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We study the compression driven magnetic reconnection in the relativistic electron-positron plasma. Making use of a 2.5D particle-in-cell code, we simulated compression of a magnetized plasma layer containing a current sheet within it. We…

Astrophysics · Physics 2009-11-13 Yuri Lyubarsky , Michael Liverts

This article gives an overview of recent highlights from experimental measurements of heavy-ion collisions at ultra-relativistic energies: Measurements of electroweak probes constrain both the initial collision geometry and the nuclear…

Nuclear Experiment · Physics 2020-12-17 Yvonne Pachmayer

We study how a high-speed solar wind stream embedded in a slow solar wind influences the spread of solar energetic protons in interplanetary space. To model the energetic protons, we used a recently developed particle transport code that…

Space Physics · Physics 2019-04-10 Nicolas Wijsen , Angels Aran , Jens Pomoell , Stefaan Poedts

We report on the first measurement of angular correlations between high-energy pions and slow protons in electron-nucleus ($eA$) scattering, providing a new probe of how a nucleus responds to a fast-moving quark. The experiment employed the…

Nuclear Experiment · Physics 2026-02-06 S. J. Paul , M. Arratia , H. Hakobyan , W. Brooks , A. Acar , P. Achenbach , J. S. Alvarado , W. R. Armstrong , N. A. Baltzell , L. Barion , M. Bashkanov , M. Battaglieri , F. Benmokhtar , A. Bianconi , A. S. Biselli , F. Bossù , S. Boiarinov , K. -T. Brinkmann , W. J. Briscoe , V. Burkert , T. Cao , D. S. Carman , P. Chatagnon , H. Chinchay , G. Ciullo , P. L. Cole , A. D'Angelo , N. Dashyan , R. De Vita , A. Deur , S. Diehl , C. Djalali , R. Dupre , H. Egiyan , A. El Alaoui , L. Elouadrhiri , P. Eugenio , M. Farooq , S. Fegan , A. Filippi , C. Fogler , G. Gavalian , G. P. Gilfoyle , R. W. Gothe , B. Gualtieri , M. Hattawy , F. Hauenstein , T. B. Hayward , M. Hoballah , M. Holtrop , Yu-Chun Hung , Y. Ilieva , D. G. Ireland , E. L. Isupov , D. Jenkins , H. S. Jo , D. Keller , M. Khandaker , A. Kim , V. Klimenko , I. Korover , A. Kripko , V. Kubarovsky , L. Lanza , S. Lee , P. Lenisa , X. Li , D. Marchand , V. Mascagna , B. McKinnon , T. Mineeva , V. Mokeev , E. F. Molina Cardenas , C. Munoz Camacho , P. Nadel-Turonski , T. Nagorna , K. Neupane , S. Niccolai , G. Niculescu , M. Osipenko , A. I. Ostrovidov , M. Ouillon , P. Pandey , M. Paolone , L. L. Pappalardo , R. Paremuzyan , E. Pasyuk , C. Paudel , W. Phelps , N. Pilleux , P. S. H. Vaishnavi , S. Polcher Rafael , L. Polizzi , J. W. Price , Y. Prok , A. Radic , T. Reed , J. Richards , M. Ripani , J. Ritman , G. Rosner , S. Schadmand , A. Schmidt , R. A. Schumacher , Y. Sharabian , S. Shrestha , E. Sidoretti , D. Sokhan , N. Sparveris , M. Spreafico , S. Stepanyan , I. I. Strakovsky , S. Strauch , M. Tenorio , F. Touchte Codjo , R. Tyson , M. Ungaro , S. Vallarino , C. Velasquez , L. Venturelli , H. Voskanyan , E. Voutier , Y. Wang , D. P. Watts , U. Weerasinghe , X. Wei , M. H. Wood , L. Xu , Z. Xu , M. Zurek

We study the suppression of high-pT hadron spectra in nuclear collisions, supplementing the perturbative QCD factorized formalism with radiative parton energy loss. We find that the nuclear modification factor which quantifies the degree of…

High Energy Physics - Phenomenology · Physics 2008-11-26 K. J. Eskola , H. Honkanen , C. A. Salgado , U. A. Wiedemann

High-energy particles may be accelerated widely in stellar coronae; probably by the same processes we find in the Sun. Here, we have learned of two physical mechanisms that dominate the acceleration of solar energetic particles (SEPs). The…

Solar and Stellar Astrophysics · Physics 2025-03-20 Donald V. Reames

The solar wind undergoes non-adiabatic heating as it travels away from the Sun. The velocity phase space distribution of non-equilibrium ions in the solar wind indicate a source of free energy that could contribute significantly to this…

Dense high-energy monoenergetic proton beams are vital for wide applications, thus modern laser-plasma-based ion acceleration methods are aiming to obtain high-energy proton beams with energy spread as low as possible. In this work, we put…

We evaluate the achievable maximum energy of nuclei diffusively accelerated by shock wave in the jet of Cen A, based on an updated model involving the stochastic magnetic fields that are responsible for recent synchrotron X-ray…

High Energy Astrophysical Phenomena · Physics 2009-11-25 Mitsuru Honda

The nature of the intense X-ray emission from powerful extragalactic jets at large ($>1$ kpc) scale is still debated. The scenario that invokes the inverse Compton scattering of the CMB by electrons is challenged by the lack of gamma-ray…

High Energy Astrophysical Phenomena · Physics 2021-01-13 F. Tavecchio

Magnetic reconnection is a leading mechanism for dissipating magnetic energy and accelerating nonthermal particles in Poynting-flux dominated flows. In this letter, we investigate nonthermal particle acceleration during magnetic…

High Energy Astrophysical Phenomena · Physics 2016-02-17 Fan Guo , Xiaocan Li , Hui Li , William Daughton , Bing Zhang , Nicole Lloyd-Ronning , Yi-Hsin Liu , Haocheng Zhang , Wei Deng

Particle acceleration using ultraintense, ultrashort laser pulses is one of the most attractive topics in relativistic laser-plasma research. We report proton/ion acceleration in the intensity range of 5x1019 W/cm2 to 3.3x1020 W/cm2 by…

We use large hybrid (kinetic protons-fluid electrons) simulations to investigate the transport of energetic particles in self-consistent electromagnetic configurations of collisionless shocks. In previous papers of this series, we showed…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Damiano Caprioli , Anatoly Spitkovsky

We present $ab$ $initio$ study of the electronic stopping power of protons and helium ions in an insulating material, HfO$_{2}$. The calculations are carried out in channeling conditions with different impact parameters by employing…

Atomic and Molecular Clusters · Physics 2017-10-11 Chang-Kai Li , Feng Wang , Bin Liao , Xiao-Ping OuYang , Feng-Shou Zhang

Identifying the accelerators of Galactic cosmic ray protons (CRs) with energies up to a few PeV ($10^{15}$ eV) remains a theoretical and observational challenge. Supernova remnants (SNRs) represent strong candidates, as they provide…

High Energy Astrophysical Phenomena · Physics 2024-04-24 Rebecca Diesing

We consider the stochastic acceleration of particles which results from resonant interactions with plasma waves in black hole magnetospheres. We calculate acceleration rates and escape time scales for protons and electrons resonating with…

Astrophysics · Physics 2009-10-28 Charles D. Dermer , James A. Miller , Hui Li

A new, maximum proton energy, $e$, scaling law with the laser pulse energy, $E_L$ has been derived from the results of 3D particle-in-cell (PIC) simulations. Utilizing numerical modelling, protons are accelerated during interactions of the…

Plasma Physics · Physics 2015-06-22 A. V. Brantov , E. A. Govras , V. Yu. Bychenkov , W. Rozmus

Energetic particles with energies from tens of keV to a few hundreds keV are frequently observed in the Earth's magnetotail. Here we study, by means of a test particle numerical simulation, the acceleration of different ion species…

Plasma Physics · Physics 2017-11-29 F. Catapano , G. Zimbardo , S. Perri , A. Greco , D. Delcourt , A. Retino , I. J. Cohen

We report on the experimental studies of laser driven ion acceleration from double-layer target where a near-critical density target with a few-micron thickness is coated in front of a nanometer thin diamond-like carbon foil. A significant…

We study how a high-speed solar wind stream embedded in a slow solar wind affects the transport and energy changes of solar energetic protons in interplanetary space, assuming different levels of cross-field diffusion. This is done using a…

Space Physics · Physics 2020-01-08 Nicolas Wijsen , Angels Aran , Jens Pomoell , Stefaan Poedts