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String theory has been claimed to give rise to natural fuzzy dark matter candidates in the form of ultralight axions. In this paper we revisit this claim by a detailed study of how moduli stabilisation affects the masses and decay constants…

高能物理 - 理论 · 物理学 2022-06-01 Michele Cicoli , Veronica Guidetti , Nicole Righi , Alexander Westphal

We probe the stau-neutralino co-annihilation domain of the parameter space allowed by the current experimental bounds on the light Higgs mass, the b-> s \gamma decay, and the amount of neutralino cold dark matter within the framework of…

高能物理 - 唯象学 · 物理学 2008-11-26 Vadim Khotilovich , Richard Arnowitt , Bhaskar Dutta , Teruki Kamon

The EDGES Collaboration has recently reported the detection of a stronger-than-expected absorption feature in the global 21-cm spectrum, centered at a frequency corresponding to a redshift of z ~ 17. This observation has been interpreted as…

高能物理 - 唯象学 · 物理学 2018-07-11 Asher Berlin , Dan Hooper , Gordan Krnjaic , Samuel D. McDermott

We study a supersymmetric (SUSY) Standard Model in which a Higgsino is light enough to be dark matter, while the other SUSY particles are much heavier than the weak scale. We carefully treat the effects of heavy SUSY particles to the…

高能物理 - 唯象学 · 物理学 2015-02-03 Natsumi Nagata , Satoshi Shirai

We provide, in a framework of vector-like gauge theories, concrete models for conformal sequestering of dynamical supersymmetry (SUSY) breaking in the hidden sector. If the sequestering is sufficiently strong, anomaly mediation of the SUSY…

高能物理 - 唯象学 · 物理学 2009-11-11 M. Ibe , K. -I. Izawa , Yu Nakayama , Y. Shinbara , T. Yanagida

We examine supersymmetric models with mixed modulus-anomaly mediated SUSY breaking (MM-AMSB) soft terms which get comparable contributions to SUSY breaking from moduli-mediation and anomaly-mediation. The apparent (mirage) unification of…

高能物理 - 唯象学 · 物理学 2010-10-27 Howard Baer , Eun-Kyung Park , Xerxes Tata , Ting T. Wang

A generic lesson of string theory is that the coupling constants of an effective low energy theory are determined by the vacuum values of a set of fields - the so-called moduli - some of which are stabilized at relatively low masses by…

高能物理 - 理论 · 物理学 2008-11-26 S. P. de Alwis

Cosmologically long-lived, composite states arise as natural dark matter candidates in theories with a strongly interacting hidden sector at a scale of 10 - 100 TeV. Light axion-like states, with masses in the 1 MeV - 10 GeV range, are also…

高能物理 - 唯象学 · 物理学 2010-05-28 Jeremy Mardon , Yasunori Nomura , Jesse Thaler

The prediction for the Higgs mass in the dark matter selected high-scale SUSY is explored. We show the bounds on SUSY-breaking scale in models of SM $+\tilde{w}$ and SM $+\tilde{h}/\tilde{s}$ due to the observed Higgs mass at the LHC. We…

高能物理 - 唯象学 · 物理学 2015-03-13 Sibo Zheng

An electroweak (EW) sector of the Minimal Supersymmetric Standard Model (MSSM) with masses of a few hundred GeV can account for variety of experimental data, assuming the lightest neutralino to be the lightest supersymmetric (SUSY)…

高能物理 - 唯象学 · 物理学 2022-01-11 Manimala Chakraborti , Sven Heinemeyer , Ipsita Saha

The large value of the tensor-to-scalar ratio in the cosmic microwave background radiation reported by the BICEP2 collaboration gives strong impact on models of supersymmetry (SUSY). The large ratio indicates inflation with a high-energy…

高能物理 - 唯象学 · 物理学 2015-06-19 Keisuke Harigaya , Masahiro Ibe , Koji Ichikawa , Kunio Kaneta , Shigeki Matsumoto

We consider the axion-mediated scattering processes between dark matter (DM) and nucleus. Substantial contributions are made via the CP-odd gluonic current which induces the spin-dependent process. Since the QCD axion is too feebly coupled…

高能物理 - 唯象学 · 物理学 2024-08-07 Kyu Jung Bae , Jongkuk Kim

The model independent axion of string theory has a decay constant of order of the Planck scale. We explore the properties of this quintessence candidate (quintaxion) in the scheme of hidden sector supergravity breakdown. In models allowing…

高能物理 - 唯象学 · 物理学 2014-11-17 Jihn E. Kim , Hans Peter Nilles

The detection of the theoretically expected dark matter is central to particle physics and cosmology. Current fashionable supersymmetric models provide a natural dark matter candidate which is the lightest supersymmetric particle (LSP).…

高能物理 - 唯象学 · 物理学 2007-05-23 J. D. Vergados , M. E. Gomez

A renormalizable UV model for Axion-Like Particles (ALPs) or hidden photons, that may explain the dark matter usually involves a dark Higgs field which is a singlet under the standard model (SM) gauge group. The dark sector can couple to…

高能物理 - 唯象学 · 物理学 2024-05-30 Gholamhossein Haghighat , Mojtaba Mohammadi Najafabadi , Kodai Sakurai , Wen Yin

In N=1 supergravity the tree-level scalar potential of the hidden sector may have a minimum with broken local supersymmetry (SUSY) as well as a supersymmetric Minkowski vacuum. These vacua can be degenerate, allowing for a consistent…

高能物理 - 唯象学 · 物理学 2017-08-02 C. D. Froggatt , H. B. Nielsen , R. Nevzorov , A. W. Thomas

Within a multicomponent dark matter scenario, novel gamma-ray signals may arise from the decay of the heavier dark matter component into the lighter. For a scalar dark sector of this kind, the decay $\phi_2\rightarrow\phi_1 \gamma$ is…

高能物理 - 唯象学 · 物理学 2020-01-06 Avirup Ghosh , Alejandro Ibarra , Tanmoy Mondal , Biswarup Mukhopadhyaya

We study gauge theories where quasi-hidden sectors are added to the MSSM for the sake of string consistency conditions which would otherwise not be satisfied. We focus on quiver gauge theories motivated by weakly coupled type II orientifold…

高能物理 - 唯象学 · 物理学 2015-06-11 Mirjam Cvetič , James Halverson , Hernan Piragua

We investigate the phenomenological consequences of string models wherein the MSSM resides on a D-brane, and the hypercharge gaugino mass is generated in a geometrically separated hidden sector. This hypercharged anomaly-mediated SUSY…

高能物理 - 唯象学 · 物理学 2009-11-13 Howard Baer , Radovan Dermisek , Shibi Rajagopalan , Heaya Summy

Light Axionic Dark Matter, motivated by string theory, is increasingly favored for the "no-WIMP era". Galaxy formation is suppressed below a Jeans scale, of $\simeq 10^8 M_\odot$ by setting the axion mass to, $m_B \sim 10^{-22}$eV, and the…

宇宙学与河外天体物理 · 物理学 2017-12-01 Ivan De Martino , Tom Broadhurst , S. -H. Henry Tye , Tzihong Chiueh , Hsi-Yu Schive , Ruth Lazkoz