scholarly journals Rainbow scattering in rotationally inelastic collisions of HCl and H2

2021 ◽  
Vol 154 (10) ◽  
pp. 104304
Author(s):  
Masato Morita ◽  
Junxiang Zuo ◽  
Hua Guo ◽  
Naduvalath Balakrishnan
Keyword(s):  
Inelastic Collisions ◽  
Rainbow Scattering

RELAXATION PHENOMENA IN AND MICROSCOPIC TRANSPORT THEORIES OF DEEPLY INELASTIC COLLISIONS BETWEEN HEAVY IONS

1976 ◽  
Vol 37 (C5) ◽  
pp. C5-141-C5-160 ◽  
Author(s):  
Wolfgang Nörenberg
Keyword(s):  
Heavy Ions ◽  
Inelastic Collisions ◽  
Relaxation Phenomena

scholarly journals The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo

2020 ◽  
Author(s):  
Kun Ting Eddie Chua ◽  
Karia Dibert ◽  
Mark Vogelsberger ◽  
Jesús Zavala
Keyword(s):  
Dark Matter ◽  
High Speed ◽  
Cold Dark Matter ◽  
Milky Way ◽  
Direct Detection ◽  
Major Axis ◽  
Inelastic Collisions ◽  
Axis Ratio ◽  
Lower Velocity ◽  
The Impact

Abstract We study the effects of inelastic dark matter self-interactions on the internal structure of a simulated Milky Way (MW)-size halo. Self-interacting dark matter (SIDM) is an alternative to collisionless cold dark matter (CDM) which offers a unique solution to the problems encountered with CDM on sub-galactic scales. Although previous SIDM simulations have mainly considered elastic collisions, theoretical considerations motivate the existence of multi-state dark matter where transitions from the excited to the ground state are exothermic. In this work, we consider a self-interacting, two-state dark matter model with inelastic collisions, implemented in the Arepo code. We find that energy injection from inelastic self-interactions reduces the central density of the MW halo in a shorter timescale relative to the elastic scale, resulting in a larger core size. Inelastic collisions also isotropize the orbits, resulting in an overall lower velocity anisotropy for the inelastic MW halo. In the inner halo, the inelastic SIDM case (minor-to-major axis ratio s ≡ c/a ≈ 0.65) is more spherical than the CDM (s ≈ 0.4), but less spherical than the elastic SIDM case (s ≈ 0.75). The speed distribution f(v) of dark matter particles at the location of the Sun in the inelastic SIDM model shows a significant departure from the CDM model, with f(v) falling more steeply at high speeds. In addition, the velocity kicks imparted during inelastic collisions produce unbound high-speed particles with velocities up to 500 km s−1 throughout the halo. This implies that inelastic SIDM can potentially leave distinct signatures in direct detection experiments, relative to elastic SIDM and CDM.

scholarly journals Inelastic collisions in radiofrequency-dressed mixtures of ultracold atoms

2020 ◽  
Vol 2 (3) ◽  
Author(s):  
Elliot Bentine ◽  
Adam J. Barker ◽  
Kathrin Luksch ◽  
Shinichi Sunami ◽  
Tiffany L. Harte ◽  
...  
Keyword(s):  
Ultracold Atoms ◽  
Inelastic Collisions

Motion periodicity and bifurcation of a wave excited hopping ball

2019 ◽  
Vol 475 (2228) ◽  
pp. 20190137
Author(s):  
Gaurang Ruhela ◽  
Anirvan DasGupta
Keyword(s):  
Wave Amplitude ◽  
Harmonic Wave ◽  
Inelastic Collisions ◽  
Loss Of Stability ◽  
Elastic Surface ◽  
Minimum Frequency ◽  
Surface Motion ◽  
Return Map ◽  
Ball Problem ◽  
Subsequent Loss

We consider the problem of a hopping ball excited by a travelling harmonic wave on an elastic surface. The ball, considered as a particle, is assumed to interact with the surface through inelastic collisions. The surface motion due to the wave induces a horizontal drift in the ball. The problem is treated analytically under certain approximations. The phase space of the hopping motion is captured by constructing a phase-velocity return map. The fixed points of the return map and its compositions represent periodic hopping solutions. The linear stability of the obtained periodic solution is studied in detail. The minimum frequency for the onset of periodic hops, and the subsequent loss of stability at the bifurcation frequency, have been determined analytically. Interestingly, for small values of wave amplitude, the analytical solutions reveal striking similarities with the results of the classical bouncing ball problem.

Close-coupling studies of the orientation dependence of rotationally inelastic collisions

1977 ◽  
Vol 67 (6) ◽  
pp. 2703 ◽  
Author(s):  
Millard H. Alexander
Keyword(s):  
Orientation Dependence ◽  
Inelastic Collisions ◽  
Close Coupling

Infrared Laser Action in Sr Vapor Resulting from Optical Pumping and Inelastic Collisions

1969 ◽  
Vol 186 (2) ◽  
pp. 342-343 ◽  
Author(s):  
P. P. Sorokin ◽  
J. R. Lankard
Keyword(s):  
Optical Pumping ◽  
Laser Action ◽  
Infrared Laser ◽  
Inelastic Collisions

Inelastic collisions at low energies

1969 ◽  
Vol 47 (10) ◽  
pp. 1723-1729 ◽  
Author(s):  
A. Dalgarno
Keyword(s):  
Energy Loss ◽  
Cross Sections ◽  
Low Energy ◽  
Inelastic Collisions ◽  
Low Energies ◽  
Low Energy Electrons ◽  
The Cross ◽  
Loss Rates

A summary is presented of the processes by which low energy electrons lose energy in moving through the atmosphere and estimates are given of the cross sections and energy loss rates. The mechanisms by which thermal electrons cool are described and the cooling efficiencies are listed.

Analysis of deep inelastic collisions between16O and27Al

1987 ◽  
Vol 328 (2) ◽  
pp. 219-226
Author(s):  
W. Q. Shen ◽  
W. M. Qiao ◽  
W. L. Zhan ◽  
L. X. Ge ◽  
X. T. Zhu ◽  
...  
Keyword(s):  
Inelastic Collisions

scholarly journals Rainbow scattering by a coated sphere

1994 ◽  
Vol 33 (21) ◽  
pp. 4677 ◽  
Author(s):  
James A. Lock ◽  
J. Michael Jamison ◽  
Chih-Yang Lin
Keyword(s):  
Rainbow Scattering
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