CHANDRA Observations of X-ray Jet Structure on kpc to Mpc Scales

With its exquisite spatial resolution of better than 0.5 arcsecond, the Chandra observatory is uniquely capable of resolving and studying the spatial structure of extragalactic X-ray jets on scales of a few to a few hundred kilo-parsec. Our analyses of four recent Chandra images of quasar jets interpret the X-ray emission as inverse Compton scattering of high energy electrons on the cosmic microwave background. We infer that these jets are in bulk relativistic motion, carrying kinetic powers upwards of 10^46 ergs/s to distances of hundreds of kpc, with very high efficiency.Comment: 4 pages, 3 figures, to be published in the proceedings of the Bologna jet workshop, "The Physics of Relativistic Jets in the CHANDRA and XMM Era.

Isospin Response of the 4-He Continuum

This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440

Study of Dipole Resonance Strength in 12-C via the Reactions 12-C(pol.p,p'c)

This research was sponsored by the National Science Foundation Grant NSF PHY-931478

Diffraction Symmetry in Crystalline, Close-Packed C60

We have grown crystals of the carbon structure C60 by sublimation. In contrast to solution-grown crystals, the sublimed crystals have long range order with no evidence of solvent inclusions. Sublimed C60 forms three dimensional, faceted crystals with a close-packed, face-centered cubic unit cell. We have refined a crystal structure using the "soccer ball" model of the C60 molecule. The results indicate that the C60 molecule has the expected spherical shape, however the data are not sufficiently accurate to unambiguously determine atomic positions

Isospin Response of the 4-He Continuum

This research was sponsored by the National Science Foundation Grant NSF PHY-931478

Mott Transition in Degenerate Hubbard Models: Application to Doped Fullerenes

The Mott-Hubbard transition is studied for a Hubbard model with orbital degeneracy N, using a diffusion Monte-Carlo method. Based on general arguments, we conjecture that the Mott-Hubbard transition takes place for U/W \propto \sqrt{N}, where U is the Coulomb interaction and W is the band width. This is supported by exact diagonalization and Monte-Carlo calculations. Realistic parameters for the doped fullerenes lead to the conclusion that stoichiometric A_3 C_60 (A=K, Rb) are near the Mott-Hubbard transition, in a correlated metallic state.Comment: 4 pages, revtex, 1 eps figure included, to be published in Phys.Rev.B Rapid Com

Structural and electronic properties of (NH3)xK3C60

We have investigated the synthesis, structure, and electronic properties of (NH3)xK3C60 by exposing preformed K3C60 to NH3 vapor. Measurements were made on bulk powders and films with a variety of techniques including in-situ x-ray diffraction and monitoring of NH3 pressure, Raman scattering and ac susceptibility. The reaction of NH3 with K3C60 is completely reversible and leaves the (C60)3- charge state intact, while allowing the distance between the C60 molecules to vary. We observe two different crystallographic structures at x=1 and x=8-10. The x=1 structure is face-centered orthorhombic with a single NH3 on the octahedral interstitial site. It is single phase at 100°C and NH3 pressures 400 torr and remains single phase at 0 torr if the temperature is reduced to 25°C. Although (NH3)K3C60 exhibits no superconductivity at ambient pressure, superconductivity can be induced by hydrostatic pressure with an onset at 28 K. The details of the x=8-10 structure are uncertain, however it appears that this phase is body-centered tetragonal with NH3 on both the octahedral and tetrahedral sites. It occurs at room temperature and NH3 pressures 500 torr, but is not stable at lower NH3 pressures. Resistivity measurements of NH3-doped K3C60 films show that the formation of the new structure results in a rapid increase of the resistivity to values exceeding 1 cm