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The nonbaryonic dark matter of the Universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro world and mechanisms of its symmetry breaking. In the early Universe heavy metastable particles can…

宇宙学与河外天体物理 · 物理学 2017-09-22 K. M. Belotsky , A. D. Dmitriev , E. A. Esipova , V. A. Gani , A. V. Grobov , M. Yu. Khlopov , A. A. Kirillov , S. G. Rubin , I. V. Svadkovsky

We analyze two-particle binding factors of H2, LiH, and HeH+ molecules/ions with the help of our original exact diagonalization ab intio (EDABI) approach. The interelectronic correlations are taken into account rigorously within the second…

强关联电子 · 物理学 2022-08-24 M. Hendzel , M. Fidrysiak , J. Spałek

To understand how the circumstellar environments of post-AGB stars develop into planetary nebulae, we initiate a systematic study of 2D axisymmetric hydrodynamic simulations of protoplanetary nebula (pPN) with a modified ZEUS code. The aim…

太阳与恒星天体物理 · 物理学 2019-10-08 Igor Novikov , Michael Smith

We use the Green Bank Telescope to search for $^3He^+$ emission from a sample of four Galactic planetary nebulae: NGC 3242, NGC 6543, NGC 6826, and NGC 7009. During the era of primordial nucleosynthesis the light elements $^2H$, $^3He$,…

星系天体物理 · 物理学 2021-04-07 T. M. Bania , Dana S. Balser

In spite of the great success of LHC experiments, we do not know whether the discovered "standard model-like" Higgs particle is really what the standard model predicts or a particle some new physics has in its low energy effective theory.…

高能物理 - 唯象学 · 物理学 2014-05-07 C. S. Lim

We have examined the distribution of HI and H$_2$ gases in four face-on galaxies by using the observed dat a of CO and HI line emissions from the literatures. We demonstrate that the gas phase transition of HI and H$_2$ occurs suddenly…

天体物理学 · 物理学 2007-05-23 Mareki Honma , Yoshiaki Sofue , Nobuo Arimoto

We analyze the dynamical evolution of binary stars that interact with a static background of single stars in the environment of a massive black hole (MBH). All stars are considered to be single mass, Newtonian point particles. We follow the…

宇宙学与河外天体物理 · 物理学 2009-08-03 Clovis Hopman

The detection of organic molecules with increasing complexity and potential biological relevance is opening the possibility to understand the formation of the building blocks of life in the interstellar medium. One of the families of…

星系天体物理 · 物理学 2017-02-22 V. M. Rivilla , M. T. Beltrán , J. Martín-Pintado , F. Fontani , P. Caselli , R. Cesaroni

Deuterium, a heavy isotope of hydrogen, is a key tracer of the formation of the Solar System. Recent JWST observations have expanded the dataset of D/H ratios in methane on the KBOs Eris and Makemake, providing new insights into their…

地球与行星天体物理 · 物理学 2025-03-21 Olivier Mousis , Aaron Werlen , Tom Benest Couzinou , Antoine Schneeberger

Two dimensional concordance plots involving the baryon-to-photon ratio, $\eta$, and an effective number of light neutrinos, $N_{\nu}$, are used to discuss the overall consistency of standard big-bang nucleosynthesis in light of recent…

天体物理学 · 物理学 2008-11-26 Christian Y. Cardall , George M. Fuller

Formamide has a key role in prebiotic chemistry as it is the simplest molecule containing the four most important atoms from a biological point of view: hydrogen, carbon, nitrogen and oxygen. Due to its importance, the formation of this…

化学物理 · 物理学 2021-11-02 Berta Martínez-Bachs , Albert Rimola

We investigate molecular evolution in a star-forming core that is initially a hydrostatic starless core and collapses to form a low-mass protostar. The results of a one-dimensional radiation-hydrodynamics calculation are adopted as a…

天体物理学 · 物理学 2009-11-13 Yuri Aikawa , Valentine Wakelam , Robin T. Garrod , Eric Herbst

The solid-state C$_2$H$_2$ chemistry in interstellar H$_2$O-rich ice has been proposed to explain astronomically observed complex organic molecules (COMs), including ketene (CH$_2$CO), acetaldehyde (CH$_3$CHO), and ethanol (CH$_3$CH$_2$OH),…

星系天体物理 · 物理学 2024-05-14 K. -J. Chuang , C. Jäger , J. C. Santos , Th. Henning

After hydrogen, oxygen, and carbon, nitrogen is one of the most chemically active species in the interstellar medium (ISM). Nitrogen bearing molecules have great importance as they are actively involved in the formation of biomolecules.…

太阳与恒星天体物理 · 物理学 2021-08-30 Prasanta Gorai , Bratati Bhat , Milan Sil , Suman K. Mondal , Rana Ghosh , Sandip K. Chakrabarti , Ankan Das

Context: Modern versions of the Miller-Urey experiment claim that formamide (NH$_2$CHO) could be the starting point for the formation of metabolic and genetic macromolecules. Intriguingly, formamide is indeed observed in regions forming…

With the first principles calculations of H and He induced energetics change we demonstrate that in W the accumulation of H (up to 9) and He (up to 4) in a single vacancy (V) surprisingly reduce the formation energy of first and second…

材料科学 · 物理学 2013-05-03 Yu-Wei You , Xiang-Shan Kong , Q. F. Fang , Jun-Ling Chen , G. -N. Luo , C. S. Liu , B. C. Pan , Y. Daid

Non-thermal photons deriving from radiative transitions among the internal ladder of atoms and molecules are an important source of photons in addition to thermal and stellar sources in many astrophysical environments. In the present work…

星系天体物理 · 物理学 2017-08-02 C. M. Coppola , M. V. Kazandjian , D. Galli , A. N. Heays , E. F. van Dishoeck

The emerging possibilities to steer and control electronic motion on subcycle time scales with strong electric fields enable studying the nonperturbative optical response and Bloch bands' topological properties, originated from Berry's…

介观与纳米尺度物理 · 物理学 2021-01-12 Hamed Koochaki Kelardeh

Mott physics is at the root of a plethora of many-body quantum phenomena in quantum materials. Recently, the stacked or twisted structures of van der Waals (vdW) materials have emerged as a unique platform for realizing exotic correlated…

We study the impact of molecular (${\rm H_2}$) and atomic (HI) hydrogen cooling on the galaxy formation threshold. We calculate the fraction of dark matter (DM) halos that exceeds a critical mass required for star formation,…

星系天体物理 · 物理学 2025-04-09 Ethan O. Nadler
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