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相关论文: Common Origin of Visible and Dark Universe

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Dark and baryonic matter contribute comparable energy density to the present Universe. The dark matter may also be responsible for the cosmic positron/electron excesses. We connect these phenomena with Dirac seesaw for neutrino masses. In…

高能物理 - 唯象学 · 物理学 2009-10-29 Pei-Hong Gu , Utpal Sarkar , Xinmin Zhang

We investigate the possibility that both the baryon asymmetry of the universe and the observed cold dark matter density are generated by decays of a heavy scalar field which dominates the universe before nucleosynthesis. Since baryons and…

高能物理 - 唯象学 · 物理学 2008-11-26 Ryuichiro Kitano , Hitoshi Murayama , Michael Ratz

The similar cosmological energy budgets in visible baryons and dark matter motivate one to consider a common origin for the generation of both. We outline the key features of scenarios that can accommodate a unified framework for the…

高能物理 - 唯象学 · 物理学 2015-06-04 Hooman Davoudiasl , Rabindra N. Mohapatra

In a baryon-symmetric universe, the baryon asymmetry observed for visible matter is matched by an equal and opposite asymmetry for dark matter, thereby closely connecting the number densities of both types of matter. This is a necessary…

高能物理 - 唯象学 · 物理学 2015-06-12 Raymond R. Volkas

We explore a new origin of neutrino dark energy and baryon asymmetry in the universe. The neutrinos acquire small masses through the Dirac seesaw mechanism. The pseudo-Nambu-Goldstone boson associated with neutrino mass-generation provides…

高能物理 - 唯象学 · 物理学 2009-01-06 Pei-Hong Gu , Hong-Jian He , Utpal Sarkar

In the present universe visible and dark matter contribute comparable energy density although they have different properties. This coincidence can be elegantly explained if the dark matter relic density, originating from a dark matter…

高能物理 - 唯象学 · 物理学 2011-09-05 Pei-Hong Gu , Manfred Lindner , Utpal Sarkar , Xinmin Zhang

The similar mass densities observed for visible and dark matter in the present-day universe suggest a common origin for both. A scheme called "pangenesis" for realising this using the Affleck-Dine mechanism in a baryon-symmetric universe is…

高能物理 - 唯象学 · 物理学 2015-06-04 Raymond R. Volkas

We investigate the possibility that dark matter and the baryon asymmetry of the Universe are generated by the same mechanism, following an idea initially proposed by V.A. Kuzmin and recently discussed by R. Kitano and I. Low. In our model,…

高能物理 - 唯象学 · 物理学 2009-11-11 Nicolas Cosme , Laura Lopez Honorez , Michel H. G. Tytgat

In this work, we explain three beyond standard model (BSM) phenomena, namely neutrino masses, the baryon asymmetry of the Universe and Dark Matter, within a single model and in each explanation the right handed (RH) neutrinos play the prime…

高能物理 - 唯象学 · 物理学 2019-06-26 Anirban Biswas , Sandhya Choubey , Laura Covi , Sarif Khan

The similar cosmological abundances observed for visible and dark matter suggest a common origin for both. By viewing the dark matter density as a dark-sector asymmetry, mirroring the situation in the visible sector, we show that the…

高能物理 - 唯象学 · 物理学 2012-03-01 Kalliopi Petraki , Mark Trodden , Raymond R. Volkas

We propose a new model to explain the neutrino masses, the dark energy and the baryon asymmetry altogether. In this model, neutrinos naturally acquire small Majorana masses via type-II seesaw mechanism, while the pseudo-Nambu-Goldstone…

高能物理 - 唯象学 · 物理学 2008-11-26 Pei-Hong Gu , Hong-Jian He , Utpal Sarkar

In this paper we present a possible origin of dark matter and dark energy from a solution of the Einstein's equation to a primordial universe, which was presented in a previous paper. We also analyze the Dirac's equation in this primordial…

广义相对论与量子宇宙学 · 物理学 2010-10-01 A. C. V. V. de Siqueira

Combining one established idea with two recent ones, it is pointed out for the first time that three of the outstanding problems of particle physics and cosmology, i.e. neutrino mass, dark matter, and baryogenesis, may have a common…

高能物理 - 唯象学 · 物理学 2009-11-11 Ernest Ma

A physical mechanism that produces three energy components is proposed as the common origin of dark energy and dark matter. The first two have equations of state W ~ 0 and act like dark matter, while the last has W ~ -1 at low redshifts…

广义相对论与量子宇宙学 · 物理学 2012-12-12 I. Gontijo

We propose a new solution to the origin of dark energy. We suggest that it was created dynamically from the condensate of a singlet neutrino at a late epoch of the early Universe through its effective self interaction. This singlet neutrino…

高能物理 - 唯象学 · 物理学 2014-11-20 Jitesh R. Bhatt , Bipin R. Desai , Ernest Ma , G. Rajasekaran , Utpal Sarkar

About 80\% of the mass of the present Universe is made up of the unknown (dark matter), while the rest is made up of ordinary matter. It is a very intriguing question why the {\it mass} densities of dark matter and ordinary matter (mainly…

高能物理 - 唯象学 · 物理学 2019-10-23 Masahiro Ibe , Ayuki Kamada , Shin Kobayashi , Takumi Kuwahara , Wakutaka Nakano

We propose a new framework for explaining the proximity of the baryon and dark matter relic densities \Omega_{DM} \approx 5\Omega_B. The scenario assumes that the number density of the observed dark matter states is generated due to decays…

高能物理 - 唯象学 · 物理学 2015-06-12 James Unwin

The cosmological origin of both dark and baryonic matter can be explained through a unified mechanism called hylogenesis where baryon and antibaryon number are divided between the visible sector and a GeV-scale hidden sector, while the…

高能物理 - 唯象学 · 物理学 2012-12-04 Nikita Blinov , David E. Morrissey , Kris Sigurdson , Sean Tulin

For the first time, we have a plausible, complete accounting of matter and energy in the Universe. Expressed a fraction of the critical density it goes like this: neutrinos, between 0.3% and 15%; stars, 0.5%; baryons (total), 5%; matter…

天体物理学 · 物理学 2007-05-23 Michael S. Turner

For the first time, we have a plausible and complete accounting of matter and energy in the Universe. Expressed a fraction of the critical density it goes like this: neutrinos, between 0.3% and 15%; stars, between 0.3% and 0.6%; baryons…

天体物理学 · 物理学 2009-10-31 Michael S. Turner
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