Results 241 to 250 of about 107,571 (269)

Sample environment for simultaneous quasi-elastic neutron scattering and Raman spectroscopy experiments demonstrated on polymer films under changing humidity and temperature. [PDF]

J Appl Crystallogr
Kreuzer LP, Wolf M, Ganster F, Garvey CJ, Stephan A, Betker M, Juranyi F, Müller-Buschbaum P.   +7 more
europepmc   +1 more source

Structure and composition of supported lipid bilayers: a comparison between solvent‐assisted lipid bilayer and vesicle fusion methods

Journal of Applied Crystallography, EarlyView.
Neutron reflectometry is used to compare supported lipid bilayers formed by vesicle fusion and solvent‐assisted lipid bilayer (SALB) methods, revealing structurally comparable architectures with minor differences in acyl chain thickness and low residual solvent incorporation.
Birgit Felderer, Claire Buchanan, Shuhong Wang, Hsin-Hui Shen, Andrew Nelson, Stephen C. L. Hall, Marité Cárdenas   +6 more
wiley   +1 more source

Proton Acceleration with Relativistic Electromagnetic Shock. [PDF]

Adv Sci (Weinh)
Xiao T, Zhang X, Kong F, Zheng X, Gong Z, Shen B.   +5 more
europepmc   +1 more source

Compact stars with non-uniform relativistic polytrope. [PDF]

Sci Rep
Nouh MI, Foda MM, Aboueisha MS.
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

Bond-Reversibility Effects on Self-Crowding of Unimacromolecular Nano-Objects. [PDF]

ACS Macro Lett
Ruiz-Bardillo A, Asenjo-Sanz I, Verde-Sesto E, Porcar L, Kohlbrecher J, Pomposo JA, Moreno AJ, Arbe A, Colmenero J.   +8 more
europepmc   +1 more source

Consensus clustering-based undersampling for improved classification of transient events in time-domain astronomy surveys. [PDF]

Sci Rep
Boongoen T, Iam-On N.
europepmc   +1 more source

Constraining the equation of state in neutron-star cores via the long-ringdown signal. [PDF]

Nat Commun
Ecker C, Gorda T, Kurkela A, Rezzolla L.
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