scholarly journals Cosmology of the Twin Higgs without explicit ℤ2 breaking

2021 ◽  
Vol 2021 (12) ◽  
Author(s):  
Hugues Beauchesne ◽  
Yevgeny Kats

Abstract The cosmology of the Twin Higgs requires the breaking of the ℤ2 symmetry, but it is still an open question whether this breaking needs to be explicit. In this paper, we study how the Mirror Twin Higgs could be modified to be compatible with current cosmological constraints without explicit ℤ2 breaking. We first present a simple toy model that can realize baryogenesis without explicit ℤ2 breaking or reaching temperatures that would lead to domain walls. The model can also either solve the Neff problem and bring the abundance of mirror atoms to an allowed level or provide the correct dark matter abundance. We then present another simple model that leads to mirror neutron dark matter and thus acceptable dark matter self-interactions. We also include in appendix a series of results on energy exchange between different sectors that might prove useful for other cosmological problems.

2013 ◽  
Vol 22 (14) ◽  
pp. 1350082 ◽  
Author(s):  
SHUO CAO ◽  
NAN LIANG

In order to test if there is energy transfer between dark energy (DE) and dark matter (DM), we investigate cosmological constraints on two forms of nontrivial interaction between the DM sector and the sector responsible for the acceleration of the universe, in light of the newly revised observations including OHD, CMB, BAO and SNe Ia. More precisely, we find the same tendencies for both phenomenological forms of the interaction term Q = 3γHρ, i.e. the parameter γ to be a small number, |γ| ≈ 10-2. However, concerning the sign of the interaction parameter, we observe that γ > 0 when the interaction between dark sectors is proportional to the energy density of dust matter, whereas the negative coupling (γ < 0) is preferred by observations when the interaction term is proportional to DE density. We further discuss two possible explanations to this incompatibility and apply a quantitative criteria to judge the severity of the coincidence problem. Results suggest that the γm IDE model with a positive coupling may alleviate the coincidence problem, since its coincidence index C is smaller than that for the γd IDE model, the interacting quintessence and phantom models by four orders of magnitude.


2009 ◽  
Author(s):  
Ki-Young Choi ◽  
Csaba Balazs ◽  
Fei Wang

2021 ◽  
Vol 2021 (02) ◽  
pp. 019-019
Author(s):  
Niklas Becker ◽  
Deanna C. Hooper ◽  
Felix Kahlhoefer ◽  
Julien Lesgourgues ◽  
Nils Schöneberg

2004 ◽  
Vol 70 (4) ◽  
Author(s):  
Sergio del Campo ◽  
Ramón Herrera ◽  
Diego Pavón

2010 ◽  
Vol 19 (03) ◽  
pp. 305-316 ◽  
Author(s):  
AHMAD SHEYKHI

We consider the agegraphic models of dark energy in a braneworld scenario with brane–bulk energy exchange. We assume that the adiabatic equation for the dark matter is satisfied while it is violated for the agegraphic dark energy due to the energy exchange between the brane and the bulk. Our study shows that with the brane–bulk interaction, the equation of state parameter of agegraphic dark energy on the brane, wD, can have a transition from the normal state, where wD > -1, to the phantom regime, where wD < -1, while the effective equation of state for dark energy always satisfies [Formula: see text].


2018 ◽  
Vol 782 ◽  
pp. 1-5 ◽  
Author(s):  
Keisuke Harigaya ◽  
Masahiro Kawasaki
Keyword(s):  

1997 ◽  
Vol 180 ◽  
pp. 268-268
Author(s):  
G. Pascoli

The physico-chemical origin of the hydrogenated carbon clusters (cumulenes, PAHs, graphite or amorphous carbon) in space is still an open question. We have worked out a numerical simulation code in order to build up planar (graphite-like) carbon clusters. We assume that hydrogen atoms can fix on the carbon skeleton following a random process allowing for H2 formation. The structures we have found are very complex. In a given cluster, several molecular entities can simultaneously be present: (sp2) carbon chains, rings or compact formations (aromatic structures or small PAHs). We argue that these very contorted hydrogenated structures could be ubiquitous in the interstellar medium, in carbon-rich circumstellar regions and in PNe.


2016 ◽  
Vol 93 (4) ◽  
Author(s):  
Ruth Lazkoz ◽  
Iker Leanizbarrutia ◽  
Vincenzo Salzano

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