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相关论文: Molecular photodissociation

200 篇论文

Pure acetonitrile (CH3CN) and mixed CO:CH3CN and H2O:CH3CN ices have been irradiated at 15K with Vacuum UltraViolet (VUV) photons in the 7-13.6 eV range using synchrotron radiation. VUV photodesorption yields of CH3CN and of photo-products…

As many organic molecules, formic acid (HCOOH) has two conformers (trans and cis). The energy barrier to internal conversion from trans to cis is much higher than the thermal energy available in molecular clouds. Thus, only the most stable…

星系天体物理 · 物理学 2016-11-23 S. Cuadrado , J. R. Goicoechea , O. Roncero , A. Aguado , B. Tercero , J. Cernicharo

The presence of dust can strongly affect the chemical composition of the interstellar medium. We model the chemistry in photodissociation regions (PDRs) using both gas-phase and dust-phase chemical reactions. Our aim is to determine the…

星系天体物理 · 物理学 2016-06-22 G. B. Esplugues , S. Cazaux , R. Meijerink , M. Spaans , P. Caselli

Isotope separation is one of the grand challenges of modern society and holds great potential for basic science, medicine, energy, and defense. We consider here a new and general approach to isotope separation. The method is based on an…

原子物理 · 物理学 2010-05-10 M. Jerkins , I. Chavez , U. Even , M. G. Raizen

The formation of low-mass stars in molecular clouds involves accretion disks and jets, which are of broad astrophysical interest. Accreting stars represent the closest examples of these phenomena. Star and planet formation are also…

太阳与恒星天体物理 · 物理学 2020-05-21 P. C. Schneider , H. M. Günther , K. France

External photoevaporation of protoplanetary discs, by massive O stars in stellar clusters, is thought to be a significant process in the evolution of a disc. It has been shown to result in significant mass loss and disc truncation,…

地球与行星天体物理 · 物理学 2025-08-28 Tyger Peake , Thomas J. Haworth , Mari-Liis Aru , William J. Henney

We modelled \HH\ and CO formation incorporating the fractionation and selective photodissociation affecting CO when \AV\ $\la2$mag. UV absorption measurements typically have N(\cotw)/N(\coth) $\approx 65$ that are reproduced with the…

星系天体物理 · 物理学 2017-02-01 Harvey S. Liszt

We investigate photoisomerization (PI), the shape change of a molecule upon photoabsorption, in a dissipative environment using a simple spin-boson model. We identify two classes of environment depending on whether it "entangles" with the…

材料科学 · 物理学 2007-05-23 Chang-Qin Wu , Jian-Xin Li , Dung-Hai Lee

We present a time-resolved study of the photodissociation dynamics of OCS after UV-photoexcitation at $\lambda=237$ nm. OCS molecules ($X\,^1\Sigma^+$) were primarily excited to the $1\,^1\!A''$ and the $2\,^1\!A'$ Renner-Teller components…

Photophoresis is a physical process based on momentum exchange between an illuminated dust particle and its gaseous environment. Its net effect in protoplanetary discs (PPD) is the outward transport of solid bodies from hot to cold regions.…

地球与行星天体物理 · 物理学 2016-03-23 Nicolas Cuello , Jean-François Gonzalez , Francesco C. Pignatale

Photonic molecules, named by analogy with chemical molecules, are clusters of closely located electromagnetically interacting microcavities or "photonic atoms". As two or several microcavities are brought close together, their optical modes…

光学 · 物理学 2015-05-13 Svetlana V. Boriskina , Trevor M. Benson , Phillip Sewell

We present a method to control photodissociation by manipulating the bond softening mechanism occurring in strong shaped laser fields, by varying the chirp sign and magnitude of an ultra-short laser pulse. Manipulation of bond-softening is…

Recent observations indicate that star formation occurs only in the molecular phase of a galaxy's interstellar medium. A realistic treatment of star formation in simulations and analytic models of galaxies therefore requires that one…

宇宙学与河外天体物理 · 物理学 2015-05-20 Mark R. Krumholz , Nickolay Y. Gnedin

We present a self-consistent theory, as well as an illustrative application to a realistic system, of phase control of photoabsorption in an optically dense medium. We demonstrate that, when propagation effects are taken into consideration,…

量子物理 · 物理学 2009-11-06 David Petrosyan , P. Lambropoulos

The effects of the UV background radiation on the formation of sub-galactic clouds are studied by means of one-dimensional hydrodynamical simulations. The radiative transfer of the ionizing photons due to the absorption by HI, HeI and HeII,…

天体物理学 · 物理学 2009-10-31 Tetsu Kitayama , Satoru Ikeuchi

An overview is given of the chemical processes that occur in primordial systems under the influence of radiation, metal abundances and dust surface reactions. It is found that radiative feedback effects differ for UV and X-ray photons at…

天体物理学 · 物理学 2009-11-13 M. Spaans

We study the photo-desorption occurring in H$_2$O:CO:NH$_3$ ice mixtures irradiated with monochromatic (550 and 900 eV) and broad band (250--1250 eV) soft X-rays generated at the National Synchrotron Radiation Research Center (Hsinchu,…

The study and quantification of UV photon-induced desorption of frozen molecules furthers our understanding of the chemical evolution of cold interstellar regions. Nitric oxide (NO) is an important intermediate species in both gas-phase and…

星系天体物理 · 物理学 2017-10-05 R. Dupuy , G. Féraud , M. Bertin , X. Michaut , T. Putaud , P. Jeseck , L. Philippe , C. Romanzin , V. Baglin , R. Cimino , J. -H. Fillion

A new mechanism is described, analyzed and visualized, for the dissipation of suprathermal rotation energy of molecules in magnetic fields, a necessary condition for their alignment. It relies upon the Lorentz force perturbing the motion of…

星系天体物理 · 物理学 2016-02-17 Renaud Papoular

Photofragment translational spectroscopy has been used to characterize the photodissociation of CH$_3$I and CF$_3$I adsorbed on thin films of a variety of aromatic molecules, initiated by near-UV light. Thin films (nominally 10 monolayers)…

化学物理 · 物理学 2025-01-06 E. T. Jensen