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      Anion Recognition in Water: Recent Advances from a Supramolecular and Macromolecular Perspective

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          Abstract

          The recognition of anions in water remains a key challenge in modern supramolecular chemistry, and is essential if proposed applications in biological, medical, and environmental arenas that typically require aqueous conditions are to be achieved. However, synthetic anion receptors that operate in water have, in general, been the exception rather than the norm to date. Nevertheless, a significant step change towards routinely conducting anion recognition in water has been achieved in the past few years, and this Review highlights these approaches, with particular focus on controlling and using the hydrophobic effect, as well as more exotic interactions such as C−H hydrogen bonding and halogen bonding. We also look beyond the field of small‐molecule recognition into the macromolecular domain, covering recent advances in anion recognition based on biomolecules, polymers, and nanoparticles.

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          Rapid planetesimal formation in turbulent circumstellar discs

          The initial stages of planet formation in circumstellar gas discs proceed via dust grains that collide and build up larger and larger bodies (Safronov 1969). How this process continues from metre-sized boulders to kilometre-scale planetesimals is a major unsolved problem (Dominik et al. 2007): boulders stick together poorly (Benz 2000), and spiral into the protostar in a few hundred orbits due to a head wind from the slower rotating gas (Weidenschilling 1977). Gravitational collapse of the solid component has been suggested to overcome this barrier (Safronov 1969, Goldreich & Ward 1973, Youdin & Shu 2002). Even low levels of turbulence, however, inhibit sedimentation of solids to a sufficiently dense midplane layer (Weidenschilling & Cuzzi 1993, Dominik et al. 2007), but turbulence must be present to explain observed gas accretion in protostellar discs (Hartmann 1998). Here we report the discovery of efficient gravitational collapse of boulders in locally overdense regions in the midplane. The boulders concentrate initially in transient high pressures in the turbulent gas (Johansen, Klahr, & Henning 2006), and these concentrations are augmented a further order of magnitude by a streaming instability (Youdin & Goodman 2005, Johansen, Henning, & Klahr 2006, Johansen & Youdin 2007) driven by the relative flow of gas and solids. We find that gravitationally bound clusters form with masses comparable to dwarf planets and containing a distribution of boulder sizes. Gravitational collapse happens much faster than radial drift, offering a possible path to planetesimal formation in accreting circumstellar discs.
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            Systematic evolution of ligands by exponential enrichment: RNA ligands to bacteriophage T4 DNA polymerase

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              In vitro selection of RNA molecules that bind specific ligands.

              Subpopulations of RNA molecules that bind specifically to a variety of organic dyes have been isolated from a population of random sequence RNA molecules. Roughly one in 10(10) random sequence RNA molecules folds in such a way as to create a specific binding site for small ligands.
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                Author and article information

                Contributors
                C.J.Serpell@kent.ac.uk
                paul.beer@chem.ox.ac.uk
                Journal
                Angew Chem Int Ed Engl
                Angew. Chem. Int. Ed. Engl
                10.1002/(ISSN)1521-3773
                ANIE
                Angewandte Chemie (International Ed. in English)
                John Wiley and Sons Inc. (Hoboken )
                1433-7851
                1521-3773
                27 November 2015
                February 2016
                : 55
                : 6 ( doiID: 10.1002/anie.v55.6 )
                : 1974-1987
                Affiliations
                [ 1 ] Chemistry Research Laboratory Department of ChemistryUniversity of Oxford Mansfield Road Oxford OX1 3TAUK
                [ 2 ] School of Physical Sciences, Ingram BuildingUniversity of Kent Canterbury Kent CT2 7NHUK
                Author information
                http://orcid.org/0000-0003-1555-3479
                http://orcid.org/0000-0002-2848-9077
                Article
                ANIE201506589
                10.1002/anie.201506589
                4755225
                26612067
                6548c9d9-327b-41bc-8fcb-574fa4436e30
                © 2015 The Authors. Published by Wiley-VCH Verlag GmbH & Co. KGaA.

                This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.

                History
                : 16 July 2015
                Page count
                Figures: 15, Tables: 0, References: 104, Pages: 14
                Funding
                Funded by: EPSRC
                Funded by: European Research Council
                Award ID: 267426
                Categories
                Review
                Reviews
                Molecular Recognition
                Custom metadata
                2.0
                anie201506589
                February 5, 2016
                Converter:WILEY_ML3GV2_TO_NLMPMC version:4.7.6 mode:remove_FC converted:09.02.2016

                Chemistry
                anions,host–guest systems,molecular recognition,supramolecular chemistry,water
                Chemistry
                anions, host–guest systems, molecular recognition, supramolecular chemistry, water

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