Results 301 to 310 of about 320,327 (338)

A golay metalens for long-range, large aperture, thermal imaging via sparse aperture computational imaging. [PDF]

Nat Commun
Wang J, Wirth-Singh A, Saragadam V, Johnson R, Majumdar A, Veeraraghavan A.   +5 more
europepmc   +1 more source

Fiber-Based Ultra-High-Speed Diffuse Speckle Contrast Analysis System for Deep Blood Flow Sensing Using a Large SPAD Camera. [PDF]

Biosensors (Basel)
Wang Q, Bi R, Zheng S, Erdogan AT, Qi Y, Li C, Hua Y, Pan M, Wang Y, Finlayson N, Olivo M, Henderson RK, Li DD.   +12 more
europepmc   +1 more source

Strong Rest-UV Emission Lines in a “Little Red Dot” Active Galactic Nucleus at z = 7: Early Supermassive Black Hole Growth alongside Compact Massive Star Formation?

Hollis B. Akins, Caitlin M. Casey, Danielle A. Berg, John Chisholm, Aidan P. Cloonan, Maximilien Franco, Steven L. Finkelstein, Seiji Fujimoto, Anton M. Koekemoer, Vasily Kokorev, Erini Lambrides, Brant Robertson, Anthony J. Taylor, D. A. Coulter, Ori D. Fox, Mitchell Karmen   +15 more
openalex   +1 more source

Norbornene Homopolymerization Limits Cell Spreading in Thiol-Ene Photoclick Hydrogels. [PDF]

Adv Healthc Mater
Gentry JL, Caliari SR.
europepmc   +1 more source

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Compact Stars

Modern Physics Letters A, 2018
An analysis and construction is presented for a stellar model characterized by two parameters (w, n) associated with the compactness ratio and anisotropy, respectively. The reliability range for the parameter w [Formula: see text] 1.97981225149 corresponds with a compactness ratio u [Formula: see text] 0.2644959374, the density and pressures are ...
Gabino Estevez-Delgado, Joaquin Estevez-Delgado   +1 more
openaire   +3 more sources

Compact stars: Neutron stars or quark stars or hybrid stars?

Physics Reports, 1994
Abstract Using results from energy calculations of neutron matter, we construct various neutron star equations of state. From these equations of state, together with the Tolman-Oppenheimer-Volkoff equations, we calculate quantities such as pressure, mass density, mass energy density, total mass, radius, and moment of inertia for neutron stars ...
openaire   +1 more source

Compact Stars

2020
Valeria Ferrari, Leonardo Gualtieri, Paolo Pani   +2 more
openaire   +2 more sources

Axisymmetric Rotating Compact Stars

2020
In the previous chapter, we have discussed about the tidal deformability measurement of compact stars with GW170817 and how to apply this measurement to constrain compact star EoSs and hence on models of strong interaction. Such a constraint is made mainly via the inspiral GW signal. In fact, important clues could also be found in the post-merger phase
openaire   +1 more source

Coalescence of black hole–neutron star binaries

Living Reviews in Relativity, 2021
Koutarou Kyutoku, Masaru Shibata, Keisuke Taniguchi   +2 more
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