skip to main content


Title: High Dense Gas Fraction in a Gas-rich Star-forming Galaxy at z = 1.2
Award ID(s):
1614213
NSF-PAR ID:
10026041
Author(s) / Creator(s):
; ; ; ; ;
Date Published:
Journal Name:
The Astrophysical Journal
Volume:
838
Issue:
2
ISSN:
1538-4357
Page Range / eLocation ID:
136
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
More Like this
  1. Abstract

    Polymeric membrane‐based gas separation technology has significant advantages compared with traditional amine‐based CO2separation method. In this work, SEBS block copolymer is used as a polymer matrix to incorporate triethylene oxide (TEO) functionality. The short ethylene oxide segment is chosen to avoid crystallization, which is confirmed by differential scanning calorimetry and wide‐angle X‐ray scattering characterizations. The gas permeability results reveal that CO2/N2selectivity increased with increasing content of TEO functional group. The highest CO2permeability (281 Barrer) and CO2/N2selectivity (31) were obtained for the membrane with the highest TEO incorporation (57 mol%). Increasing the TEO content in these copolymers results in an increase in CO2solubility and a decrease in C2H6solubility. For example, as the grafted TEO content increased from 0 to 57 mol%, the CO2solubility and CO2/C2H6solubility selectivity increased from 0.72 to 1.3 cm3(STP)/cm3atm and 0.47 to 1.3 at 35°C, respectively. The polar ether linkage in TEO‐grafted SEBS copolymers exhibits favorable interaction with CO2and unfavorable interaction with nonpolar C2H6, thus enhancing CO2/C2H6solubility selectivity.

     
    more » « less
  2. The reaction of the D1-silylidyne radical (SiD; X 2 Π) with phosphine (PH 3 ; X 1 A 1 ) was conducted in a crossed molecular beams machine under single collision conditions. Merging of the experimental results with ab initio electronic structure and statistical Rice–Ramsperger–Kassel–Marcus (RRKM) calculations indicates that the reaction is initiated by the barrierless formation of a van der Waals complex (i0) as well as intermediate (i1) formed via the barrierless addition of the SiD radical with its silicon atom to the non-bonding electron pair of phosphorus of the phosphine. Hydrogen shifts from the phosphorous atom to the adjacent silicon atom yield intermediates i2a, i2b, i3; unimolecular decomposition of these intermediates leads eventually to the formation of trans / cis -phosphinidenesilyl (HSiPH, p2/p4) and phosphinosilylidyne (SiPH 2 , p3) via hydrogen deuteride (HD) loss (experiment: 80 ± 11%, RRKM: 68.7%) and d - trans / cis -phosphinidenesilyl (DSiPH, p2′/p4′) plus molecular hydrogen (H 2 ) (experiment: 20 ± 7%, RRKM: 31.3%) through indirect scattering dynamics via tight exit transition states. Overall, the study reveals branching ratios of p2/p4/p2′/p4′ ( trans / cis HSiPH/DSiPH) to p3 (SiPH 2 ) of close to 4 : 1. The present study sheds light on the complex reaction dynamics of the silicon and phosphorous systems involving multiple atomic hydrogen migrations and tight exit transition states, thus opening up a versatile path to access the previously elusive phosphinidenesilyl and phosphinosilylidyne doublet radicals, which represent potential targets of future astronomical searches toward cold molecular clouds (TMC-1), star forming regions (Sgr(B2)), and circumstellar envelopes of carbon rich stars (IRC + 10216). 
    more » « less