• Je něco špatně v tomto záznamu ?

Step Towards Modeling the Atmosphere of Titan: State-Selected Reactions of O(+) with Methane

J. Hrušák, I. Paidarová,

. 2016 ; 46 (4) : 419-424. [pub] 20160411

Jazyk angličtina Země Nizozemsko

Typ dokumentu časopisecké články

Perzistentní odkaz   https://www.medvik.cz/link/bmc17024076

Methane conversion and in particular the formation of the C-O bond is one of fundamental entries to organic chemistry and it appears to be essential for understanding parts of atmospheric chemistry of Titan, but, in broader terms it might be also relevant for Earth-like exoplanets. Theoretical study of the reactions of methane with atomic oxygen ion in its excited electronic states requires treating simultaneously at least 19 electronic states. Development of a computational strategy that would allow chemically reasonable and computationally feasible treatment of the CH4 (X)/O(+) ((2)D, (2)P) system is by far not trivial and it requires careful examination of all the complex features of the corresponding 19 potential energy surfaces. Before entering the discussion of the rich (photo) chemistry, inspection of the long range behavior of the system with focus on electric dipole transition moments is required. Our calculations show nonzero probability for the reactants to decay before entering the multiple avoided crossings region of the [CH4 + O → products](+) reaction. For the CH4/O(+) ((2)P) system non-zero transition moment probabilities occur over the entire range of considered C-O distances (up to 15 Å), while for the CH4/O(+) ((2)D) system these probabilities are lower by one order of magnitude and were found only at C-O distances smaller than 6 Å.

Citace poskytuje Crossref.org

000      
00000naa a2200000 a 4500
001      
bmc17024076
003      
CZ-PrNML
005      
20170908123656.0
007      
ta
008      
170720s2016 ne f 000 0|eng||
009      
AR
024    7_
$a 10.1007/s11084-016-9503-4 $2 doi
035    __
$a (PubMed)27068153
040    __
$a ABA008 $b cze $d ABA008 $e AACR2
041    0_
$a eng
044    __
$a ne
100    1_
$a Hrušák, J $u J. Heyrovský Institute of Physical Chemistry, Academy of Sciences of the Czech Republic, v. v. i., Dolejškova 3, 182 23, Prague, Czech Republic. jan.hrusak@jh-inst.cas.cz.
245    10
$a Step Towards Modeling the Atmosphere of Titan: State-Selected Reactions of O(+) with Methane / $c J. Hrušák, I. Paidarová,
520    9_
$a Methane conversion and in particular the formation of the C-O bond is one of fundamental entries to organic chemistry and it appears to be essential for understanding parts of atmospheric chemistry of Titan, but, in broader terms it might be also relevant for Earth-like exoplanets. Theoretical study of the reactions of methane with atomic oxygen ion in its excited electronic states requires treating simultaneously at least 19 electronic states. Development of a computational strategy that would allow chemically reasonable and computationally feasible treatment of the CH4 (X)/O(+) ((2)D, (2)P) system is by far not trivial and it requires careful examination of all the complex features of the corresponding 19 potential energy surfaces. Before entering the discussion of the rich (photo) chemistry, inspection of the long range behavior of the system with focus on electric dipole transition moments is required. Our calculations show nonzero probability for the reactants to decay before entering the multiple avoided crossings region of the [CH4 + O → products](+) reaction. For the CH4/O(+) ((2)P) system non-zero transition moment probabilities occur over the entire range of considered C-O distances (up to 15 Å), while for the CH4/O(+) ((2)D) system these probabilities are lower by one order of magnitude and were found only at C-O distances smaller than 6 Å.
650    12
$a atmosféra $7 D001272
650    _2
$a exobiologie $7 D018559
650    12
$a mimozemské prostředí $7 D005118
650    _2
$a methan $x chemie $7 D008697
650    12
$a teoretické modely $7 D008962
650    _2
$a kyslík $x chemie $7 D010100
650    12
$a Saturn $7 D018539
655    _2
$a časopisecké články $7 D016428
700    1_
$a Paidarová, I $u J. Heyrovský Institute of Physical Chemistry, Academy of Sciences of the Czech Republic, v. v. i., Dolejškova 3, 182 23, Prague, Czech Republic.
773    0_
$w MED00007799 $t Origins of life and evolution of the biosphere the journal of the International Society for the Study of the Origin of Life $x 1573-0875 $g Roč. 46, č. 4 (2016), s. 419-424
856    41
$u https://pubmed.ncbi.nlm.nih.gov/27068153 $y Pubmed
910    __
$a ABA008 $b sig $c sign $y a $z 0
990    __
$a 20170720 $b ABA008
991    __
$a 20170908124257 $b ABA008
999    __
$a ok $b bmc $g 1239757 $s 984989
BAS    __
$a 3
BAS    __
$a PreBMC
BMC    __
$a 2016 $b 46 $c 4 $d 419-424 $e 20160411 $i 1573-0875 $m Origins of life and evolution of the biosphere $n Orig Life Evol Biosph $x MED00007799
LZP    __
$a Pubmed-20170720

Najít záznam

Citační ukazatele

Nahrávání dat ...

Možnosti archivace

Nahrávání dat ...