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Dark matter (DM) as a thermal relic of the primordial plasma is increasingly pressured by direct and indirect searches, while the same production mechanism in a decoupled sector is much less constrained. We extend the standard treatment of…

高能物理 - 唯象学 · 物理学 2021-05-19 Torsten Bringmann , Paul Frederik Depta , Marco Hufnagel , Kai Schmidt-Hoberg

In this work, we investigate a scenario in which heavy Majorana Right-Handed Neutrinos (RHNs) are in thermal equilibrium with a dark sector with temperature higher than the Standard Model (SM) thermal bath. Specifically, we consider the…

高能物理 - 唯象学 · 物理学 2018-04-03 Nicolás Bernal , Chee Sheng Fong

We have calculated the leading-twist next-to-leading order (NLO), i.e., O(alpha_s), correction to the light-cone sum-rules prediction for the electromagnetic form factors of the nucleon. We have used the Ioffe nucleon interpolation current…

高能物理 - 唯象学 · 物理学 2009-02-19 K. Passek-Kumericki , G. Peters

The production of two-jet final states in deep inelastic scattering is an important QCD precision observable. We compute it for the first time to next-to-next-to-leading order (NNLO) in perturbative QCD. Our calculation is fully…

高能物理 - 唯象学 · 物理学 2016-07-27 James Currie , Thomas Gehrmann , Jan Niehues

We present the first systematic derivation of the one-loop correction to the large scale matter power spectrum in a mixed cold+hot dark matter cosmology with subdominant massive neutrino hot dark matter. Starting with the equations of…

天体物理学 · 物理学 2009-11-19 Yvonne Y. Y. Wong

Evaluating the relic density of dark matter is an interesting possibility to constrain the parameter space of new physics models. However, this calculation is affected by several sources of uncertainty. On the particle physics side,…

高能物理 - 唯象学 · 物理学 2010-12-01 Björn Herrmann

We examine a scenario for freeze-in production of dark matter, which occurs due to the large thermal correction to the mass of a decaying mediator particle present in the thermal bath of the early Universe. We show that the decays, which…

高能物理 - 唯象学 · 物理学 2022-03-14 Partha Konar , Rishav Roshan , Sudipta Show

We investigate the relic density n_\chi of non-relativistic long-lived or stable particles \chi in non-standard cosmological scenarios. We calculate the relic abundance starting from arbitrary initial temperatures of the radiation-dominated…

高能物理 - 唯象学 · 物理学 2008-11-26 Manuel Drees , Hoernisa Iminniyaz , Mitsuru Kakizaki

We discuss different aspects which could influence temperatures deduced from experimental isotopic yields in the multifragmentation process. It is shown that fluctuations due to the finite size of the system and distortions due to the decay…

核理论 · 物理学 2011-07-19 S. R. Souza , W. P. Tan , R. Donangelo , C. K. Gelbke , W. G. Lynch , M. B. Tsang

The complete next-to-next-to-leading order (i.e. $O(v^2)$, $O(v \alpha_s)$ and $O(\alpha_s^2)$) relativistic corrections to the total photon mediated $t\bar t$ production cross section at threshold are presented in the framework of…

高能物理 - 唯象学 · 物理学 2016-08-25 A. H. Hoang , T. Teubner

Thermal freeze-out offers an attractive explanation of the dark matter density free from fine-tuning of initial conditions. For dark matter with a mass below tens of MeV, photons, electrons, and neutrinos are the only available direct…

高能物理 - 唯象学 · 物理学 2024-05-10 Xiaoyong Chu , Josef Pradler

Freeze-in of multi-component dark sectors is governed not only by the interaction with the thermal plasma, but also by their internal dynamics. Full thermalisation within the dark sector is not guaranteed, raising the question of impact of…

高能物理 - 唯象学 · 物理学 2026-04-17 Shiuli Chatterjee , Andrzej Hryczuk

Next-to-leading order QCD corrections to the $\gamma^{*} \longrightarrow Q\bar{Q}-Reggeon$ vertex are calculated, where $Q\bar{Q}$ denotes a heavy quark pair $c\bar c$ or $b\bar b$. The heavy quark mass effects on the photon impact factor…

高能物理 - 唯象学 · 物理学 2022-09-14 Li Ping Sun , Long Bin Chen , Cong Feng Qiao , Kuang Ta Chao

Thermal corrections, including relativistic effects, for the positronium atom are discussed. The theoretical description of thermal corrections is carried out within the framework of relativistic quantum electrodynamics. As a result,…

原子物理 · 物理学 2022-03-14 D. Solovyev , T. Zalialiutdinov , A. Anikin

We calculate the second order corrections to vacuum polarization tensor of photons at low temperatures, i.e; T $\le 10^{10}$ K ($T << m_e$). The thermal contributions to the QED coupling constant are evaluated at temperatures below the…

高能物理 - 唯象学 · 物理学 2009-09-29 Samina S. Masood , Mahnaz Q. Haseeb

For processes involving structure functions and/or fragmentation functions, arguments that, over a range of a proper kinematic variable, there is a part that dominates the next-to-leading order (NLO) corrections are briefly reviewed. The…

高能物理 - 唯象学 · 物理学 2009-11-07 A. P. Contogouris , Z. Merebashvili

After a period of inflationary expansion, the Universe reheated and reached full thermal equilibrium at the reheating temperature T_R. In this work we point out that, in the context of effective low-energy supersymmetric models, LHC…

高能物理 - 唯象学 · 物理学 2008-11-26 Ki-Young Choi , Leszek Roszkowski , Roberto Ruiz de Austri

We investigate whether the late-time (at $z\leq 100$) velocity dispersion expected in Warm Dark Matter scenarios could have some effect on the cosmic web (i.e., outside of virialized halos). We consider effective hydrodynamical equations,…

宇宙学与河外天体物理 · 物理学 2013-05-30 Patrick Valageas

We investigate a new bound on the low reheating temperature in a scenario where the Universe experiences early matter-domination before reheating after which the standard big bang cosmology begins. In many models of dark matter (DM), the…

宇宙学与河外天体物理 · 物理学 2017-08-30 Ki-Young Choi , Tomo Takahashi

We present the complete next-to-leading order (NLO) QCD corrections to the top quark associated with $\gamma$ production induced by model-independent $tq\gamma$ and $tqg$ flavor-changing neutral-current (FCNC) couplings at hadron colliders,…

高能物理 - 唯象学 · 物理学 2015-03-18 Yue Zhang , Bo Hua Li , Chong Sheng Li , Jun Gao , Hua Xing Zhu
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