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We briefly discuss the status of double parton scattering (DPS) on both theoretical and experimental sides and summarize the state of the naive DPS model, where the scatterers are taken completely independent. We then elaborate on some of…

High Energy Physics - Phenomenology · Physics 2015-08-12 Tomas Kasemets

Models where Dark Matter and Dark Energy interact with each other have been proposed to solve the coincidence problem. We review the motivations underlying the need to introduce such interaction, its influence on the background dynamics and…

Cosmology and Nongalactic Astrophysics · Physics 2016-08-24 B. Wang , E. Abdalla , F. Atrio-Barandela , D. Pavon

We argue that dark matter particles which have strong interactions with the Standard Model particles are not excluded by current astrophysical constraints. These dark matter particles have unique signatures at colliders; instead of missing…

High Energy Physics - Phenomenology · Physics 2011-09-29 Yang Bai , Arvind Rajaraman

We investigate cosmological implications of an energy density contribution arising by elastic dark matter self-interactions. Its scaling behaviour shows that it can be the dominant energy contribution in the early universe. Constraints from…

Cosmology and Nongalactic Astrophysics · Physics 2011-04-06 Rainer Stiele , Tillmann Boeckel , Jurgen Schaffner-Bielich

Polarization of both electron and positron beams at a future linear collider (LC) allows for the measurement of transverse polarization asymmetries. These asymmetries have been shown to be particularly sensitive to graviton or other spin-2,…

High Energy Physics - Phenomenology · Physics 2009-11-10 Thomas G. Rizzo

In Phys. Rev. D 98, 103023 (2018), a novel scenario was proposed to probe the interactions between dark matter (DM) particles and electrons, via hydrogen-atmosphere pulsating white dwarfs (DAVs) in globular clusters. The estimation showed…

High Energy Physics - Phenomenology · Physics 2020-01-01 Jia-Shu Niu , Hui-Fang Xue

Heavy objects like the W, Z and t are short-lived compared with typical hadronization times. When pairs of such particles are produced, the subsequent hadronic decay systems may therefore become interconnected. We study such potential…

High Energy Physics - Phenomenology · Physics 2011-02-15 Valery A. Khoze , Torbjörn Sjöstrand

The freeze-in mechanism describes the out-of-equilibrium production of dark matter (DM) particles via feeble couplings or non-renormalisable interactions with large suppression scales. In the latter case, predictions suffer from a strong…

High Energy Physics - Phenomenology · Physics 2025-04-16 Cristina Benso , Felix Kahlhoefer , Henda Mansour

The neutron star properties are generally determined by the equation of state of $\beta$-equilibrated dense matter. In this work, we consider the interaction of fermionic dark matter (DM) particles with the nucleons via Higgs exchange and…

High Energy Astrophysical Phenomena · Physics 2022-01-19 H. C. Das , Ankit Kumar , Bharat Kumar , S. K. Patra

While the paradigm of a weakly interacting massive particle (WIMP) has guided our search strategies for dark matter in the past decades, their null-results have stimulated growing interest in alternative explanations pointing towards…

High Energy Physics - Phenomenology · Physics 2018-05-22 Jan Heisig

Despite significant experimental sensitivity to point-like, weakly interacting particles at the electroweak mass scale, dark matter has not been found yet. This could hint at a more complex dark sector with multiple states or composite dark…

High Energy Physics - Phenomenology · Physics 2023-01-02 Juri Smirnov

Interactions between dark matter (DM) and radiation (photons or neutrinos) in the early Universe suppress density fluctuations on small mass scales. Here we perform a thorough analysis of structure formation in the fully non-linear regime…

Cosmology and Nongalactic Astrophysics · Physics 2015-04-14 J. A. Schewtschenko , R. J. Wilkinson , C. M. Baugh , C. Boehm , S. Pascoli

Mutual Coulomb interactions between electrons lead to a plethora of interesting physical and chemical effects, especially if those interactions involve many fluctuating electrons over large spatial scales. Here, we identify and study in…

I analyze $D$-$\ol D$ mixing using the techniques of heavy quark effect field theory. The analysis suggests that the there may be important cancellations among the dispersive effects of different kinds of final states, so that the total…

High Energy Physics - Phenomenology · Physics 2009-09-11 Howard Georgi

We explore the use of polarized $e^+/e^-$ beams and/or the information on final state decay lepton polarizations in probing the interaction of the Higgs boson with a pair of vector bosons. A model independent analysis of the process $e^+…

High Energy Physics - Phenomenology · Physics 2009-11-13 Sudhansu S. Biswal , Debajyoti Choudhury , Rohini M. Godbole , Mamta

In this paper we investigate the interaction between dark matter and dark energy by considering two different interacting scenarios, i.e. the cases of constant interaction function and variable interaction function. By fitting the current…

Cosmology and Nongalactic Astrophysics · Physics 2012-03-23 Jianbo Lu , Yabo Wu , Yongyi Jin , Yan Wang

The experimental results on some centrality depending characteristics of hadron-nuclear and nuclear-nuclear interactions at high energies demonstrate the regime changes. Appearance of strong interaction matter's mixed states is considered…

High Energy Physics - Experiment · Physics 2015-06-25 M. K. Suleymanov , O. B. Abdinnov , N. S. Angelov , B. Z. Belashev , Ya. G. Guseynaliyev , A. A. Kuznetchov , A. S. Vodopianov

We study the freeze-in of gravitationally interacting dark matter in extra dimensions. Focusing on a minimal dark matter candidate that only interacts with the SM via gravity in a five-dimensional model we find that a large range of dark…

High Energy Physics - Phenomenology · Physics 2023-04-26 Arturo de Giorgi , Stefan Vogl

The decay and annihilation cross sections of dark matter particles may depend on the value of a chameleonic scalar field that both evolves cosmologically and takes different values depending on the local matter density. This possibility…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-20 Kimberly K. Boddy , Sean M. Carroll , Mark Trodden

Many popular models of new physics beyond the Standard Model use a parity to stabilize weakly interacting, dark matter candidates. We examine the potential for the CERN Large Hadron Collider to distinguish models with parity stabilized dark…

High Energy Physics - Phenomenology · Physics 2009-07-29 Devin G. E. Walker
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