Electron ionisation of cyanoacetylene: Ionisation cross sections and dication formation
نویسندگان
چکیده
Abstract Cyanoacetylene (HC 3 N) is an important trace species in the atmosphere of Titan. We report, for first time, absolute partial electron ionisation cross sections and precursor-specific cyanoacetylene, following experimental computational investigation. Our methodology involves using 2D ion-ion coincidence mass spectrometry to generate relative sections, over energy range 50 – 200 eV. These values are then normalised scale, a binary encounter-Bethe (BEB) calculation total section. The BEB agrees well with previous determinations literature. spectrometric observations HC 2 N + HCN , ions connectivity markedly different that neutral molecule, point towards rich cationic landscape possessing several local minima. Indeed, [HC N] 2+ minima involving variety cyclic configurations revealed by preliminary investigation, along two linear bent geometries H atom migration (CCCNH ). Determination transition state between these indicates dication able explore majority this conformational at our energies. This investigation energetics also determines adiabatic double 30.3 eV lowest lying singlet HCCCN 30.1 lowest-lying triplet state. bulk cation pairs detected experiment appear originate from excited states, not ground observe 5 two-body dissociations subsequent decay one generated such processes accounts three-body we observe.
منابع مشابه
Evidence of triple collision dynamics in partial photo-ionisation cross sections of helium
Experimental results on partial photo-ionisation cross sections of helium are analysed in the light of recent advances in the semiclassical theory of two-electron atoms. Byun et al [1] predict that the total photo-ionisation cross section below the double-ionisation threshold can, semiclassically, be described in terms of contributions associated with classical orbits starting and ending in the...
متن کاملSimulations of ionisation triggering
We review recent pilot simulations that incorporate feedback from ionising radiation in SPH calculations of star forming clouds. In the case that the ionising radiation source is located within the star forming cloud, the inhomogeneity of the cloud significantly modifies the way that feedback operates compared with spherically symmetric cloud models. Inflow/outflow behaviour develops, combining...
متن کاملRadiative effects of tropospheric ionisation
Introduction Conclusions References Tables Figures Back Close Abstract Introduction Conclusions References Tables Figures Back Close Abstract Despite the increasing evidence that cosmic ray variations may influence clouds and climate, there has been little discussion of the direct radiative effects of atmospheric ionisation. Laboratory experiments show that hydrated molecular cluster-ions, form...
متن کاملBeam Cooling with ionisation losses
This novel type of particle “cooling”, called Ionization Cooling, is applicable to slow ( ) ions stored in a small ring. The many traversals through a thin foil enhance the nuclear reaction probability, in a steady configuration in which ionisation losses are recovered at each turn by a RF-cavity. For a uniform target “foil”, typically few hundred v ≈ 0.1c μg cm thick, transverse betatron oscil...
متن کاملMuon Ionisation Cooling Experiment MICE
The Muon Ionisation Cooling Experiment (MICE) is currently under construction at the Rutherford Appleton Laboratory. MICE will prove the technology necessary for muon ionisation cooling. In ionisation cooling, particle beam emittance is reduced by passage through an energy absorbing medium and RF cavities. In its final configuration, MICE will consist of a 5.5 metre cell of an ionisation coolin...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Journal of Physics B
سال: 2022
ISSN: ['0953-4075', '1361-6455']
DOI: https://doi.org/10.1088/1361-6455/ac6781