activity
19992008
most citedFlux pinning and phase separation in oxygen rich La2-xSrxCuO4+y system

8 citations · 8 across the 2 of their papers we have counts for

collaborators

6 papers

cond-mat.supr-con20088 cited

Flux pinning and phase separation in oxygen rich La2-xSrxCuO4+y system

Hashini E. Mohottala, B. O. Wells, J. I. Budnick +3

We have studied the magnetic characteristics of a series of super-oxygenated La2-xSrxCuO4+y samples. As shown in previous work, these samples spontaneously phase separate into an o…

astro-ph2007

Toward a galaxian luminosity-metallicity relation spanning ten magnitudes

Ivo Saviane, Fabio Bresolin, John Salzer

We describe the two projects by which we are assembling a database of near-IR luminosities and direct oxygen abundances for both high- and low-mass star-forming galaxies in the nea…

physics.atom-ph2004

Measurement method for the nuclear anapole moment of laser trapped alkali atoms

E. Gomez, S. Aubin, G. D. Sprouse +2

Weak interactions within a nucleus generate a nuclear spin dependent parity violating electromagnetic moment; the anapole moment. In heavy nuclei, the anapole moment is the dominan…

physics.comp-ph2002

An accurate spectral method for solving the Schroedinger equation

G. H. Rawitscher, I. Koltracht

The solution of the Lippman-Schwinger (L-S) integral equation is equivalent to the the solution of the Schroedinger equation. A new numerical algorithm for solving the L-S equation…

astro-ph2001

A Planet Candidate in the Stellar Triple System HD178911

S. Zucker, D. Naef, D. W. Latham +9

We report the detection of a low-mass companion orbiting the solar-type star HD178911B, the distant component of the stellar triple system HD178911. The variability of HD178911B wa…

astro-ph1999

X-ray/TeV-gamma-ray observations of several strong flares of Mkn 501 during 1997 and implications

H. Krawczynski, P. S. Coppi, T. Maccarone +1

During more than 6 months in 1997, the BL Lac object Mkn 501 was in an exceptionally bright state, both in the X-ray band and in the Very High Energy (VHE) band. In this paper we p…