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We compute the cosmological background radiation of gamma rays and neutrinos due to neutralino annihilation in evolving dark matter halos, assuming the observed dark matter is comprised of thermally excited neutralinos in the MSSM. The…

Astrophysics · Physics 2014-10-13 Dominik Elsaesser , Karl Mannheim

Global topological defects produce nonzero stress-energy throughout spacetime, and as a result can have observable gravitational influence on surrounding matter. Gravitational effects of global strings are used to place bounds on their…

General Relativity and Quantum Cosmology · Physics 2009-10-30 Shane L. Larson , William A. Hiscock

We use string duality to describe instanton induced spontaneous supersymmetry breaking in string compactifications with additional background fields. Dynamical supersymmetry breaking by space-time instantons in the heterotic string theory…

High Energy Physics - Theory · Physics 2014-11-18 P. Mayr

Supermassive black hole binaries source gravitational waves measured by Pulsar Timing Arrays. The frequency spectrum of this stochastic background is predicted more precisely than its amplitude. We argue that Dark Matter friction can…

Cosmology and Nongalactic Astrophysics · Physics 2023-07-04 Anish Ghoshal , Alessandro Strumia

In this mini-review, we summarize a variety of findings pertaining to consequences of the landscape of string theory for supersymmetry (SUSY) phenomenology. The idea is to adopt the MSSM as the most parsimonious 4-d low energy EFT after…

High Energy Physics - Phenomenology · Physics 2022-03-01 Howard Baer , Vernon Barger , Shadman Salam , Dibyashree Sengupta

Superheavy dark matter (SHDM) exchanges energy with its environment much slower than particles with masses close to the electroweak (EW) scale and has therefore different small-scale clustering properties. Using the neutralino as candidate…

Astrophysics of Galaxies · Physics 2010-10-06 V. Berezinsky , V. Dokuchaev , Yu. Eroshenko , M. Kachelriess , M. Aa. Solberg

If supersymmetry turns out to be a symmetry of nature at low energies, the first order of business to measure the soft breaking parameters. But one will also want to understand the symmetry, and its breaking, more microscopically. Two…

High Energy Physics - Theory · Physics 2017-08-23 Michael Dine

We study the phenomenology of a recent string construction with a quantum mechanically stable dark energy. A mild supersymmetry protects the vacuum energy but also allows $O(10 - 100)$ TeV scale superpartner masses. The construction is…

High Energy Physics - Theory · Physics 2020-01-08 Jonathan J. Heckman , Craig Lawrie , Ling Lin , Jeremy Sakstein , Gianluca Zoccarato

We explore multi-component dark matter models where the dark sector consists of multiple stable states with different mass scales, and dark forces coupling these states further enrich the dynamics. The multi-component nature of the dark…

High Energy Physics - Phenomenology · Physics 2009-06-30 Kathryn M. Zurek

We study the formation and properties of dark neutron stars in a scenario where dark matter is made up of (heavy) dark baryons in a sequestered copy of the MSSM. This scenario naturally explains the coincidence of baryonic and dark matter…

High Energy Physics - Phenomenology · Physics 2025-11-05 Jacob A. Litterer , João G. Rosa

We survey the low-energy supersymmetry phenomenology of a three-family Pati-Salam model constructed from intersecting D6-branes in Type IIA string theory on the T^6/(Z_2 x Z_2) orientifold which possesses many of the phenomenological…

High Energy Physics - Phenomenology · Physics 2010-01-12 James A. Maxin , Van E. Mayes , D. V. Nanopoulos

Under the hypothesis of a Dark Matter composed by supersymmetric particles like neutralinos, we investigate the possibility that their annihilation in the haloes of nearby galaxies could produce detectable fluxes of $\gamma$-photons.…

Astrophysics · Physics 2009-11-10 Lidia Pieri , Enzo Branchini

Dark matter can be captured by celestial objects and accumulate at their centers, forming a core of dark matter that can collapse to a small black hole, provided that the annihilation rate is small or zero. If the nascent black hole is big…

High Energy Physics - Phenomenology · Physics 2021-05-13 Javier F. Acevedo , Joseph Bramante , Alan Goodman , Joachim Kopp , Toby Opferkuch

The fragmentation of horizon crossing superstrings creates loops that accrete and bind to collapsing matter perturbations if the string tension is less than a critical value and if the loops are large-scale. For typical model parameters…

Cosmology and Nongalactic Astrophysics · Physics 2009-09-01 David F. Chernoff

We investigate the possibility that the galactic dark matter exists in an scenario where the phantom field is responsible for the dark energy. We obtain the statically and spherically approximate solution for this kind of the galaxy system…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-20 Ming-Hsun Li , Kwei-Chou Yang

Decaying or annihilating dark matter particles could be detected through gamma-ray emission from the species they decay or annihilate into. This is usually done by modelling the flux from specific dark matter-rich objects such as the Milky…

Cosmology and Nongalactic Astrophysics · Physics 2022-12-01 Deaglan J. Bartlett , Andrija Kostić , Harry Desmond , Jens Jasche , Guilhem Lavaux

Primordial micro black holes can constitute dark matter if short-distance gravity is modified by extra dimensions or a large number of species and if the memory-burden effect sufficiently suppresses Hawking evaporation. The resulting black…

High Energy Physics - Phenomenology · Physics 2026-03-18 Manuel Ettengruber , Florian Kühnel

The instability of dark matter may produce visible signals in the spectrum of cosmic gamma-rays. We consider this possibility in frameworks with additional spatial dimensions and supersymmetry. Examples of particles include…

Astrophysics · Physics 2011-11-10 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari

The cold dark matter may be in a meta-stable state and decays to other particles with a very long lifetime. If the decaying products of the dark matter are weakly interacting, e.g. neutrinos, then it would have little impact on…

Astrophysics · Physics 2008-11-26 Yan Gong , Xuelei Chen

We show how to make a topological string theory starting from an $N=4$ superconformal theory. The critical dimension for this theory is $\hat c= 2$ ($c=6$). It is shown that superstrings (in both the RNS and GS formulations) and critical…

High Energy Physics - Theory · Physics 2009-10-28 Nathan Berkovits , Cumrun Vafa
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