Showing 1–20 of 27 results
/ Date/ Name
Mar 23, 2004Field dependence of the zero energy density of states around vortices in an anisotropic gap superconductorJul 1, 1999A 4% Geometric Distance to the Galaxy NGC4258 from Orbital Motions in a Nuclear Gas DiskApr 13, 2006Specific heat and low-lying excitations in the mixed state for a type II superconductorJun 22, 2006CO emission from candidate photo-dissociation regions in M81Oct 10, 2014Multi-molecule ALMA observations towards the Seyfert 1 galaxy NGC 1097Aug 20, 2009Direct Numerical Confirmation of Pinning Induced Sign Change in Superconducting Hall Effect in Type-II SuperconductorsJun 30, 2008LDA + Negative U Solves a Puzzle of too Large Calculated Magnetic Moment in Iron-based Superconductor LaFeAsO_{1-x}F_xFeb 20, 1998VLBA Continuum Observations of NGC 4258: Constraints on an Advection-Dominated Accretion FlowJan 14, 2004Radio Observations of the Afterglow of GRB 030329May 12, 2002Reentrant vortex lattice transformation in four-fold symmetric superconductorsMay 13, 2014Magnetic field distribution and characteristic fields of the vortex lattice for a clean superconducting niobium sample in an external field applied along a three-fold axisSep 9, 2004Carbon-substitution dependent multiple superconducting gap of MgB$_{2}$: a "sub-meV" resolution photoemission studyNov 19, 2013Influence of Shear Motion on Evolution of Molecular Clouds in the Spiral Galaxy M51Oct 23, 2011Effect of Born and unitary impurity scattering on the Kramer-Pesch shrinkage of a vortex core in an s-wave superconductorSep 7, 2009First-principles-based $\pm s$-wave modelling for iron-based superconductors:Studies for specific heat and nuclear magnetic relaxation rateJun 4, 2002Dense Molecular Gas in Lenticular GalaxiesSep 3, 1997New upper limits on the interstellar O2 abundanceSep 14, 2004How to detect gap nodes of a superconductor by angle-resolved specific heat experiment?Jun 3, 2011On the absence of molecular absorption in high redshift millimetre-band searchesSep 14, 1995Molecular gas observations and enhanced massive star formation efficiencies in M100