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Related papers: Kaluza-Klein relics from warped reheating

200 papers

We attempt to quantify the widely-held belief that large hierarchies induced by strongly-warped geometries are common in the string theory landscape. To this end, we focus on the arguably best-understood subset of vacua -- type IIB…

High Energy Physics - Theory · Physics 2008-11-26 A. Hebecker , J. March-Russell

We describe type $II_A$ cosmological brane inflation scenarios based on the holographic MQCD model of Aharony et al \cite{Aharony:2010mi}. The scenarios can be related via T-duality to the type $II_B$ KKLMMT model \cite{Kachru:2003sx}. They…

High Energy Physics - Theory · Physics 2015-05-30 Horatiu Nastase , Jacob Sonnenschein

In Universal Extra Dimension (UED) scenarios, the lightest Kaluza-Klein (KK) particle is naturally stable due to a remnant discrete symmetry, KK parity, arising from extra-dimensional compactification. This stability requires no ad hoc…

High Energy Physics - Phenomenology · Physics 2026-02-13 Kirtiman Ghosh , Abhishek Roy , Rameswar Sahu

One interpretation of proton stability is the existence of extra-flat directions of the MSSM, in particular $u^{c}u^{c}d^{c}e^{c}$ and $QQQL$, where the operators lifting the potential are suppressed by a mass scale $\Lambda$ which is much…

High Energy Physics - Phenomenology · Physics 2008-11-26 John McDonald , Osamu Seto

In the Einstein frame picture of Starobinky's $R^2$ inflation model, cosmic inflation is driven by a slowly rolling inflaton field, called scalaron, and followed by a coherently oscillating scalaron phase. Since the scalaron oscillates…

Cosmology and Nongalactic Astrophysics · Physics 2014-07-16 Naoyuki Takeda , Yuki Watanabe

Many new physics models predict resonances with masses in the TeV range which decay into a pair of top quarks. With its large cross section, t-bar t production at the Large Hadron Collider (LHC) offers an excellent opportunity to search for…

High Energy Physics - Phenomenology · Physics 2008-11-26 U. Baur , L. H. Orr

We reconsider the issue of large-volume compactifications of the heterotic string in light of the recent discoveries about strongly-coupled string theories. Our conclusion remains firmly negative with respect to classical compactifications…

High Energy Physics - Theory · Physics 2009-10-30 Elena Caceres , Vadim S. Kaplunovsky , I. Michael Mandelberg

We discuss the cosmology of string models with perturbative supersymmetry breaking at a scale of ${\cal O}$(TeV). Such models exhibit Kaluza-Klein like spectra and contain unstable massive gravitinos/gravitons. We find that considerations…

High Energy Physics - Phenomenology · Physics 2011-02-16 S. A. Abel , S. Sarkar

We consider the most general Kaluza-Klein (KK) compactification on $S^1/\mathbb{Z}_2$ of a five dimensional ($5D$) graviton-dilaton system, with a non-vanishing dilaton background varying linearly along the fifth dimension. We show that…

High Energy Physics - Theory · Physics 2021-09-30 Ignatios Antoniadis , Chrysoula Markou , François Rondeau

We study the evolution of gravitational waves(GWs) after inflation in a brane-world cosmology embedded in five-dimensional anti-de Sitter spacetime. Contrary to the standard four-dimensional results, the GWs at the high-energy regime in…

High Energy Physics - Theory · Physics 2015-06-26 Takashi Hiramatsu , Kazuya Koyama , Atsushi Taruya

The first inflationary model conceived was the one proposed by Starobinsky which includes an additional term quadratic in the Ricci-scalar R in the Einstein-Hilbert action. The model is now considered a target for several future cosmic…

Cosmology and Nongalactic Astrophysics · Physics 2021-01-27 S. Santos da Costa , M. Benetti , R. M. P. Neves , F. A. Brito , R. Silva , J. S. Alcaniz

Known mechanisms for breaking of supersymmetry at the level of string theory imply that at least one of the internal dimensions has a very large size. Experimental detection of the associated light Kaluza-Klein (KK) excitations would be a…

High Energy Physics - Theory · Physics 2008-02-03 Karim Benakli

Big Bang nucleosynthesis in the presence of decaying relic neutral particles is examined in detail. All non-thermal processes important for the determination of light-element abundance yields of 2H, 3H, 3He, 4He, 6Li, and 7Li are coupled to…

High Energy Physics - Phenomenology · Physics 2009-11-11 Karsten Jedamzik

Recent cosmic microwave background observations favor low energy scale inflationary models in a closed universe. However, onset of inflation in such models for a closed universe is known to be severely problematic. In particular, such a…

General Relativity and Quantum Cosmology · Physics 2021-03-03 Lucia Gordon , Bao-Fei Li , Parampreet Singh

We analyze observational constraints on the parameter space of tachyonic inflation with a Gaussian potential and discuss some predictions of this scenario. As was shown by Kofman and Linde, it is extremely problematic to achieve the…

High Energy Physics - Theory · Physics 2008-11-26 Joris Raeymaekers

The magnetic fluxbrane solution with a strongly warped throat is studied in the Type IIA supergravity theory with co-dimension one local source which surves as $Z_{2}$-symmetric UV boundary of the throat. Overall volume of extra space is…

High Energy Physics - Theory · Physics 2008-11-26 Boris L. Altshuler

The eta problem is one of the most significant obstacles to building a successful inflationary model in string theory. Planck mass suppressed corrections to the inflaton potential generally lead to inflaton masses of order the Hubble scale…

High Energy Physics - Theory · Physics 2010-01-15 Damien A. Easson , Ruth Gregory

We study the cosmological properties of a metastable de Sitter vacuum obtained recently in the framework of type IIB flux compactifications in the presence of three D7-brane stacks, based on perturbative quantum corrections at both…

High Energy Physics - Theory · Physics 2020-11-04 Ignatios Antoniadis , Osmin Lacombe , George K. Leontaris

We reevaluate the thermal relic density of the Kaluza-Klein (KK) dark matter in universal extra dimension models. In particular, we consider the effect of the resonance caused by second KK particles on the density. We find that the…

High Energy Physics - Phenomenology · Physics 2009-11-11 Mitsuru Kakizaki , Shigeki Matsumoto , Yoshio Sato , Masato Senami

A finite duration of cosmic inflation can result in features $\mathcal{P}_{\mathcal{R}}(k) = |\alpha_k-\beta_k\,\mathrm{e}^{\mathrm{i}\delta_k}|^2 \,\mathcal{P}_{\mathcal{R}}^{(0)}(k)$ in the primordial power spectrum that carry information…

General Relativity and Quantum Cosmology · Physics 2025-03-17 Eugenio Bianchi , Mauricio Gamonal