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We study the effect of the chiral symmetry restoration (CSR) on heavy-ion collisions observables in the energy range $\sqrt{s_{NN}}$=3-20 GeV within the Parton-Hadron-String Dynamics (PHSD) transport approach. The PHSD includes the…

Nuclear Theory · Physics 2016-11-01 A. Palmese , W. Cassing , E. Seifert , T. Steinert , P. Moreau , E. L. Bratkovskaya

The Large Hadron Collider (LHC) at CERN is a 7 TeV proton synchrotron, with a design stored energy of 362 MJ per beam. The high-luminosity (HL-LHC) upgrade will increase this to 675 MJ per beam. In order to protect the superconducting…

We present theory for coherent effects observed in crystal collimation experiments that is in good quantitative agreement with RHIC and Tevatron data. We show that coherent scattering in a bent crystal strongly amplifies beam diffusion,…

Accelerator Physics · Physics 2008-11-26 V. M. Biryukov

The generation of the ultra-bright beams required by modern accelerators and drivers of free-electron lasers (FELs) has generally relied on chicane-based bunch compressions that often result in the microbunching instability. Following…

Accelerator Physics · Physics 2014-09-09 Alex H. Lumpkin

This paper presents simulations of the synchrotron self-Compton (SSC) spectrum within the Internal-Collision-induced Magnetic Reconnection and Turbulence (ICMART) model. We investigate how key parameters like the magnetization $\sigma_0$…

High Energy Astrophysical Phenomena · Physics 2026-02-16 Xueying Shao , He Gao

Accretion-powered X-ray pulsars exhibit significant variability of the Cyclotron Resonance Scattering Feature (CRSF) centroid energy on pulse-to-pulse timescales, and also on much longer timescales. Two types of spectral variability are…

High Energy Astrophysical Phenomena · Physics 2015-06-05 P. A. Becker , D. Klochkov , G. Schonherr , O. Nishimura , C. Ferrigno , I. Caballero , P. Kretschmar , M. T. Wolff , J. Wilms , R. Staubert

The A0 Photoinjector at Fermilab can produce high charge (10-14 nC) electron bunches of low emittance (20 pi mm-mrad for 12 nC). We have undertaken a study of the optimal compression conditions. Off-crest acceleration in the 9-cell capture…

Accelerator Physics · Physics 2007-05-23 M. J. Fitch , A. C. Melissinos , N. Barov , J. -P. Carneiro , H. T. Edwards , W. H. Hartung

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

Physics of charmonium suppression in nuclear collisions drastically changes between the energies of SPS and RHIC. Mechanisms suppressing charmonia at SPS are reviewed, neither of which is important at RHIC. On the other hand, coherence, or…

High Energy Physics - Phenomenology · Physics 2009-11-07 B. Z. Kopeliovich

In this paper we study the semileptonic decays of the $B_c$ meson in the Light-Cone Sum Rule (LCSR) approach. The result for each channel depends on the corresponding distribution amplitude of the final meson. For the case of $B_c$ decaying…

High Energy Physics - Phenomenology · Physics 2008-11-26 Tao Huang , Fen Zuo

Cyclotron Radiation Emission Spectroscopy (CRES) is an approach to measuring the energy of an electron trapped in an externally applied magnetic field. The bare electron can come from different interactions, including photoelectric…

Atomic Physics · Physics 2020-08-12 Kareem Kazkaz , Nathan Woollett

We demonstrate the DC-Kerr effect in PECVD Silicon-rich Nitride (SRN) and use it to demonstrate a third order nonlinear susceptibility, \c{hi}^((3)), as high as (6 +/- 0.58)x10-19 m2/v2. We employ spectral shift versus applied voltage…

Optics · Physics 2021-09-08 Alex Friedman , Hani Nejadriahi , Rajat Sharma , Yeshaiahu Fainman

We investigate binary mergers of galaxy clusters, the formation of shocks, and the resulting radio relics using three-dimensional simulations. The initial setup consists of two idealized spherical subclusters with a mass ratio below three,…

High Energy Astrophysical Phenomena · Physics 2026-05-27 Hyesung Kang , Dongsu Ryu , Jeongbhin Seo

Cosmic rays (CRs) may drive outflows and alter the phase structure of the circumgalactic medium, with potentially important implications on galaxy formation. However, these effects ultimately depend on the dominant mode of transport of CRs…

A design for a compact x-ray light source (CXLS) with flux and brilliance orders of magnitude beyond existing laboratory scale sources is presented. The source is based on inverse Compton scattering of a high brightness electron bunch on a…

Optimum suppression of higher order modes in single-ring hollow-core photonic crystal fibers (SR-PCFs) occurs when the capillary-to-core diameter ratio d/D = 0.68. Here we report that, in SR-PCFs with sub-optimal values of d/D, higher-order…

It is known that the alignment of an high-energy e- beam with specific crystal directions leads to a significant increase of the coherent radiation emission. This enhancement can be exploited to create an intense photon source. An elective…

We discuss the new data for the production of the $\psi'$ meson in pA collisions at 450 GeV at CERN-SPS (of the NA50-collaboration) [1]. We extract from the CERN data $\sigma(\psi' N)\approx 8$ mb under the assumption that the $\psi'$ is…

Nuclear Theory · Physics 2009-11-10 L. Gerland , L. Frankfurt , M. Strikman , H. Stocker

We study on-shell decays of light vector meson resonances $\rho$, $K^*$ and $\phi$ in the framework of chiral constituent quark model using resummation calculations. Such studies are necessary for showing that chiral dynamics works well at…

High Energy Physics - Phenomenology · Physics 2014-11-17 Yi-Bin Huang , Xiao-Jun Wang , Mu-Lin Yan

We present a quantitative analysis of the time-delay effect on the cosmic background radiation (CBR) by static gravitational potential of galaxy clusters. This is primarily motivated by growing observational evidence that clusters have…

Astrophysics · Physics 2009-10-31 Da-Ming Chen , Xiang-Ping Wu , Dong-Rong Jiang
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