JINA - Virtual Journal of Nuclear Astrophysics, 16 November 2018
Volume 16, Issue 46 (27 Articles)
- # 1 - A Volume-Limited Survey of mCP Stars Within 100pc I: Fundamental Parameters and Chemical Abundances. (arXiv:1811.05633v1 [astro-ph.SR])
- # 2 - Initial Mass Function Variations Cannot Explain the Ionizing Spectrum of Low Metallicity Starbursts. (arXiv:1811.03856v1 [astro-ph.GA])
- # 3 - Masses, Oxygen and Carbon abundances in CHEPS dwarf stars. (arXiv:1811.05011v1 [astro-ph.SR])
- # 4 - Nuclear Kinetic Equilibrium During Big Bang Nucleosynthesis. (arXiv:1811.04932v1 [hep-ph])
- # 5 - On the importance of progenitor asymmetry to shock revival in core-collapse supernovae. (arXiv:1811.05515v1 [astro-ph.HE])
- # 6 - Progenitor constraints on the Type Ia supernova SN 2014J from Hubble Space Telescope H$beta$ and [O III] observations. (arXiv:1811.04944v1 [astro-ph.HE])
- # 7 - Spectral lines in the CaII triplet region for RAVE DR6 chemical abundance pipeline. (arXiv:1811.05365v1 [astro-ph.SR])
- # 8 - The "Fundamental Metallicity Relation" in CALIFA, SDSS-IV MaNGA and high-z galaxies. (arXiv:1811.06015v1 [astro-ph.GA])
- # 9 - The trajectories of galaxies in groups: mass loss and preprocessing. (arXiv:1811.06530v1 [astro-ph.GA])
- # 10 - Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors. (arXiv:1811.05483v1 [astro-ph.SR])
- # 11 - Astrophysical $S_{E2}$ factor of the ${}^{12}mathrm{C}(alpha,gamma){}^{16}mathrm{O}$ reaction through the ${}^{12}mathrm{C}({}^{11}mathrm{B},{}^{7}mathrm{Li}){}^{16}mathrm{O}$ transfer reaction. (arXiv:1811.06220v1 [nucl-ex])
- # 12 - Understanding the energy resolution of liquid argon neutrino detectors. (arXiv:1811.06159v1 [hep-ph])
- # 13 - New Results for the p7Be-->8Bgamma Astrophysical S-factor from 10 keV to 5 MeV and Reactions Rate from 0.01 to 10 T9. (arXiv:1811.03737v1 [nucl-th])
- # 14 - Turbulence in the Accretion Disks in Semi-Detached Binary Systems with Various Component-Mass Ratios
- # 15 - Partial cross section of neutron-induced reactions on 136 Xe at E n = 5 MeV for 0 νββ background
studies
- Journal of Physics G: Nuclear and Particle Physics
- http://iopscience.iop.org/0954-3899/45/12/125101
- # 16 - Photobombing stars lead to cosmic false identity
- Photobombing stars lead to cosmic false identity
- https://www.nature.com/articles/d41586-018-07413-x
- # 17 - Noise sources and their limitations on the performance of compound semiconductor hard radiation detectors
- # 18 - $β$-decay half-lives of $^{134,134m}mathrm{Sb}$ and their isomeric yield ratio produced by the spontaneous fission of $^{252}mathrm{Cf}$
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.98.054307
- # 19 - First limit on neutrinoless quadruple $β$ decay of $^{150}mathrm{Nd}$ to the ${0}_{1}^{+}$ state of $^{150}mathrm{Gd}$
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.98.055501
- # 20 - Gravitational waves and mass ejecta from binary neutron star mergers: Effect of large eccentricities
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.98.104005
- # 21 - Heavy sterile neutrinos in stellar core-collapse
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.98.103010
- # 22 - Tracking Black Hole Kicks from Gravitational-Wave Observations
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.121.191102
- # 23 - Lifetime measurement of the state in 74Rb and isospin properties of quadrupole transition strengths at N = Z
- # 24 - Large galaxy found lurking on the Milky Way's far side
- # 25 - Collisions of Neutron Stars with Primordial Black Holes as Fast Radio Bursts Engines
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/868/1/17
- # 26 - Don’t Blink: Constraining the Circumstellar Environment of the Interacting Type Ia Supernova 2015cp
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/868/1/21
- # 27 - Electrical resistivity and Hall effect in binary neutron star mergers
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.

