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A solid target in contact with a plasma charges (negatively) to reflect the more mobile species (electrons) and thus keep the bulk plasma quasineutral. To shield the bulk plasma from the charged target, there is an oppositely (positively)…

Plasma Physics · Physics 2025-01-20 Alessandro Geraldini , Stephan Brunner , Felix I. Parra

We present a new perspective on the symmetries that govern the formation of large-scale structures across the Universe, particularly focusing on the transition from the seeds of galaxy clusters to the seeds of galaxies themselves. We…

Cosmology and Nongalactic Astrophysics · Physics 2024-03-28 Giovanni Montani , Nakia Carlevaro

We investigate phantom cosmology in which the scale factor is a power law, and we use cosmological observations from Cosmic Microwave Background (CMB), Baryon Acoustic Oscillations (BAO) and observational Hubble data, in order to impose…

Cosmology and Nongalactic Astrophysics · Physics 2011-11-28 Chakkrit Kaeonikhom , Burin Gumjudpai , Emmanuel N. Saridakis

The nature of dark matter sets the timeline for the formation of first collapsed halos and thus affects the sources of reionization. Here, we consider two different models of dark matter: cold dark matter (CDM) and thermal warm dark matter…

Cosmology and Nongalactic Astrophysics · Physics 2020-08-31 Anchal Saxena , Suman Majumdar , Mohd Kamran , Matteo Viel

Laser light incident on targets at intensities such that the electron dynamics is ultrarelativistic gives rise to a harmonic power spectrum extending to high orders and characterized by a relatively slow decay with the harmonic number m…

Plasma Physics · Physics 2008-10-06 T. J. M. Boyd , R. Ondarza-Rovira

The conventional cold, particle interpretation of dark matter (CDM) still lacks laboratory support and struggles with the basic properties of common dwarf galaxies, which have surprisingly uniform central masses and shallow density…

Astrophysics of Galaxies · Physics 2014-06-26 Hsi-Yu Schive , Tzihong Chiueh , Tom Broadhurst

With recent Lyman-alpha forest data from BOSS and XQ-100, some studies suggested that the lower mass limit on the fuzzy dark matter (FDM) particles is lifted up to $10^{-21}\,\mathrm{eV}$. However, such a limit was obtained by $\Lambda$CDM…

Cosmology and Nongalactic Astrophysics · Physics 2018-08-14 Jiajun Zhang , Jui-Lin Kuo , Hantao Liu , Yue-Lin Sming Tsai , Kingman Cheung , Ming-Chung Chu

We have recently proposed a mechanism of photon-axion oscillations as a way of rendering supernovae dimmer without cosmic acceleration. Subsequently, it has been argued that the intergalactic plasma may interfere adversely with this…

High Energy Physics - Phenomenology · Physics 2009-09-17 Csaba Csaki , Nemanja Kaloper , John Terning

Thermal freeze-out is a prominent example of dark matter (DM) production mechanism in the early Universe that can yield the correct relic density of stable weakly interacting massive particles (WIMPs). At the other end of the mass scale,…

High Energy Physics - Phenomenology · Physics 2020-08-05 Sebastian Trojanowski , Philippe Brax , Carsten van de Bruck

We estimate the survival probability of $J/{\psi}$ in relativistic heavy-ion collisions, using both short-distance QCD and nuclear absorption mechanism. The suppression is found to be almost 100 percent for a thermally equilibrating…

High Energy Physics - Phenomenology · Physics 2014-11-17 Gouranga C Nayak

We explore the impacts of ultraviolet (UV) radiation feedback on galaxies during the epoch of reionisation by cosmological simulations in which hydrodynamics and the transfer of the H and He ionising photons are consistently coupled.…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Kenji Hasegawa , Benoit Semelin

The post-recombination streaming of baryons through dark matter keeps baryons out of low mass (<10^6 solar masses) halos coherently on scales of a few comoving Mpc. It has been argued that this will have a large impact on the 21-cm signal…

Cosmology and Nongalactic Astrophysics · Physics 2011-10-24 Jonathan M. Bittner , Abraham Loeb

One widely discussed mechanism to produce highly coherent radio emission of fast radio bursts (FRBs) is coherent emission by bunches, either via curvature radiation or inverse Compton scattering (ICS). It has been suggested that the plasma…

High Energy Astrophysical Phenomena · Physics 2022-11-09 Yuanhong Qu , Bing Zhang , Pawan Kumar

Contrarily to general believe, a first-order cosmological perturbation theory based on Einstein's General Theory of Relativity explains the formation of massive primeval stars in a flat Friedmann-Lemaitre-Robertson-Walker universe after…

General Relativity and Quantum Cosmology · Physics 2010-09-21 P. G. Miedema

Conventional wisdom was that thermal relics from the epoch of reionization (EOR) would vanish swiftly. Recently, however, it was shown that these relics can survive to lower redshifts ($z \sim 2$) than previously thought, due to gas at mean…

Cosmology and Nongalactic Astrophysics · Physics 2021-02-05 Paulo Montero-Camacho , Yi Mao

This conference proceedings paper provides a short summary of the constraints presented in Menci et al. 2016, 2017 on the mass of thermal WDM candidates, and of the results presented in Romanello et al. 2021 on how Reionization scenarios…

Cosmology and Nongalactic Astrophysics · Physics 2023-01-11 Marco Castellano , Nicola Menci , Massimiliano Romanello

We present a general description of the scalar field dark matter (SFDM) hypothesis in the cosmological context. The scenario of structure formation under such a hypothesis is based on Jeans instabilities of fluctuations of the scalar field.…

We consider the $J/\Psi$ suppression at a high energy heavy ion collision. An ideal gas of massive hadrons in thermal and chemical equilibrium is formed in the central region. The finite-size gas expands longitudinally in accordance with…

High Energy Physics - Phenomenology · Physics 2009-10-31 Dariusz Prorok , Ludwik Turko

Recent analysis of the Milky Way's satellite galaxies reveals that these objects share a common central mass density, even though their luminosities range over five orders of magnitude. This observation can be understood in the context of…

Astrophysics of Galaxies · Physics 2015-05-14 Martin Stringer , Shaun Cole , Carlos Frenk

Complimenting recent work on the effective field theory of cosmological large scale structures, here we present detailed approximate analytical results and further pedagogical understanding of the method. We start from the collisionless…

Cosmology and Nongalactic Astrophysics · Physics 2014-04-02 Mark P. Hertzberg
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