skip to main content
US FlagAn official website of the United States government
dot gov icon
Official websites use .gov
A .gov website belongs to an official government organization in the United States.
https lock icon
Secure .gov websites use HTTPS
A lock ( lock ) or https:// means you've safely connected to the .gov website. Share sensitive information only on official, secure websites.


Title: Ultrastable Carboxyl‐Functionalized Pore‐Space‐Partitioned Metal‐Organic Frameworks for Gas Separation
Abstract Isoreticular chemistry, which enables property optimization by changing compositions without changing topology, is a powerful synthetic strategy. One of the biggest challenges facing isoreticular chemistry is to extend it to ligands with strongly coordinating substituent groups such as unbound −COOH, because competitive interactions between such groups and metal ions can derail isoreticular chemistry. It is even more challenging to have an isoreticular series of carboxyl‐functionalized MOFs capable of encompassing chemically disparate metal ions. Here, with the simultaneous introduction of carboxyl functionalization and pore space partition, a family of carboxyl‐functionalized materials is developed in diverse compositions from homometallic Cr3+and Ni2+to heterometallic Co2+/V3+, Ni2+/V3+, Co2+/In3+, Co2+/Ni2+. Cr‐MOFs remain highly crystalline in boiling water. Unprecedentedly, one Cr‐MOF can withstand the treatment cycle with 10mNaOH and 12mHCl, allowing reversible inter‐conversion between unbound −COOH acid form and −COObase form. These materials exhibit excellent sorption properties such as high uptake capacity for CO2(100.2 cm3 g−1) and hydrocarbon gases (e.g., 142.1 cm3 g−1for C2H2, 110.5 cm3 g−1for C2H4) at 1 bar and 298K, high benzene/cyclohexane selectivity (up to ≈40), and promising separation performance for gas mixtures such as C2H2/CO2and C2H2/C2H4 more » « less
Award ID(s):
2117040
PAR ID:
10556496
Author(s) / Creator(s):
; ; ; ;
Publisher / Repository:
Wiley
Date Published:
Journal Name:
Advanced Materials
ISSN:
0935-9648
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
More Like this
  1. Abstract Although metal–organic frameworks are coordination‐driven assemblies, the structural prediction and design using metal‐ligand interactions can be unreliable due to other competing interactions. Leveraging non‐coordination interactions to develop porous assemblies could enable new materials and applications. Here, we use a multi‐module MOF system to explore important and pervasive impact of ligand‐ligand interactions on metal‐ligand as well as ligand‐ligand co‐assembly process. It is found that ligand‐ligand interactions play critical roles on the scope or breakdown of isoreticular chemistry. With cooperative di‐ and tri‐topic ligands, a family of Ni‐MOFs has been synthesized in various structure types including partitioned MIL‐88‐acs (pacs), interruptedpacs(i‐pacs), and UMCM‐1‐muo. A new type of isoreticular chemistry on the muo platform is established between two drastically different chemical systems. The gas sorption and electrocatalytic studies were performed that reveal excellent performance such as high C2H2/CO2selectivity of 21.8 and high C2H2uptake capacity of 114.5 cm3/g at 298 K and 1 bar. 
    more » « less
  2. Abstract Isoreticular chemistry is among the most powerful strategies for designing novel materials with optimizable pore geometry and properties. Of great significance to the further advance of isoreticular chemistry is the development of broadly applicable new concepts capable of guiding and systematizing the ligand‐family expansion as well as establishing correlations between dissimilar and seemingly uncorrelated ligands for better predictive synthetic design and more insightful structure and property analysis. Here ligand circuit concept is proposed and its use has been demonstrated for the synthesis of a family of highly stable, high‐performance pore‐space‐partitioned materials based on an acyclic ligand,trans,trans‐muconic acid. This work represents a key step toward developing highly porous and highly stable pore‐space‐partitioned materials from acyclic ligands. The new materials exhibit excellent sorption properties such as high uptake capacity for CO2(81.3 cm3 g−1) and C2H2(165.4 cm3 g−1) by CPM‐7.3a‐NiV. CPM‐7.3a‐CoV shows C2H6‐selective C2H6/C2H4separation properties and its high uptakes for C2H4(134.0 cm3 g−1) and C2H6(148.0 cm3 g−1) at 1 bar and 298 K contribute to the separation potential of 1.35 mmol g−1. The multi‐cycle breakthrough experiment confirms the promising separation performance for C2H2/CO2
    more » « less
  3. Abstract Currently, few porous vanadium metal‐organic frameworks (V‐MOFs) are known and even fewer are obtainable as single crystals, resulting in limited information on their structures and properties. Here this work demonstrates remarkable promise of V‐MOFs by presenting an extensible family of V‐MOFs with tailorable pore geometry and properties. The synthesis leverages inter‐modular synergy on a tri‐modular pore‐partitioned platform. New V‐MOFs show a broad range of structural features and sorption properties suitable for gas storage and separation applications for C2H2/CO2, C2H6/C2H4, and C3H8/C3H6. Thec/aratio of the hexagonal cell, a measure of pore shape, is tunable from 0.612 to 1.258. Other tunable properties include pore size from 5.0 to 10.9 Å and surface area from 820 to 2964 m2g−1. With C2H2/CO2selectivity from 3.3 to 11 and high uptake capacity for C2H2from 65.2 to 182 cm3g−1(298K, 1 bar), an efficient separation is confirmed by breakthrough experiments. The near‐record high uptake for C2H6(166.8 cm3g−1) contributes to the promise for C2H6‐selective separation of C2H6/C2H4. The multi‐module pore expansion enables transition from C3H6‐selective to more desirable C3H8‐selective separation with extraordinarily high C3H8uptake (254.9 cm3g−1) and high separation potential (1.25 mmol g−1) for C3H8/C3H6(50:50 v/v) mixture. 
    more » « less
  4. Abstract Trigonal planar M3(O/OH) trimers are among the most important clusters in inorganic chemistry and are the foundational features of multiple high‐impact MOF platforms. Here we introduce a concept called isoreticular cluster series and demonstrate that M3(O/OH), as the first member of a supertrimer series, can be combined with a higher hierarchical member (double‐deck trimer here) to advance isoreticular chemistry. We report here an isoreticular series of pore‐space‐partitioned MOFs called M3M6pacsmade from co‐assembly between M3single‐deck trimer and M3x2double‐deck trimer. Important factors were identified on this multi‐modular MOF platform to guide optimization of each module, which enables the phase selection of M3M6pacsby overcoming the formation of previously‐always‐observed same‐cluster phases. The newpacsmaterials exhibit high surface area and high uptake capacity for CO2and small hydrocarbons, as well as selective adsorption properties relevant to separation of industrially important mixtures such as C2H2/CO2and C2H2/C2H4. Furthermore, new M3M6pacsmaterials show electrocatalytic properties with high activity. 
    more » « less
  5. Context. Carbon monoxide (CO) is a poor tracer of H2in the diffuse interstellar medium (ISM), where most of the carbon is not incorporated into CO molecules, unlike the situation at higher extinctions. Aims. We present a novel, indirect method for constraining H2column densities (NH2) without employing CO observations. We show that previously recognized nonlinearities in the relation between the extinction,AV(H2), derived from dust emission and the H Icolumn density (NH I) are due to the presence of molecular gas. Methods. We employed archival (NH2) data, obtained from the UV spectra of stars, and calculatedAV(H2) toward these sight lines using 3D extinction maps. The following relation fits the data: logNH2= 1.38742 (logAV(H2))3− 0.05359 (logAV(H2))2+ 0.25722 logAV(H2) + 20.67191. This relation is useful for constrainingNH2in the diffuse ISM as it requires onlyNH Iand dust extinction data, which are both easily accessible. In 95% of the cases, the estimates produced by the fitted equation have deviations of less than a factor of 3.5. We constructed aNH2map of our Galaxy and compared it to the CO integrated intensity (WCO) distribution. Results. We find that the average ratio (XCO) betweenNH2andWCOis approximately equal to 2 × 1020cm−2(K km s−1)−1, consistent with previous estimates. However, we find that theXCOfactor varies by orders of magnitude on arcminute scales between the outer and the central portions of molecular clouds. For regions withNH2≳ 1020cm−2, we estimate that the average H2fractional abundance,fH2= 2NH2/(2NH2+NH I), is 0.25. Multiple (distinct) largely atomic clouds are likely found along high-extinction sightlines (AV≥ 1 mag), hence limitingfH2in these directions. Conclusions. More than 50% of the lines of sight withNH2≥ 1020cm−2are untraceable by CO with aJ= 1−0 sensitivity limitWCO= 1 K km s−1
    more » « less