Searcharxiv⌕ Search

arXiv subjects

S. Kondo

Publications and source records attributed to S. Kondo.

20 records · Page 2Linked to original sources

Specific Heat (1.2-108 K) and Thermal Expansion (4.4-297 K) Measurements of the 3d Heavy Fermion Compound LiV_{2}O_{4}

Specific heat C_{p}(T) measurements of the heavy fermion normal-spinel structure compound LiV_{2}O_{4} were carried out using a heat-pulse calorimeter over the temperature T range from 1.2 to 108 K. The electronic specific heat C_{e}(T) of LiV_{2}O_{4} is extracted from the C_{p}(T) data using the lattice contribution obtained for LiTi_{2}O_{4}, a superconductor with T_{c} = 11.8 K. The electronic specific heat coefficient γ(T) = C_{e}(T)/T of LiV_{2}O_{4} is found to be 0.42 and 0.43 J/mol K^2 at T = 1 K for two different high magnetic purity samples, respectively. γ(T) decreases rapidly with increasing temperature from 4 to 30 K and then decreases much more slowly from 0.13 J/mol K^2 at 30 K to 0.08 J/mol K^2 at 108 K. The C_{e}(T) is compared with theoretical predictions for the spin S = 1/2 Kondo model, a generic Fermi liquid model, and an antiferromagnetically coupled quantum-disordered metal. Each of these theories can adequately describe C_{e}(T) in the Fermi liquid regime at low (~ 1 to 10 K) temperatures, consistently yielding a large extrapolated γ(0) = 428(3) mJ/mol K^2. However, none of these theories describes C_{e}(T) from ~ 10 K to 108 K. Our C_{e}(T) data are also in severe disagreement with the magnetic specific heat of the spin S = 1/2 Heisenberg model. Thermal expansion measurements of LiV_{2}O_{4} were carried out from 4.4 to 297 K using a differential capacitance dilatometer. Strong increases in the thermal expansion coefficient and Grüneisen parameter Γare found below \~ 20 K, confirming the results of Chmaissem et al. [Phys. Rev. Lett. 79, 4866 (1997)] obtained using neutron diffraction. We estimate that Γ(0) is about 11.4.

cond-mat.str-el↗

A Search for Very High Energy Neutrinos from Active Galactic Nuclei

We report the results of a search for neutrino-induced particle cascades using a deep ocean water Cherenkov detector. The effective mass of the detector, a string of seven 40 cm diameter photomultipliers at 5.2 m spacing, is found through simulation analysis to be surprisingly large: greater than 1 megaton of water at incident neutrino energies of 1 PeV. We find no evidence for neutrino-induced cascades in 18.6 hours of observation. Although the limit implied by this observation is the strongest yet for predictions of active galatic nuclei (AGN) neutrinos at energies above 100 TeV, perhaps the more intriguing result is that the power of these techniques can be exploited to test these AGN models in a relatively short time.

astro-ph↗