Abstract Small carbon clusters (C n , n=2-15) are produced in a molecular beam by pulsed laser vaporization and studied with vacuum ultraviolet (VUV) photoionization mass spectrometry. The required VUV radiation in the 8-12 eV range is provided by the Advanced Light Source (ALS) at the Lawrence Berkeley National Laboratory. Mass spectra at various ionization energies reveal the qualitative relative abundances of the neutral carbon clusters produced. By far the most abundant species is C 3 . Using the tunability of the ALS, ionization threshold spectra are recorded for the clusters up to 15 atoms in size. The ionization thresholds are compared to those measured previously with charge transfer bracketing methods. To interpret the ionization t...
The first results are presented of a new experiment designed both to generate and characterize spect...
In this work we present a systematic theoretical study of neutral and positively charged hydrogenate...
The growth mechanism of hydrocarbons in ionizing environments, such as the interstellar medium (ISM)...
Small carbon clusters (Cn, n = 2-15) are produced in a molecular beam by pulsed laser vaporization ...
Author Institution: Department of Chemistry, University of Georgia, Athens, GA 306025; Chemical Scie...
Author Institution: Department of Chemistry, Univeristy of Georgia, Athens, GA, 30602-2556; Chemical...
Dissociation energies, ionization potentials and fragmentation dynamics of neutral, singly- and doub...
Results from single photon vacuum ultraviolet photoionization of astrophysically relevant CnN cluste...
I.S. Yang, K.J. Taylor, M.J. Craycraft, J. Conceicao, C.L. Pettiette, O. Cheshnovsky and R.E. Smalle...
In this work, we present an alternative to complex laser setups or synchrotron light sources to accu...
Electronic spectra are measured for mass-selected C+2( = 6–14) clusters over the visible and near-in...
Lifshitz C, Sandler P, Grützmacher H-F, Sun J, Weiske T, Schwarz H. Application of thermal kinetics ...
The aim of this work is to understand the fragmentation of small neutral carbon clusters formed by h...
Electronic spectra are measured for protonated carbon clusters (C2n+1H+) containing between 7 and 21...
The first results are presented of a new experiment designed both to generate and characterize spect...
The first results are presented of a new experiment designed both to generate and characterize spect...
In this work we present a systematic theoretical study of neutral and positively charged hydrogenate...
The growth mechanism of hydrocarbons in ionizing environments, such as the interstellar medium (ISM)...
Small carbon clusters (Cn, n = 2-15) are produced in a molecular beam by pulsed laser vaporization ...
Author Institution: Department of Chemistry, University of Georgia, Athens, GA 306025; Chemical Scie...
Author Institution: Department of Chemistry, Univeristy of Georgia, Athens, GA, 30602-2556; Chemical...
Dissociation energies, ionization potentials and fragmentation dynamics of neutral, singly- and doub...
Results from single photon vacuum ultraviolet photoionization of astrophysically relevant CnN cluste...
I.S. Yang, K.J. Taylor, M.J. Craycraft, J. Conceicao, C.L. Pettiette, O. Cheshnovsky and R.E. Smalle...
In this work, we present an alternative to complex laser setups or synchrotron light sources to accu...
Electronic spectra are measured for mass-selected C+2( = 6–14) clusters over the visible and near-in...
Lifshitz C, Sandler P, Grützmacher H-F, Sun J, Weiske T, Schwarz H. Application of thermal kinetics ...
The aim of this work is to understand the fragmentation of small neutral carbon clusters formed by h...
Electronic spectra are measured for protonated carbon clusters (C2n+1H+) containing between 7 and 21...
The first results are presented of a new experiment designed both to generate and characterize spect...
The first results are presented of a new experiment designed both to generate and characterize spect...
In this work we present a systematic theoretical study of neutral and positively charged hydrogenate...
The growth mechanism of hydrocarbons in ionizing environments, such as the interstellar medium (ISM)...