Nuclear Science References (NSR)

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NSR database version of April 26, 2024.

Search: Author = F.Weber

Found 26 matches.

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2023LI44 Phys.Rev. C 108, 025810 (2023)

J.J.Li, A.Sedrakian, F.Weber

Universal relations for compact stars with heavy baryons

doi: 10.1103/PhysRevC.108.025810
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2023WE04 Phys.Rev. C 107, 034313 (2023)

F.Weber, T.E.Albrecht-Schonzart, S.O.Allehabi, S.Berndt, M.Block, H.Dorrer, C.E.Dullmann, V.A.Dzuba, J.G.Ezold, V.V.Flambaum, V.Gadelshin, S.Goriely, A.Harvey, R.Heinke, S.Hilaire, M.Kaja, T.Kieck, N.Kneip, U.Koster, J.Lantis, C.Mokry, D.Munzberg, S.Nothhelfer, S.Oberstedt, S.Peru, S.Raeder, J.Runke, V.Sonnenschein, M.Stemmler, D.Studer, P.Thorle-Pospiech, H.Tomita, N.Trautmann, S.Van Cleve, J.Warbinek, K.Wendt

Nuclear moments and isotope shifts of the actinide isotopes ^249-253Cf probed by laser spectroscopy

NUCLEAR MOMENTS ^{249,250,251,252,253}Cf; measured hyperfine spectra; deduced energy positions of three atomic ground-state transitions, isotope shifts. ^249,251,253Cf; deduced nuclear magnetic dipole moments, hyperfine parameters. ^249,253Cf; deduced spectroscopic quadrupole moments. Comparison with previous experimental data. Laser resonance ionisation high-resolution spectroscopy. Comparison to theoretical estimations. RISIKO mass separator at Johannes Gutenberg University Mainz.

doi: 10.1103/PhysRevC.107.034313
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2022NO01 Phys.Rev. C 105, L021302 (2022)

S.Nothhelfer, Th.E.Albrecht-Schonzart, M.Block, P.Chhetri, Ch.E.Dullmann, J.G.Ezold, V.Gadelshin, A.Gaiser, F.Giacoppo, R.Heinke, T.Kieck, N.Kneip, M.Laatiaoui, Ch.Mokry, S.Raeder, J.Runke, F.Schneider, J.M.Sperling, D.Studer, P.Thorle-Pospiech, N.Trautmann, F.Weber, K.Wendt

Nuclear structure investigations of ^253-255Es by laser spectroscopy

NUCLEAR MOMENTS ^253,254,255Es; measured hyperfine spectra; deduced J, isotope shifts, hyperfine constants, nuclear spins, magnetic dipole moments, electric quadrupole moments. Comparison with previous experimental data. Laser resonance ionization spectroscopy. RISIKO mass separator at Johannes Gutenberg University Mainz.

doi: 10.1103/PhysRevC.105.L021302
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Data from this article have been entered in the XUNDL database. For more information, click here.

2019MA53 Phys.Rev. C 100, 015803 (2019)

G.Malfatti, M.G.Orsaria, G.A.Contrera, F.Weber, I.F.Ranea-Sandoval

Hot quark matter and (proto-) neutron stars

doi: 10.1103/PhysRevC.100.015803
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2017RA28 Phys.Rev. C 96, 065807 (2017)

I.F.Ranea-Sandoval, M.G.Orsaria, S.Han, F.Weber, W.M.Spinella

Color superconductivity in compact stellar hybrid configurations

doi: 10.1103/PhysRevC.96.065807
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2016RA13 Phys.Rev. C 93, 045812 (2016)

I.F.Ranea-Sandoval, S.Han, M.G.Orsaria, G.A.Contrera, F.Weber, M.G.Alford

Constant-sound-speed parametrization for Nambu-Jona-Lasinio models of quark matter in hybrid stars

doi: 10.1103/PhysRevC.93.045812
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2016SP02 Eur.Phys.J. A 52, 61 (2016)

W.M.Spinella, F.Weber, G.A.Contrera, M.G.Orsaria

Neutrino emissivity in the quark-hadron mixed phase of neutron stars

doi: 10.1140/epja/i2016-16061-x
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2015DE31 Phys.Rev. C 92, 035810 (2015)

S.M.de Carvalho, R.Negreiros, M.Orsaria, G.A.Contrera, F.Weber, W.Spinella

Thermal evolution of hybrid stars within the framework of a nonlocal Nambu-Jona-Lasinio model

doi: 10.1103/PhysRevC.92.035810
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2014OR01 Phys.Rev. C 89, 015806 (2014)

M.Orsaria, H.Rodrigues, F.Weber, G.A.Contrera

Quark deconfinement in high-mass neutron stars

doi: 10.1103/PhysRevC.89.015806
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2012BL02 Phys.Rev. C 85, 022802 (2012)

D.Blaschke, H.Grigorian, D.N.Voskresensky, F.Weber

Cooling of the neutron star in Cassiopeia A

doi: 10.1103/PhysRevC.85.022802
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2011MA84 J.Phys.:Conf.Ser. 312, 042018 (2011)

M.Malheiro, R.P.Negreiros, F.Weber, V.Usov

The Effects of Charge On The Structure of Strange Stars

doi: 10.1088/1742-6596/312/4/042018
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2009GO19 Phys.Rev. C 80, 015804 (2009)

B.Golf, J.Hellmers, F.Weber

Impact of strange quark matter nuggets on pycnonuclear reaction rates in the crusts of neutron stars

NUCLEAR REACTIONS ¹²C(¹²C, X), ¹²C(¹⁶O, X), ¹⁶O(¹⁶O, X), ⁵⁶Fe(⁵⁶Fe, X), ¹⁰⁰Ru(¹⁰⁰Ru, X), ¹¹⁸Kr(¹¹⁸Kr, X), E not given; calculated reaction rates for one-component (OCP) and multi-component plasmas (MCP) as a function of density of matter in neutron stars.