158 related articles for article (PubMed ID: 23609225)
21. Database Development of SiO
Lee Y; Yeom H; Choi D; Kim S; Lee J; Kim J; Lee H; You S
Nanomaterials (Basel); 2022 Oct; 12(21):. PubMed ID: 36364604
[TBL] [Abstract][Full Text] [Related]
22. Noble gas-transition-metal complexes: coordination of VO2 and VO4 by Ar and Xe atoms in solid noble gas matrixes.
Zhao Y; Gong Y; Chen M; Zhou M
J Phys Chem A; 2006 Feb; 110(5):1845-9. PubMed ID: 16451016
[TBL] [Abstract][Full Text] [Related]
23. RgBF2(+) complexes (Rg = Ar, Kr, and Xe): the cations with large stabilities.
Lv Z; Chen GH; Li D; Wu D; Huang XC; Li ZR; Liu WG
J Chem Phys; 2011 Apr; 134(15):154302. PubMed ID: 21513382
[TBL] [Abstract][Full Text] [Related]
24. Reactivity and regioselectivity of noble gas endohedral fullerenes Ng@C(60) and Ng(2)@C(60) (Ng=He-Xe).
Osuna S; Swart M; Solà M
Chemistry; 2009 Dec; 15(47):13111-23. PubMed ID: 19859923
[TBL] [Abstract][Full Text] [Related]
25. Noble Gas-Tungsten Peroxide Complexes in Noble Gas Matrixes: Infrared Spectroscopy and Density Functional Theoretical Study.
Zhou Z; Zhao Y
J Phys Chem A; 2019 Jan; 123(2):556-564. PubMed ID: 30571114
[TBL] [Abstract][Full Text] [Related]
26. A velocity map imaging study of gold-rare gas complexes: Au-Ar, Au-Kr, and Au-Xe.
Hopkins WS; Woodham AP; Plowright RJ; Wright TG; Mackenzie SR
J Chem Phys; 2010 Jun; 132(21):214303. PubMed ID: 20528018
[TBL] [Abstract][Full Text] [Related]
27. Coulomb explosion in dicationic noble gas clusters: a genetic algorithm-based approach to critical size estimation for the suppression of Coulomb explosion and prediction of dissociation channels.
Nandy S; Chaudhury P; Bhattacharyya SP
J Chem Phys; 2010 Jun; 132(23):234104. PubMed ID: 20572686
[TBL] [Abstract][Full Text] [Related]
28. Spectral Signatures of Protonated Noble Gas Clusters of Ne, Ar, Kr, and Xe: From Monomers to Trimers.
Tan JA; Kuo JL
Molecules; 2022 May; 27(10):. PubMed ID: 35630674
[TBL] [Abstract][Full Text] [Related]
29. Anionic chemistry of noble gases: formation of Mg-NG (NG = Xe, Kr, Ar) compounds under pressure.
Miao MS; Wang XL; Brgoch J; Spera F; Jackson MG; Kresse G; Lin HQ
J Am Chem Soc; 2015 Nov; 137(44):14122-8. PubMed ID: 26488848
[TBL] [Abstract][Full Text] [Related]
30. Vibrational shifts of HXeCl in matrix environments.
Niimi K; Nakayama A; Ono Y; Taketsugu T
J Phys Chem A; 2014 Jan; 118(2):380-7. PubMed ID: 24372421
[TBL] [Abstract][Full Text] [Related]
31. Unprecedented Enhancement of Noble Gas-Noble Metal Bonding in NgAu
Ghosh A; Ghanty TK
J Phys Chem A; 2016 Dec; 120(50):9998-10006. PubMed ID: 27957860
[TBL] [Abstract][Full Text] [Related]
32. Theoretical prediction on the structures and stability of the noble-gas containing anions FNgCC- (Ng=He, Ar, Kr, and Xe).
Peng CY; Yang CY; Sun YL; Hu WP
J Chem Phys; 2012 Nov; 137(19):194303. PubMed ID: 23181302
[TBL] [Abstract][Full Text] [Related]
33. Noble gas-transition metal complexes: coordination of ScO+ by multiple Ar, Kr, and Xe atoms in noble gas matrixes.
Zhao Y; Wang G; Chen M; Zhou M
J Phys Chem A; 2005 Aug; 109(30):6621-3. PubMed ID: 16834012
[TBL] [Abstract][Full Text] [Related]
34. Noble gas encapsulation into carbon nanotubes: predictions from analytical model and DFT studies.
Balasubramani SG; Singh D; Swathi RS
J Chem Phys; 2014 Nov; 141(18):184304. PubMed ID: 25399144
[TBL] [Abstract][Full Text] [Related]
35. Heavy noble gases in solar wind delivered by Genesis mission.
Meshik A; Hohenberg C; Pravdivtseva O; Burnett D
Geochim Cosmochim Acta; 2014 Feb; 127():326-347. PubMed ID: 29151613
[TBL] [Abstract][Full Text] [Related]
36. Noble gas-actinide complexes of the CUO molecule with multiple Ar, Kr, and Xe atoms in noble-gas matrices.
Andrews L; Liang B; Li J; Bursten BE
J Am Chem Soc; 2003 Mar; 125(10):3126-39. PubMed ID: 12617681
[TBL] [Abstract][Full Text] [Related]
37. Binding of noble metal clusters with rare gas atoms: theoretical investigation.
Jamshidi Z; Far MF; Maghari A
J Phys Chem A; 2012 Dec; 116(51):12510-7. PubMed ID: 23206291
[TBL] [Abstract][Full Text] [Related]
38. Experimental and theoretical studies of the infrared spectra and bonding properties of NgBeCO₃ and a comparison with NgBeO (Ng = He, Ne, Ar, Kr, Xe).
Zhang Q; Chen M; Zhou M; Andrada DM; Frenking G
J Phys Chem A; 2015 Mar; 119(11):2543-52. PubMed ID: 25321412
[TBL] [Abstract][Full Text] [Related]
39. Infrared spectra of NgBeS (Ng = Ne, Ar, Kr, Xe) and BeS2 in noble-gas matrices.
Wang Q; Wang X
J Phys Chem A; 2013 Feb; 117(7):1508-13. PubMed ID: 23327099
[TBL] [Abstract][Full Text] [Related]
40. Xe Recovery from Nuclear Power Plants Off-Gas Streams: Molecular Simulations of Gas Permeation through DD3R Zeolite Membrane.
Bashmmakh BJ; Wang X; Jameson CJ; Murad S
Membranes (Basel); 2023 Aug; 13(9):. PubMed ID: 37755190
[TBL] [Abstract][Full Text] [Related]
[Previous] [Next] [New Search]
