site stats

Phys. rev. c 92 051301 r 2015

WebbPhys. Rev. C 91, 051301 (2015). [12] Lapoux, V. et al. Radii and binding energies in oxygen isotopes: a puzzle for nuclear forces. Phys. Rev. Lett. 117, 052501 (2016). [13] Hagen, G. … WebbNetdev Archive on lore.kernel.org help / color / mirror / Atom feed * [BUG REPORT] kernel panic in tcp_sendpage() on null pointer dereference @ 2015-04-07 22:57 Tuan Bui 2015 …

Single-particle structure of the N = 20, 28 isotones within the ...

WebbThe control of polarization state in soft and hard X-ray light is of crucial interest to probe structural and symmetry properties of matter. Thanks to their Apple-II type undulators, … play2car https://mistressmm.com

IM-SRG in nuclear physics - Personal page - GitHub Pages

Webb23 dec. 2015 · We review recent advances in the shell model Monte Carlo approach for the microscopic calculation of statistical and collective properties of nuclei. We discuss applications to the calculation of i) level densities in nickel isotopes, implementing a recent method to circumvent the odd-particle sign problem; ii) state densities in heavy nuclei; iii) … Webb23 sep. 2024 · [3] Delion D S and Dumitrescu A 2015 At. Data Nucl. Data Tables 101 1. Crossref; Google Scholar [4] Gamow G 1928 Z. Phys. 51 204. Crossref; Google Scholar … WebbPhys. Rev. C, 87 :051305, 2013. Department of Physics Contact Phone: 303.315.7390 Department Chair: Michael "Bodhi" Rogers, PhD, RPA Department Chair Email: … play 2 boulogne

High-spin structures of 77,79,81,83 As isotopes - Academia.edu

Category:From EFTs to Nuclei

Tags:Phys. rev. c 92 051301 r 2015

Phys. rev. c 92 051301 r 2015

IM-SRG in nuclear physics - Personal page - GitHub Pages

Webb1 maj 2015 · Phys. Rev. C 91, 051301 (R) (2015) - Accurate nuclear radii and binding energies from a chiral interaction Rapid Communication Accurate nuclear radii and … WebbFavored Authors. We offer real benefits to our authors, including fast-track processing of papers. Learn more

Phys. rev. c 92 051301 r 2015

Did you know?

Webb\documentstyle{article} \textheight= 23 cm \textwidth= 15 cm \topmargin=0cm \oddsidemargin=0truecm \evensidemargin=0truecm %\pagestyle{empty} … WebbHagen et al., Nature Physics 12, 186–190 (2016) What is the size of the atomic nucleus? Significantly smaller skins were obtained. Circle from NNLOsat chiral interaction, …

WebbJ. Simonis [email protected] Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany K. Hebeler [email protected] Institut für Kernphysik, Technische … Webb12 apr. 2024 · In addition to advancing the DM-electron scattering rate calculations, in Refs. [10], [68] we expanded the calculation of DM-electron absorption. In targets with …

Webb7 juli 2016 · At the Radioactive Isotope Beam Factory stable primary beams are accelerated up to 345 MeV/u and incident on a primary target to produce cocktail secondary beams with the fragment separator BigRIPS ranging from the lightest nuclei up to the lead region. For in-beam γ-ray spectroscopy, the secondary beams impinge on a … Webb2 sep. 2024 · In the present work, the $$\\mathcal {\\alpha }$$ α decay half-lives for even-even polonium–uranium nuclei, including three isotopes $$^{214-218}$$ 214 - 218 U Zhang et al. (in Phys Rev Lett 126:152502, 2024), are studied within the generalized liquid drop model with the total $$\\mathcal {\\alpha }$$ α decay energy-dependent $$\\mathcal …

Webb5 feb. 2024 · [18] Chowdhury P R, Samanta C and Basu D N 2008 Phys. Rev. C 77 044603. Go to reference in article Crossref Google Scholar [19] Santhosh K P, Sahadevan S and …

Webb4 sep. 2024 · The virial stress tensor-based instantaneous heat flux, which is used by LAMMPS, is only valid for the small subset of simulations that contain only pairwise interactions. For systems that contain many-body interactions using 3- or 4-body potentials, a more complete derivation is required. primarily substantive approachWebb6 apr. 2024 · An analysis of the astrophysical S factor of the proton-proton weak capture (p+p→H2+e⁺+νe) is performed on a large energy range covering solar-core and early Universe temperatures. The measurement... primarily subjectiveWebb3 dec. 2024 · In our previous work [Surblys et al., Phys. Rev. E 99, 051301 (R) (2024)], we have demonstrated that atomic stress could be used to efficiently compute heat flux for … play2go in download