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A field theory is studied where the consistency condition of equations of motion dictates strong correlation between states of "primordial" fermion fields and local value of the dark energy. In regime of the fermion densities typical for…

高能物理 - 理论 · 物理学 2007-05-23 E. I. Guendelman , A. B. Kaganovich

A field theory is proposed where the regular fermionic matter and the dark fermionic matter are different states of the same "primordial" fermion fields. In regime of the fermion densities typical for normal particle physics, the primordial…

高能物理 - 理论 · 物理学 2016-11-09 E. I. Guendelman , A. B. Kaganovich

A field theory is proposed where the regular fermionic matter and the dark fermionic matter are different states of the same "primordial" fermion fields. In regime of the fermion densities typical for normal particle physics, the primordial…

广义相对论与量子宇宙学 · 物理学 2007-05-23 E. I. Guendelman , A. B. Kaganovich

A field theory is proposed where the regular fermionic matter and the dark fermionic matter are different states of the same "primordial" fermion fields. In regime of the fermion densities typical for normal particle physics, each of the…

广义相对论与量子宇宙学 · 物理学 2009-11-10 E. I. Guendelman , A. B. Kaganovich

There exist field theory models where the fermionic energy-momentum tensor contains a term proportional to g_{\mu\nu}\bar{\Psi}\Psi which can be responsible for a dark matter to dark energy transmutation. We study some cosmological aspects…

高能物理 - 理论 · 物理学 2007-05-23 E. I. Guendelman , A. B. Kaganovich

We study a new field theory effect in the cosmological context in the Two Measures Field Theory (TMT). TMT is an alternative gravity and matter field theory where the gravitational interaction of fermionic matter is reduced to that of…

广义相对论与量子宇宙学 · 物理学 2010-11-05 E. I. Guendelman , A. B. Kaganovich

In a dense cloud of massive fermions interacting by exchange of a light scalar field, the effective mass of the fermion can become negligibly small. As the cloud expands, the effective mass and the total energy density eventually increase…

高能物理 - 唯象学 · 物理学 2016-11-15 T. Goldman , G. J. Stephenson , P. M. Alsing , B. H. J. McKellar

Dark matter (DM) with a mass below a few keV must have a phase space distribution that differs substantially from the Standard Model particle thermal phase space: otherwise, it will free stream out of cosmic structures as they form. We…

高能物理 - 唯象学 · 物理学 2021-08-09 Marcela Carena , Nina M. Coyle , Ying-Ying Li , Samuel D. McDermott , Yuhsin Tsai

A model for the Universe is proposed whose constituents are: (a) a dark energy field modeled by a fermionic field non-minimally coupled with the gravitational field, (b) a matter field which consists of pressureless baryonic and dark matter…

广义相对论与量子宇宙学 · 物理学 2008-11-26 M. O. Ribas , F. P. Devecchi , G. M. Kremer

We propose a renormalizable theory with minimal particle content and symmetries, that successfully explains the number of Standard Model (SM) fermion families, the SM fermion mass hierarchy, the tiny values for the light active neutrino…

高能物理 - 唯象学 · 物理学 2020-09-16 A. E. Cárcamo Hernández , D. T. Huong , H. N. Long

Extension of particle symmetry implies new conserved charges and the lightest particles, possessing such charges, should be stable. Created in early Universe, stable charged heavy leptons and quarks can exist and, hidden in elusive atoms…

天体物理学 · 物理学 2007-05-23 Maxim Yu. Khlopov

Quantum fields are considered as generators of infinite-dimensional Clifford algebra $Cl(\infty)$, which can be either orthogonal (in case of fermions) or symplectic (in case of bosons). A generic quantum state can be expressed as a…

综合物理 · 物理学 2022-08-31 Matej Pavšič

This paper reports improvements and new results for a well developed theory of tachyons (faster-than-light particles) and follows the suggestion that neutrinos - especially the low energy neutrinos in the Cosmic Neutrino Background - may be…

综合物理 · 物理学 2025-06-23 Charles Schwartz

To explain the acceleration of the cosmological expansion researchers have considered an unusual form of mass-energy generically called dark energy. Dark energy has a ratio of pressure over mass density which obeys $w=p/\rho <-1/3$. This…

高能物理 - 理论 · 物理学 2008-12-19 Max Chaves , Douglas Singleton

Dark Matter constitutes most of the matter in the presently accepted cosmological model for our Universe. The extreme conditions of ordinary baryonic matter, namely high density and compactness, in Neutron Stars make these objects suitable…

高能天体物理现象 · 物理学 2017-10-20 M. Cermeño , M. Ángeles Pérez-García , Joseph Silk

In an earlier paper I proposed a highly symmetric semi-classical initial condition to describe the universe in the period leading up to the electroweak transition and completely determine all cosmology after that. Nothing beyond the…

宇宙学与河外天体物理 · 物理学 2022-03-25 Daniel Friedan

We explore the physics of a gas of particles interacting with a condensate that spontaneously breaks Lorentz invariance. The equation of state of this gas varies from 1/3 to less than -1 and can lead to the observed cosmic acceleration. The…

天体物理学 · 物理学 2009-11-10 Simon DeDeo

A fermion ground state energy functional is set up in terms of particle density, relative pair density, and kinetic energy tensor density. It satisfies a minimum principle if constrained by a complete set of compatibility conditions. A…

化学物理 · 物理学 2009-10-17 Bin Liu , Jerome K. Percus

The phenomenon of emergent physics in condensed-matter many-body systems has become the paradigm of modern physics, and can probably also be applied to high-energy physics and cosmology. This encouraging fact comes from the universal…

强关联电子 · 物理学 2009-11-11 G. E. Volovik

We study the physical conditions for the occurrence of ferromagnetic instability in a neutral plasma of fermions. We consider a system of two species $M$ and $Y$ which are oppositely charged under a local $U(1)_{X}$, with $M$ much lighter…

宇宙学与河外天体物理 · 物理学 2019-01-21 R. B. MacKenzie , M. B. Paranjape , U. A. Yajnik
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