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The relativistic hydrodynamical model HYLANDER-C is used to give estimates for single inclusive particle momentum spectra in $\sqrt{s}$ = 200 $GeV/nucleon$ Au+Au collisions that will be investigated experimentally in the near future. The…

Nuclear Theory · Physics 2008-11-26 B. R. Schlei , D. Strottman

We aim to investigate the blowout jet-like prominence eruption, which occurred on October 6$^{th}$, 2023, with the help of imaging and spectroscopic observations. Firstly, the prominence rises slowly with a speed of 33 km/s, followed by a…

Solar and Stellar Astrophysics · Physics 2026-03-12 Pradeep Kayshap , Petr Jelinek , B. Suresh Babu , Ashok Kumar Baral , Yuandeng Shen

Meteoroids impacting the Earth on a daily basis are fragments of asteroids and comets. By studying fireballs produced during their disintegration in the atmosphere, we can gain information about their source regions and the properties of…

Earth and Planetary Astrophysics · Physics 2022-11-30 J. Borovicka , P. Spurny , L. Shrbeny

We propose a new strategy for the experimental search of the QCD phase transition in heavy ion collisions: One may tune collision energy around the point where the lifetime of the fireball is expected to be longest. We demonstrate that the…

High Energy Physics - Phenomenology · Physics 2009-10-28 C. M. Hung , E. V. Shuryak

We estimate the event-by-event (e-by-e) distribution of the ratio ($\sigma$) of the magnetic field energy to the fluid energy density in the transverse plane of Au-Au collisions at $\sqrt{s_{\rm NN}}$ = 200 GeV. A Monte-Carlo (MC) Glauber…

Nuclear Theory · Physics 2015-12-09 Victor Roy , Shi Pu

A minimal model for curved detonations is studied, illustrating the role of the reaction rate on the detonation speed and its propagation limits. The model is based on a simple extension of the minimal Fickett toy model for detonations…

Fluid Dynamics · Physics 2023-12-08 Matei Ioan Petru Rădulescu , Aliou Sow

Fireball observations from camera networks provide position and time information along the trajectory of a meteoroid that is transiting our atmosphere. The complete dynamical state of the meteoroid at each measured time can be estimated…

Earth and Planetary Astrophysics · Physics 2017-11-07 Eleanor K. Sansom , Mark G. Rutten , Phillip A. Bland

We report simultaneous multicolour observations in 5 bands (UBVRI) of the flickering variability of the cataclysmic variable AE Aqr. Our aim is to estimate the parameters (colours, temperature, size) of the fireballs that produce the…

Solar and Stellar Astrophysics · Physics 2015-06-11 R. K. Zamanov , G. Y. Latev , K. A. Stoyanov , S. Boeva , B. Spassov , S. V. Tsvetkova

Standard GRB fireballs must carry free neutrons. This crucially changes the mechanism of fireball deceleration by an external medium. As the ion fireball decelerates, the coasting neutrons form a leading front. They gradually decay, leaving…

Astrophysics · Physics 2007-05-23 Andrei M. Beloborodov

We investigate the initiation and early evolution of 12 solar eruptions, including six active region hot channel and six quiescent filament eruptions, which were well observed by the \textsl{Solar Dynamics Observatory}, as well as by the…

Solar and Stellar Astrophysics · Physics 2020-05-20 X. Cheng , J. Zhang , B. Kliem , T. {Török} , C. Xing , Z. J. Zhou , B. Inhester , M. D. Ding

As fireball networks grow, the number of events observed becomes unfeasible to manage by manual efforts. Reducing and analysing big data requires automated data pipelines. Triangulation of a fireball trajectory can swiftly provide…

We present a single-freeze-out model with thermal and geometric parameters dependent on the position within the fireball and use it to describe the rapidity and transverse-momentum spectra of pions, kaons, protons, and antiprotons measured…

Nuclear Theory · Physics 2008-11-26 Wojciech Broniowski , Barlomiej Biedron

The neutron yields observed in inertial confinement fusion experiments for higher convergence ratios are about two orders of magnitude smaller than the neutron yields predicted by one-dimensional models, the discrepancy being attributed to…

Nuclear Experiment · Physics 2007-05-23 Silviu Olariu

We report late-time observations of the radio afterglow of GRB 030329. The light curves show a clear achromatic flattening at 50 days after the explosion. We interpret this flattening as resulting from the blast wave becoming…

Astrophysics · Physics 2010-05-12 D. A. Frail , A. M. Soderberg , S. R. Kulkarni , E. Berger , S. A. Yost , D. W. Fox , F. A. Harrison

The jet composition and radiative efficiency of GRBs are poorly constrained from the data. If the jet composition is matter-dominated (i.e. a fireball), the GRB prompt emission spectra would include a dominant thermal component originating…

High Energy Astrophysical Phenomena · Physics 2021-03-10 Bing Zhang , Yu Wang , Liang Li

Transverse energy ($E_T$) distributions have been measured for Au+Au collisions at $\sqrt{s_{NN}}= 200$ GeV by the STAR collaboration at RHIC. $E_T$ is constructed from its hadronic and electromagnetic components, which have been measured…

Nuclear Experiment · Physics 2008-11-26 STAR Collaboration , J. Adams

Environmental molecular beam experiments are used to examine water interactions with liquid methanol films at temperatures from 170 K to 190 K. We find that water molecules with 0.32 eV incident kinetic energy are efficiently trapped by the…

For the calorimetric determination of the primary energy of extensive air showers, measured by fluorescence telescopes, a precise knowledge of the conversion factor (fluorescence yield) between the deposited energy in the atmosphere and the…

Astrophysics · Physics 2009-06-23 Tilo Waldenmaier , Johannes Blümer , Hans Klages

Observations of very early multi-wavelength afterglows are critical to reveal the properties of the radiating fireball and its environment as well as the central engine of gamma-ray bursts (GRBs). We report our optical observations of GRB…

In this paper, we carry out multiwavelength and multiview observations of the prominence eruption, which generates a C2.3 class flare and a coronal mass ejection (CME) on 2023 March 7. For the first time, we apply the revised cone model to…

Solar and Stellar Astrophysics · Physics 2024-10-31 Qingmin Zhang , Yudi Ou , Zhenghua Huang , Yongliang Song , Suli Ma
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