10_{\rm H}$. It was recently realized that,…

高能物理 - 唯象学 · 物理学 2024-10-28 Anca Preda , Goran Senjanović , Michael Zantedeschi

A good fit of the fermion masses and mixings has been found in the minimal renormalizable supersymmetric SO(10). This solution needs a strongly split supersymmetry breaking scenario with gauginos and higgsinos around 100 TeV, sfermions…

高能物理 - 唯象学 · 物理学 2009-01-06 Borut Bajc , Ilja Dorsner , Miha Nemevsek

Asymmetric symmetry breaking models dynamically break the G X G gauge symmetries of mirror models to distinct subgroups in the two sectors. The coincidental abundances of visible and dark matter, $\Omega_{DM} \simeq 5\Omega_{VM}$, motivates…

高能物理 - 唯象学 · 物理学 2015-07-08 Stephen J. Lonsdale
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