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Study sheds light on turbulence in astrophysical plasmas(图)     sheds light  turbulence  astrophysical plasmas       font style='font-size:12px;'> 2017/12/19
Plasmas, gas-like collections of ions and electrons, make up an estimated 99 percent of the visible matter in the universe, including the sun, the stars, and the gaseous medium that permeates the spac...
近日,国际顶级天体物理杂志《The Astrophysical Journal》刊发了武汉理工大学理学院青年教师廖恺博士(第一作者)论文“The Distance Duality Relation From Strong Gravitational Lensing”(利用强引力透镜研究宇宙距离对偶关系),提出了一种全新的测试宇宙学基本原理以及基础物理学的方法。
Magnetic reconnection is a fundamental process in a plasma that facilitates the release of energy stored in the magnetic field by permitting a change in the magnetic topology. In this article we prese...
DAMA and CoGeNT without astrophysical uncertainties     DAMA  CoGeNT without  astrophysical  uncertainties       font style='font-size:12px;'> 2011/10/18
The CoGeNT collaboration has reported evidence of an annual modulation in its first fifteen months of data. Here we compare the amplitude and phase of this signal to the modulation observed by the DAM...
The surface tension of cold and dense QCD phase transitions has appeared recently as a key ingredient in different astrophysical scenarios, ranging from core-colapse supernovae explosions to compact s...
A technique is presented for producing synthetic images from numerical simulations whereby the image resolution is adapted around prominent features. In so doing, adaptive image ray-tracing (AIR) impr...
We measure the recoil velocity as a function of spin for equal-mass, highly-spinning black-hole binaries, with spins in the orbital plane, equal in magnitude and opposite in direction. We con rm that...
Integrating Out Astrophysical Uncertainties      Astrophysical Uncertainties        font style='font-size:12px;'> 2010/11/16
Underground searches for dark matter involve a complicated interplay of particle physics, nuclear physics, atomic physics and astrophysics. We attempt to remove the uncertainties associated with astro...
We present the results of spectroscopy of 71 objects with steep and ultra-steep spectra (α < −0.9, S / ν ) from the“Big Trio” (RATAN-600–VLA–BTA) project, performed with the “Scorpio” spectrogra...
Astronomically, there are viable mechanisms for distributing organic material throughout the Milky Way. Biologically, the destructive effects of ultraviolet light and cosmic rays means that the majori...
Astrophysical Jets : what can we learn from Solar Ejections?      Sun  coronal mass ejections  Galaxies  jets  Magnetic reconnection       font style='font-size:12px;'> 2010/11/11
Ejections from the Sun can be observed with a higher resolution than in any other astrophysical object: can we build up on solar results and apply them to astrophysical objects? Aim of this work is to...
Los trabajos que, junto con mi director, presentaremos a continuaci&acute;on se engloban dentro de la tesis de doctorado titulada “Emisi&acute;on no-t&acute;ermica asociada a ondas de choque astrof&a...
We formulate and implement the Euler equations with SGS dynamics and provide numerical tests of an SGS turbulence energy model that predicts the turbulent pressure of unresolved velocity fluctuations ...
The multidimensional gas-kinetic scheme for the Navier-Stokes equations under gravitational fields [J. Comput. Phys. 226 (2007) 2003-2027] is extended to resistive magnetic flows. The non-magnetic par...
We propose a physically transparent analytic model of astrophysical S-factors as a function of a center-of-mass energy E of colliding nuclei (below and above the Coulomb barrier) for non-resonant fusi...

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