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Related papers: Composite Weak Bosons and Dark Matter

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The weak bosons are bound states of two fermions and their antiparticles, denoted as haplons. The confinement scale of the associated gauge group SU(2) is of the order of 0.5 TeV. Besides the weak bosons there exist also new bosons, an…

High Energy Physics - Phenomenology · Physics 2013-04-17 Harald Fritzsch

The weak bosons are bound states of new constituents. The p-wave excitations are studied. The state with the lowest mass is identified with the boson, which has been discovered at the LHC. Specific properties of the excited bosons are…

High Energy Physics - Phenomenology · Physics 2017-07-04 Harald Fritzsch

The weak bosons consist of two fermions, bound by a new confining gauge force. The mass scale of this new interaction is determined. At energies below 0.5 TeV the standard electroweak theory is valid. A neutral isoscalar weak boson X must…

High Energy Physics - Phenomenology · Physics 2015-05-28 Harald Fritzsch

The weak bosons are bound states of fermions. Here the excitations of the weak bosons are discussed. Especially we study the decays of these excited states into weak bosons and photons.

High Energy Physics - Phenomenology · Physics 2017-04-26 Harald Fritzsch

The leptons, quarks and weak bosons are bound states of new constituents. An isosinglet weak boson should exist, the X particle, which might have a mass of about 400 GeV and a width of about 20 GeV.

High Energy Physics - Phenomenology · Physics 2022-01-06 Harald Fritzsch

The weak bosons, leptons and quarks are considered as composite particles. The interaction of the constituents is a confining gauge interaction. The standard electroweak model is a low energy approximation. The mixing of the neutral weak…

High Energy Physics - Phenomenology · Physics 2010-11-05 Harald Fritzsch

The dark sector of the Universe is beginning to be clarified step by step. If the dark energy is vacuum energy, then 123 orders are exactly reduced by ordinary physical processes. For many years these unexplained orders were called a crisis…

General Physics · Physics 2017-05-31 Vladimir Burdyuzha

Dark matter (comprising a quarter of the Universe) is usually assumed to be due to one and only one weakly interacting particle which is neutral and absolutely stable. We consider the possibility that there are several coexisting…

High Energy Physics - Phenomenology · Physics 2007-12-03 Qing-Hong Cao , Ernest Ma , Jose Wudka , C. -P. Yuan

Dark matter is postulated as a light fermion in two natural scenarios as the outcome of a softly broken discrete symmetry. It is produced from the naturally suppressed decay of the standard-model Higgs boson through the freeze-in mechanism.

High Energy Physics - Phenomenology · Physics 2024-09-25 Ernest Ma

If the preon structure of quarks, leptons and gauge bosons will be proved then in the Universe during relativistic phase transition the production of nonperturbative preon condensates has been occured collective excitations of which are…

High Energy Physics - Phenomenology · Physics 2009-09-25 V. Burdyuzha , O. Lalakulich , Yu. Ponomarev , G. Vereshkov

The nonbaryonic dark matter of the Universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro world and particle candidates for cosmological dark matter are the lightest particles that bear new…

High Energy Physics - Phenomenology · Physics 2015-06-18 M. Yu. Khlopov

We suggest that dark matter can be identified with a stable composite fermion X^0, that arises within the holographic AdS/CFT models, where the Higgs boson emerges as a composite pseudo-goldstone boson. The predicted properties of X^0…

High Energy Physics - Phenomenology · Physics 2009-04-24 J. Lorenzo Diaz-Cruz

The low velocity part of a kinetic equilibrium dark matter distribution has higher phase space density and is more easily incorporated in formation of a low mass galaxy than the high velocity part. For relativistically decoupling fermions…

Astrophysics · Physics 2009-10-31 Jes Madsen

Particle physics candidates for cosmological dark matter are usually considered as neutral and weakly interacting. However stable charged leptons and quarks can also exist and, hidden in elusive atoms, play the role of dark matter. The…

Astrophysics · Physics 2008-01-03 M. Yu. Khlopov

The nonbaryonic dark matter of the Universe can consist of new stable charged leptons and quarks, if they are hidden in elusive "dark atoms" of composite dark matter. Such possibility can be compatible with the severe constraints on…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Maxim Yu. Khlopov

In this review of Dark Matter we review dark matter as sterile neutrinos, fermions, with their present and possibly future detection via neutrino Oscillations. We review the creation of Dark Matter via interactions with the Dark Energy…

General Physics · Physics 2020-01-10 Leonard S. Kisslinger , Debasish Das

Heavy stable charged particles can exist, hidden from us in bound atomlike states. Models with new stable charged leptons and quarks give rise to realistic composite dark matter scenarios. Significant or even dominant component of O-helium…

Astrophysics · Physics 2008-06-25 Maxim Yu. Khlopov

Dark Matter might be an accidentally stable baryon of a new confining gauge interaction. We extend previous studies exploring the possibility that the DM is made of dark quarks heavier than the dark confinement scale. The resulting…

High Energy Physics - Phenomenology · Physics 2017-11-21 Andrea Mitridate , Michele Redi , Juri Smirnov , Alessandro Strumia

The existence of cosmological dark matter is in the bedrock of the modern cosmology. The dark matter is assumed to be nonbaryonic and to consist of new stable particles. However if composite dark matter contains stable electrically charged…

High Energy Physics - Phenomenology · Physics 2018-05-02 Maxim Yu. Khlopov

The instability of dark matter may produce visible signals in the spectrum of cosmic gamma-rays. We consider this possibility in frameworks with additional spatial dimensions and supersymmetry. Examples of particles include…

Astrophysics · Physics 2011-11-10 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari
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