Zobrazeno 1 - 10
of 168
pro vyhledávání: '"Phillip C. Stancil"'
Publikováno v:
Springer Handbook of Atomic, Molecular, and Optical Physics ISBN: 9783030738921
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aae1d75005ede3e43fc4d64428a69cdd
https://doi.org/10.1007/978-3-030-73893-8_55
https://doi.org/10.1007/978-3-030-73893-8_55
Publikováno v:
Springer Handbook of Atomic, Molecular, and Optical Physics ISBN: 9783030738921
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::88df51efa533450eddb94beb5c68d6c4
https://doi.org/10.1007/978-3-030-73893-8_86
https://doi.org/10.1007/978-3-030-73893-8_86
Autor:
Benhui Yang, Naduvalath Balakrishnan, Boyi Zhou, Phillip C. Stancil, Maodu Chen, Brian K. Kendrick
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:6012-6019
The HD molecule is an important coolant in early universe chemistry models and a tracer of H2 in star-forming regions. Rate coefficients for collisional excitation and de-excitation of HD rotational and vibrational levels form important ingredients i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bcd0df8a2763d274b882048f499e8b24
https://doi.org/10.1093/mnras/stab2381
https://doi.org/10.1093/mnras/stab2381
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:381-386
Rate coefficients for rotational transitions in HD induced by H2 impact for rotational levels of HD j ≤ 8 and temperatures 10 K ≤ T ≤ 5000 K are reported. The quantum mechanical close-coupling (CC) method and the coupled-states (CS) decoupling
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::26ca1a8900c96a896436dfdaf41d480a
https://doi.org/10.1093/mnras/stz1735
https://doi.org/10.1093/mnras/stz1735
Publikováno v:
The Journal of chemical physics. 154(3)
Cross sections and rate coefficients for sulfur monoxide (SO) + H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::179029451c121047be29f148db812ab5
https://pubmed.ncbi.nlm.nih.gov/33499617
https://pubmed.ncbi.nlm.nih.gov/33499617
Autor:
Phillip C. Stancil, Connor Ballance, James Babb, Brendan M. McLaughlin, R. T. Smyth, Alfred Müller, M. S. Pindzola
Publikováno v:
High Performance Computing in Science and Engineering '19 ISBN: 9783030667917
Our prime computational effort is to support current and future measurements of atomic photoionization cross-sections at various synchrotron radiation facilities, and ion-atom collision experiments, together with plasma, fusion and astrophysical appl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::feec4227256feda3cdb374319031f2fa
https://doi.org/10.1007/978-3-030-66792-4_3
https://doi.org/10.1007/978-3-030-66792-4_3
Publikováno v:
The journal of physical chemistry letters. 11(13)
Quantum reactive scattering calculations on the vibrational quenching of HD due to collisions with H were carried out employing an accurate potential energy surface. The state-to-state cross sections for the chemical reaction HD(
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02bb33a43b6e2f6c1ea379470645e326
https://pubmed.ncbi.nlm.nih.gov/32512999
https://pubmed.ncbi.nlm.nih.gov/32512999
Autor:
Nancy S. Brickhouse, Artemis Spyrou, L. Storrie-Lombardi, Ella Sciamma-O'Brien, Alan P. Smale, Glenn M. Wahlgren, Phillip C. Stancil, Gary J. Ferland, Stefanie N. Milam
This report provides detailed findings on the critical laboratory astrophysics data needs that are required to maximize the scientific return for NASA's current and near-term planned astrophysics missions. It also provides prioritized rankings on sai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3bbf6528f27cfa4dbdad844e23b9f85f
From four independent calculations using three different theoretical approaches, rate coefficients for the formation of HeH$^+$ via the radiative association of He$^+$ and H were computed. Good agreement is found between our new calculations and prio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0de0d9ca6799509f6640fb7ad56dcfbd
Publikováno v:
Molecular Astrophysics. 13:6-21
SiO emission lines are important probes of chemical processes in diverse astrophysical environments, commonly observed in shocks associated with the outflows of young stellar objects, both low- and high-mass, and in the envelopes of evolved stars. Mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::14b4b6713c1c32b1afc38c44cc39743f
https://doi.org/10.1016/j.molap.2018.09.001
https://doi.org/10.1016/j.molap.2018.09.001