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We propose a strongly coupled supersymmetric gauge theory that can accommodate both the inflation (in the form of generalized hybrid inflation) and dark matter (DM). In this set-up, we identify the DM as the Goldstones associated with the…

高能物理 - 唯象学 · 物理学 2018-11-14 Subhaditya Bhattacharya , Abhijit Kumar Saha , Arunansu Sil , Jose Wudka

The cosmological solutions of the non-minimal $ Y (R)F^2 $ theory which are compatible with FRW space-time are investigated. In order to avoid the isotropy violation of a vector field, it can be considered that the presence of a triplet of…

广义相对论与量子宇宙学 · 物理学 2019-12-24 Özcan Sert

We classify the cosmological behaviors of the domain wall under junctions between two spacetimes in terms of various parameters: cosmological constants of bulk spacetime, a tension of a domain wall, and mass parameters of the black…

高能物理 - 理论 · 物理学 2008-11-26 Bum-Hoon Lee , Wonwoo Lee , Siyoung Nam , Chanyong Park

The 2015 Planck data release has placed tight constraints on the allowed class of inflationary models. The current data favors concave downwards inflationary potentials while offering interesting hints on possible deviations from the…

宇宙学与河外天体物理 · 物理学 2017-03-08 Eleonora Di Valentino , Laura Mersini-Houghton

After decades of successful hot big-bang paradigm, Cosmology still lacks a framework in which the early inflationary phase of the universe smoothly matches the radiation epoch and evolves to the present `quasi' de Sitter spacetime. No less…

宇宙学与河外天体物理 · 物理学 2015-06-16 S. Basilakos , J. A. S. Lima , J. Solà

We study the cosmology of the Supersymmetric Standard Model augmented by a gauge singlet to solve the $\mu$-problem and describe the evolution of the domain walls which are created during electroweak symmetry breaking due to the discrete…

高能物理 - 唯象学 · 物理学 2008-11-26 S. A. Abel , S. Sarkar , P. L. White

A radiative seesaw model with an inert doublet dark matter is a promising candidate which could explain the existence of neutrino masses, dark matter and baryon number asymmetry of the Universe, simultaneously. In addition to these issues,…

高能物理 - 唯象学 · 物理学 2015-09-23 Shoichi Kashiwase

We present a solution to the cosmological problem encountered in (supersymmetric) grand unified theories due to copious monopole production at the end of hybrid inflation. By employing thermal inflation ``driven'' by the U(1) axion…

高能物理 - 唯象学 · 物理学 2008-11-26 G. Lazarides , Q. Shafi

We discuss the entropy and the size/homogeneity/horizon problems in power-law expanding universes with one scale initial conditions. We set the minimal scale $\Lambda = 10^{25}$ GeV at which a non-inflationary solution is possible and show…

高能物理 - 唯象学 · 物理学 2009-01-07 Natalia Shuhmaher

We revisit the compatibility between the chaotic inflation, which provides a natural solution to the initial condition problem, and the metastable electroweak vacuum, which is suggested by the results of LHC and the current mass…

高能物理 - 唯象学 · 物理学 2016-11-22 Masahiro Kawasaki , Kyohei Mukaida , Tsutomu T. Yanagida

If we interpret the Bekenstein-Hawking entropy of the Hubble horizon as thermodynamic entropy, then the entanglement entropy of the superhorizon modes of curvature perturbation entangled with the subhorizon modes will exceed the…

广义相对论与量子宇宙学 · 物理学 2023-07-18 Ngo Phuc Duc Loc

TeV size extra dimensions introduce domain walls. Such walls are inconsistent with CMB anisotropies. Either inflationary dynamics washes them out, or the reheating temperature is lower then the temperature at which the walls start forming…

高能物理 - 唯象学 · 物理学 2007-05-23 C. P. Korthals Altes

We summarize three recent efforts to constrain the first few moments of cosmic creation before and during the epoch of inflation. We consider two means to explain a slight dip in the power spectrum of the cosmic microwave background for…

宇宙学与河外天体物理 · 物理学 2015-10-19 G. J. Mathews , M. R. Gangopadhyay , P. Garnavich , B. Rose , K. Ichiki , T. Kajino , D. Yamazaki

It is shown that late-time decay of domain walls can dilute unwanted relics such as moduli, if the universe was dominated by frustrated domain walls with tension $\sigma = (1 - 100 TeV)^3$. Since energy density of the frustrated domain…

高能物理 - 唯象学 · 物理学 2009-11-10 Masahiro Kawasaki , Fuminobu Takahashi

Phantom Cosmology provides an unique opportunity to "connect" the phantom driven (low en- ergy meV scale) dark energy phase to the (high energy GUT scale) inflationary era. This is possible because the energy density increases in phantom…

宇宙学与河外天体物理 · 物理学 2013-05-29 Cosmin Ilie , Tirthabir Biswas , Katherine Freese

If inflation occurs after the breaking of Peccei-Quinn symmetry then large values of the breaking scale $F$, which are forbidden in conventional axion cosmology, are permitted, provided that we inhabit a region of the Multiverse where the…

高能物理 - 唯象学 · 物理学 2007-05-23 Frank Wilczek

We analyze the cosmological consequences of locked inflation, a model recently proposed by Dvali and Kachru that can produce significant amounts of inflation without requiring slow-roll. We pay particular attention to the end of inflation…

高能物理 - 理论 · 物理学 2009-11-10 Richard Easther , Justin Khoury , Koenraad Schalm

The recent measurement of a cutoff k_min in the fluctuation power spectrum P(k) of the cosmic microwave background may vitiate the possibility that slow-roll inflation can simultaneously solve the horizon problem and account for the…

宇宙学与河外天体物理 · 物理学 2021-03-10 Fulvio Melia

Using the dS/QFT correspondence in the context of inflation allows for the study of interesting, otherwise inaccessible physics. In particular, by studying inflation via its dual field theory at the boundary of the de Sitter space, it may…

宇宙学与河外天体物理 · 物理学 2011-08-08 Mafalda Dias

We discuss inflationary cosmology in a five dimensional SO(10) model compactified on $S^1/(Z_2\times Z_2')$, which yields $SU(3)_c\times SU(2)_L\times U(1)_Y\times U(1)_X$ below the compactification scale. The gauge symmetry $SU(5)\times…

高能物理 - 唯象学 · 物理学 2014-11-17 Bumseok Kyae , Qaisar Shafi