1.5k citations
- Oak Ridge National LaboratoryUS11 papers
- Center for Astrophysics Harvard & SmithsonianUS8 papers
- Forschungszentrum JülichDE8 papers
- Triangle Universities Nuclear LaboratoryUS8 papers
- Goddard Space Flight CenterUS7 papers
- Kyungpook National UniversityKR7 papers
- University of California, BerkeleyUS7 papers
- Harvard UniversityUS6 papers
- Stanford UniversityUS6 papers
- Thomas Jefferson National Accelerator FacilityUS6 papers
- University of OsloNO6 papers
- Florida Atlantic UniversityUS5 papers
62 papers · 1 filter
Goldstone boson currents in a kaon condensed CFL phase
Andreas Gerhold, Thomas Schaefer, Andrei Kryjevski
We study the stability of the kaon condensed color-flavor locked (CFL) phase of dense quark matter with regard to the formation of a non-zero Goldstone boson current. In the kaon c…
Elastic Spin Relaxation Processes in Semiconductor Quantum Dots
Y. G. Semenov, K. W. Kim
Electron spin decoherence caused by elastic spin-phonon processes is investigated comprehensively in a zero-dimensional environment. Specifically, a theoretical treatment is develo…
Origin of charge density at LaAlO3-on-SrTiO3 hetero-interfaces; possibility of intrinsic doping
Wolter Siemons, Gertjan Koster, Hideki Yamamoto +5
As discovered by Ohtomo et al., a large sheet charge density with high mobility exists at the interface between SrTiO3 and LaAlO3. Based on transport, spectroscopic and oxygen-anne…
Lattice Simulations for Light Nuclei: Chiral Effective Field Theory at Leading Order
Bugra Borasoy, Evgeny Epelbaum, Hermann Krebs +2
We discuss lattice simulations of light nuclei at leading order in chiral effective field theory. Using lattice pion fields and auxiliary fields, we include the physics of instanta…
Linear growth of spiral SASI modes in core-collapse supernovae
John M. Blondin, Samantha Shaw
Two-dimensional axisymmetric simulations have shown that the post-bounce accretion shock in core collapse supernovae is subject to the Spherical Accretion Shock Instability, or SAS…
Pulsar spins from an instability in the accretion shock of supernovae
John M. Blondin, Anthony Mezzacappa
Rotation-powered radio pulsars are born with inferred initial rotation periods of order 300 ms (some as short as 20 ms) in core-collapse supernovae. In the traditional picture, thi…