JINA - Virtual Journal of Nuclear Astrophysics, 8 June 2018
Volume 16, Issue 23 (17 Articles)
- # 1 - An efficient method for determining the chemical evolution of gravitationally collapsing prestellar cores. (arXiv:1806.01699v1 [astro-ph.GA])
- # 2 - Big Bang Nucleosynthesis Constraint on Baryonic Isocurvature Perturbations. (arXiv:1806.00123v1 [astro-ph.CO])
- # 3 - Core collapse with magnetic fields and rotation. (arXiv:1806.00393v1 [astro-ph.HE])
- # 4 - Evolution of Highly Eccentric Binary Neutron Stars Including Tidal Effects. (arXiv:1806.00158v1 [gr-qc])
- # 5 - Stellar models with calibrated convection and temperature stratification from 3D hydrodynamics simulations. (arXiv:1806.00020v1 [astro-ph.SR])
- # 6 - Systematic investigation of the fallback accretion powered model for hydrogen-poor superluminous supernovae. (arXiv:1806.00090v1 [astro-ph.HE])
- # 7 - The structure of detonation waves in supernovae revisited. (arXiv:1806.01286v1 [astro-ph.HE])
- # 8 - unyt: Handle, manipulate, and convert data with units in Python. (arXiv:1806.02417v1 [astro-ph.IM])
- # 9 - Revised Cross Section of the $^{13}$C($alpha$,n)$^{16}$O reaction between 5 and 8 MeV. (arXiv:1806.02722v1 [nucl-ex])
- # 10 - Study of 12C(p,p',gamma)12C reaction. (arXiv:1806.02126v1 [nucl-ex])
- # 11 - The Focal plane Detector Package on the TUNL Split-pole Spectrograph. (arXiv:1806.02401v1 [physics.ins-det])
- # 12 - Study of Possibilities of Simulating the Processes of Asymmetric Explosion and Expansion of Supernovae in a Laser Experiment
- # 13 - Stellar populations dominated by massive stars in dusty starburst galaxies across cosmic time
- Stellar populations dominated by massive stars in dusty starburst galaxies across cosmic time
- https://www.nature.com/articles/s41586-018-0196-x
- # 14 - Determination of $^{20}mathrm{Ne}(p,γ)^{21}mathrm{Na}$ cross sections from ${E}_{p}=500−2000phantom{rule{0.16em}{0ex}}mathrm{keV}$
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.97.065802
- # 15 - Trojan horse measurement of the $^{10}mathrm{B}(p,{α}_{0})^{7}mathrm{Be}$ cross section in the energy range from 3 keV to 2.2 MeV
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.97.065801
- # 16 - Precision Mass Measurements of $^{58–63}mathrm{Cr}$: Nuclear Collectivity Towards the $N=40$ Island of Inversion
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.120.232501
- # 17 - Test measurement of 7 Be(p, $gamma$ γ ) 8 B with the recoil mass separator ERNA