Results 211 to 220 of about 4,103 (254)

Olefin Polymerizations Oriented by Rational Designs of Group‐13 Compounds

The Chemical Record, EarlyView.
In coordination olefin polymerization chemistry, boron and aluminum compounds play important roles in both catalyst components and monomers. This personal account introduces our recent progress on the development of catalyst systems featured by the design of group‐13 counteranions, as well as the application of boronic acid‐crosslinked polyolefins to ...
Ryo Tanaka, Yu Zou
wiley   +1 more source

Neutron capture measurements for s-process nucleosynthesis: A review about CERN n_TOF developments and contributions. [PDF]

Eur Phys J A Hadron Nucl
Domingo-Pardo C, Aberle O, Alcayne V, Alpar G, Halabi MA, Amaducci S, Babiano V, Bacak M, Balibrea-Correa J, Bartolomé J, Bernardes AP, Gameiro BB, Berthoumieux E, Beyer R, Birch M, Boromiza M, Bosnar D, Brusasco B, Caamaño M, Cahuzac A, Calviño F, Calviani M, Cano-Ott D, Casanovas A, Castelluccio DM, Catlett D, Cerutti F, Cescutti G, Chiaveri E, Claps G, Colombetti P, Colonna N, Camprini PC, Cortés G, Cortés-Giraldo MA, Cosentino L, Cristallo S, D'Ottavi A, de la Fuente Rosales G, Dellmann SF, Diakaki M, Di Castro M, Di Chicco A, Dietz M, Dupont E, Durán I, Eleme Z, Eslami M, Fargier S, Fernández-Domínguez B, Finocchiaro P, Flanagan W, Furman V, Gandhi A, García-Infantes F, Gawlik-Ramiega A, Gervino G, Gilardoni S, González-Romero E, Goula S, Griesmayer E, Guerrero C, Gunsing F, Gustavino C, Heyse J, Hillman W, Jenkins DG, Jericha E, Junghans A, Kadi Y, Kaperoni K, Kelly I, Kokkoris M, Kopatch Y, Krtička M, Kyritsis N, Lederer-Woods C, Lerendegui-Marco J, Manna A, Martínez T, Martínez-Cañada M, Masi A, Massimi C, Mastinu P, Mastromarco M, Maugeri EA, Mazzone A, Mendoza E, Mengoni A, Michalopoulou V, Milazzo PM, Moldenhauer J, Mucciola R, González EM, Musumarra A, Negret A, Odusina E, Papanikolaou D, Patronis N, Pavón-Rodríguez JA, Pellegriti MG, Pérez-Maroto P, de Rada Fiol AP, Perfetto G, Perkowski J, Petrone C, Pieretti N, Piersanti L, Pirovano E, Porras I, Praena J, Quesada JM, Reifarth R, Rochman D, Romanets Y, Rooney A, Rovira G, Rubbia C, Sánchez-Caballero A, Sahoo RN, Scarpa D, Schillebeeckx P, Smith AG, Sosnin NV, Spelta M, Stamati ME, Stasiak K, Tagliente G, Tarifeño-Saldivia A, Tarrío D, Torres-Sánchez P, Tosi S, Tsiledakis G, Valenta S, Vaz P, Vecchio G, Vescovi D, Vlachoudis V, Vlastou R, Wallner A, Weiss C, Woods PJ, Wright T, Wu R, Žugec P, The n_TOF Collaboration.   +145 more
europepmc   +1 more source

Comparison of proton and photon therapy in stereotactic arrhythmia radioablation for ventricular tachycardia. [PDF]

Phys Imaging Radiat Oncol
Shah KD, Chang CW, Patel P, Tian S, Shao Y, Higgins KA, Wang Y, Roper J, Zhou J, Tian Z, Yang X.   +10 more
europepmc   +1 more source

Backbone Dynamics of Bottlebrush Polymers Studied by Neutron Scattering. [PDF]

Macromolecules
Bichler KJ, Jakobi B, Sarter M, Schneider GJ.   +3 more
europepmc   +1 more source

Synthesis of Highly Ordered Amphiphilic Polymer Conetwork Hydrogels via the Topologically Precise Interconnection of Two Highly Incompatible Polymers. [PDF]

Chem Mater
Apostolides DE, Michael G, Andronikou K, Patrickios CS, Pásztor S, Szarka G, Petróczy A, Iván B, Sakai T, Prévost S, Tsalikis DG, Gradzielski M.   +11 more
europepmc   +1 more source

An interstellar mission to test astrophysical black holes. [PDF]

iScience
Bambi C.
europepmc   +1 more source

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Neutron star crusts

Physical Review Letters, 1993
We calculate properties of neutron star matter at subnuclear densities using an improved nuclear Hamiltonian. Nuclei disappear and the matter becomes uniform at a density of about 0.6n(s), where n(s) of about 0.16/cu fm is the saturation density of nuclear matter. As a consequence, the mass of matter in the crusts of neutron stars is only about half as
, Lorenz, , Ravenhall, , Pethick
openaire   +2 more sources

Neutron star matter

Nuclear Physics A, 1971
Abstract The matter in neutron stars is essentially in its ground state and ranges in density up to and beyond 3 × 10 14 g/cm 3 , the density of nuclear matter. Here we determine the constitution of the ground state of matter and its equation of state in the regime from 4.3 × 10 11 g/cm 3 where free neutrons begin to “drip” out of the nuclei, up ...
GORDON BAYM, HANS A. BETHE, CHRISTOPHER J. PETHICK   +2 more
openaire   +1 more source

Neutron star cores

Astrophysics and Space Science, 1975
Current theories, and the astrophysical implications, of the nature of high density neutron star matter are reviewed. Suggestions are made for a compromise between the alternatives of neutron crystallization and pion condensation.
openaire   +1 more source