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Achieving high repeatability and efficiency in laser-induced strong shock wave excitation remains a significant technical challenge, as evidenced by the extensive efforts undertaken at large-scale national laboratories to optimize the…

Far-infrared spectroscopy reveals gas cooling and its underlying heating due to physical processes taking place in the surroundings of protostars. These processes are reflected in both the chemistry and excitation of abundant molecular…

星系天体物理 · 物理学 2018-09-12 Agata Karska , Michael J. Kaufman , Lars E. Kristensen , Ewine F. van Dishoeck

We simulate shock propagation in a wide range of core-collapsing presupernovae: from compact WR stars exploding as SNe Ib/c through very extended envelopes of the narrow-line SNe IIn. We find that the same physical phenomenon of radiating…

天体物理学 · 物理学 2009-11-07 S. Blinnikov , N. Chugai , P. Lundqvist , D. Nadyozhin , S. Woosley , E. Sorokina

We report on a survey for H$\alpha$ bow shock emission around nearby $\gamma$-detected energetic pulsars. This survey adds three Balmer-dominated neutron star bow shocks to the six previously confirmed examples. In addition to the shock…

太阳与恒星天体物理 · 物理学 2015-06-18 Sasha Brownsberger , Roger W. Romani

We considered the structure of steady-state radiative shock waves propagating in the partially ionized hydrogen gas with density rho1 = 1e-10 gm/cm^3 and temperature 3000K <= T1 <= 8000K. The radiative shock wave models with electron…

天体物理学 · 物理学 2009-11-07 Yu. A. Fadeyev , H. Le Coroller , D. Gillet

New non-linear hydrodynamic models have been constructed to simulate the radial pulsations observed in the extreme helium star V652 Her. These use a finer zoning to allow higher radial resolution than in previous simulations. Models…

太阳与恒星天体物理 · 物理学 2021-10-13 C. Simon Jeffery , Pilar Montañés-Rodríguez , Hideyuki Saio

We present the results of an intensive coordinated monitoring campaign in the optical and X-ray wavelength ranges of the low-mass, pre-main sequence star V410Tau carried out with the aim to study the relation between various indicators for…

We use classical electron ensembles and the aligned-electron approximation to examine the effect of laser pulse duration on the dynamics of strong-field double ionization. We cover the range of intensities $10^{14}-10^{16} W/cm^2$ for the…

原子物理 · 物理学 2007-05-23 Phay J. Ho , J. H. Eberly

We present the first measurements of the transverse momentum spectra and mid-rapidity yields of the $\Xi^{0}(1530)$ multi-strange baryon resonance, from $\sqrt{\mathrm{s_{NN}}}=200$ GeV Au+Au collisions at RHIC from the STAR experiment.…

核实验 · 物理学 2008-11-26 R. Witt

RHIC-STAR is a mid-rapidity collider experiment for studying high energy nuclear collisions. The main physics goals of STAR experiment are 1) studying the properties of the strongly coupled Quark Gluon Plasma, 2) explore the QCD phase…

核实验 · 物理学 2016-01-27 Shusu Shi

The HeII (1640 A) line and the resonance doublet of NV (UV1) provide a good diagnostic tool to constrain the excitation mechanism of hot (Te>40,000K) atmospheric/magnetospheric plasmas in T Tauri stars (TTSs). Making use of the data…

太阳与恒星天体物理 · 物理学 2015-06-16 Ana I Gomez de Castro

Multi-dimensional particle-in-cell simulations are used to study the generation of electrostatic shocks in plasma and the reflection of background ions to produce high-quality and high-energy ion beams. Electrostatic shocks are driven by…

等离子体物理 · 物理学 2015-06-12 F. Fiuza , A. Stockem , E. Boella , R. A. Fonseca , L. O. Silva , D. Haberberger , S. Tochitsky , W. B. Mori , C. Joshi

Using the Spitzer Space Telescope, we have observed 90 weak-line and classical T Tauri stars in the vicinity of the Ophiuchus, Lupus, Chamaeleon, and Taurus star-forming regions as part of the Cores to Disks (c2d) Spitzer Legacy project. In…

Classical T Tauri stars show a plethora of in- and outflow signatures in a variety of wavelengths bands. In order to constrain gas velocities and temperatures we analyse the emission in the hot ion lines. We use all available archival FUSE…

天体物理学 · 物理学 2009-11-13 H. M. Günther , J. H. M. M. Schmitt

The far-ultraviolet (FUV; 912--1700 \AA) radiation field from accreting central stars in Classical T Tauri systems influences the disk chemistry during the period of giant planet formation. Previous efforts to measure the true…

太阳与恒星天体物理 · 物理学 2021-09-06 Kevin France , Rebecca Schindhelm , Edwin Bergin , Evelyne Roueff , Herve Abgrall

We present results of energetic laser-ion acceleration from a tailored, near solid density gas target. Colliding hydrodynamic shocks compress a pure hydrogen gas jet into a 70 {\mu}m thick target prior to the arrival of the ultra-intense…

等离子体物理 · 物理学 2016-10-19 M. H. Helle , D. F. Gordon , D. Kaganovich , Y. Chen , J. P. Palastro , A. Ting

We show experimentally that XUV radiation is produced when a laser pulse is Thomson backscattered from sheets of relativistic electrons which are formed at the rear-surface of a foil irradiated on its front side by a high-intensity laser.…

Ion acceleration driven by superintense laser pulses is attracting an impressive and steadily increasing effort. Motivations can be found in the potential for a number of foreseen applications and in the perspective to investigate novel…

等离子体物理 · 物理学 2015-06-15 Andrea Macchi , Marco Borghesi , Matteo Passoni

A theoretical investigation of the ultrafast processes and dynamics of the excited carriers upon irradiation of GaAs with femtosecond (fs) pulsed lasers is performed in conditions that induce material damage and eventually surface…

材料科学 · 物理学 2018-12-12 A. Margiolakis , G. D. Tsibidis , K. M. Dani , G. P. Tsironis

Radiative shocks play a dominant role in star formation. The accretion shocks on the first and second Larson's cores involve radiative processes and are thus characteristic of radiative shocks. In this study, we explore the formation of the…

太阳与恒星天体物理 · 物理学 2015-05-27 Benoît Commerçon , Edouard Audit , Gilles Chabrier , Jean-Pierre Chièze