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We report on the detection of hydromagnesium isocyanide, HMgNC, in the laboratory and in the carbon rich evolved star IRC+10216. The J=1-0 and J=2-1 lines were observed in our microwave laboratory equipment in Valladolid with a spectral…

A recently developed reduced activation ferritic/martensitic steel MNHS was irradiated with 200keV He ions to a fluence of 1E21ions/m^2 at 450 celsius degree and 1E20ions/m^2 at 300 celsius degree and 450 celsius degree, respectively. The…

The evolutionary calculations for population I stars with masses on the main sequence 5 M_\odot <= M_0 <= 6.1 M_\odot and initial fractional abundances of helium Y_0=0.28 and heavier elements Z_0=0.02 were carried out to the stage of…

太阳与恒星天体物理 · 物理学 2020-09-30 Yu. A. Fadeyev

In the minimal supersymmetric model, the coannihilation of the lighter stop $\tilde{t}_1$ and bino-like dark matter $\chi$ provides a feasible way to accommodate the correct dark matter relic abundance. In this scenario, due to the…

高能物理 - 唯象学 · 物理学 2020-09-23 Guang Hua Duan , Xiang Fan , Ken-ichi Hikasa , Bo Peng , Jin Min Yang

Global stellar oscillations probe the internal structure of stars. In low- to intermediate-mass red giants, these oscillations provide signatures from both the outer regions of the star as well as from the core. These signatures are…

太阳与恒星天体物理 · 物理学 2023-08-08 S. Hekker , Y. Elsworth , T. A. M. Braun , S. Basu

The H atoms inside minihalos (i.e. halos with virial temperatures T_vir < 10^4 K, in the mass range roughly from 10^4 M_sun to 10^8 M_sun) during the cosmic dark ages in a LambdaCDM universe produce a redshifted background of…

天体物理学 · 物理学 2009-11-11 Paul R. Shapiro , Kyungjin Ahn , Marcelo A. Alvarez , Ilian T. Iliev , Hugo Martel , Dongsu Ryu

Stable DC atmospheric pressure normal glow discharges in ambient air were produced between the water surface and the metallic capillary coupled with influx of helium gas. Multiple independent repeated trials indicated that vibrational…

等离子体物理 · 物理学 2013-07-10 Shaofeng Xu , Xiaoxia Zhong

We present a path-integral Monte Carlo study of dissociation in dense hydrogen ($1.75 \leq r_s \leq 2.2$, with $r_s$ the Wigner sphere radius). As temperature is lowered from $10^5$ to 5000 K, a molecular hydrogen gas forms spontaneously…

凝聚态物理 · 物理学 2009-10-28 W. R. Magro , D. M. Ceperley , C. Pierleoni , B. Bernu

We present infrared absorption studies of solid hydrogen deuteride to pressures as high as 3.4 megabar in a diamond anvil cell and temperatures in the range 5 to 295 K. Above 198 GPa the sample transforms to a mixture of HD ,H2 and D2,…

其他凝聚态物理 · 物理学 2016-04-13 Ranga P. Dias , Ori Noked , Isaac F. Silvera

Motivated by recent observations with Herschel/PACS, and the availability of new rate coefficients for the collisional excitation of CO (Yang et al. 2010), the excitation of warm astrophysical CO is revisited with the use of numerical and…

星系天体物理 · 物理学 2015-06-04 David A. Neufeld

The molecular gas in the DR21 massive star formation region is known to be affected by the strong UV field from the central star cluster and by a fast outflow creating a bright shock. The relative contribution of both heating mechanisms is…

The dc magnetoconductivity of the multisubband two-dimensional electron system formed on the liquid helium surface in the presence of resonant microwave irradiation is described, and a new mechanism of the negative linear response…

介观与纳米尺度物理 · 物理学 2015-03-19 Yuriy P. Monarkha

We study superfluid helium droplets multiply charged with ions. When stable, the charges are found to reside in equilibrium close to the droplet surface, thus representing a physical realization of Thomson's model. We find the minimum…

介观与纳米尺度物理 · 物理学 2024-10-23 Ernesto Garcia-Alfonso , Francesco Ancilotto , Manuel Barranco , Fausto Cargnoni , Nadine Halberstadt , Marti Pi

Shock waves constitute discontinuities in matter which are relevant in studying the plasma behaviour in astrophysical scenarios and in heavy-ion collision. They can produce conical emission in relativistic collisions and are also thought to…

高能天体物理现象 · 物理学 2013-09-03 Ritam Mallick , Stefan Schramm

Outflows perpendicular to the guide field are believed to be a possible signature of magnetic reconnection in the solar corona and specifically a way to detect the occurrence of ubiquitous small-angle magnetic reconnection. The aim of this…

太阳与恒星天体物理 · 物理学 2025-03-05 G. Cozzo , P. Pagano , F. Reale , P. Testa , A. Petralia , J. Martinez-Sykora , V. Hansteen , B. De Pontieu

Many present-day galaxies are known to harbor supermassive, >10^6 Mo, black holes. These central black holes must have grown through accretion from less massive seeds in the early universe. The molecules CO and H2 can be used to trace this…

天体物理学 · 物理学 2009-11-13 M. Spaans , R Meijerink

Current magnetohydrodynamic (MHD) simulations of the initiation of solar eruptions are still commonly carried out with idealized magnetic field models, whereas the realistic coronal field prior to eruptions can possibly be reconstructed…

太阳与恒星天体物理 · 物理学 2015-06-16 Chaowei Jiang , Xueshang Feng , S. T. Wu , Qiang Hu

There is evidence in 21cm HI emission for voids several kpc in size centered approximately on the Galactic centre, both above and below the Galactic plane. These appear to map the boundaries of the Galactic nuclear wind. An analysis of HI…

星系天体物理 · 物理学 2016-08-17 Felix J. Lockman , N. M. McClure-Griffiths

The present work reports new experiments of detonation diffraction in a 2D channel configuration in stoichiometric mixtures of ethylene, ethane, and methane with oxygen as oxidizer. The flow field details are obtained using high-speed…

流体动力学 · 物理学 2022-11-15 Farzane Zangene , Qiang Xiao , Matei Radulescu