Thompson Scattering in an Expanding Universe
The Thompson cross section for scattering of electromagnetic waves by a free electron in an expanding universe is derived here.
103 indexed results
The Thompson cross section for scattering of electromagnetic waves by a free electron in an expanding universe is derived here.
In this work we apply Thompson's method (of the dimensions) to study the quantum electrodynamics (QED). This method can be
A counterexample is given to the uniqueness result given in the paper by J.Cox and K.Thompson, "Note on the uniqueness
In this work we propose an action to describe diffusion limited chemical reactions belonging to various classes of universality. This
In these lecture notes we explain a connection between Yang-Mills theory on arbitrary Riemann surfaces and two types of topological
The preliminary results of a 1996 multisite campaign on the pulsating lambda Bootis star 29 Cyg are presented. This campaign,
We present infrared interferometric angular size measurements for the A7IV-V star Altair which indicate a non-circular projected disk brightness distribution.
The Milagrito water Cherenkov detector in the Jemez Mountains near Los Alamos, New Mexico took data from February 1997 to
We present submm images of Sgr A* and its surroundings obtained at 800, 600 and 450 $μ$m with the JCMT
CeRhIn5 is a heavy fermion antiferromagnet that orders at 3.8 K. The observation of pressure-induced superconductivity in CeRhIn5 at a
The Gamma-ray Large Area Space Telescope (GLAST) is now being designed by a number of collaborating institutions. It will study
We present neutron diffraction, magnetic susceptibility and specific heat data for a single-crystal sample of the cubic (Cu3Au structure) compound
We present the results of a photometric survey for variable stars in the nearby globular cluster M5. A 14.8x22.8 arcmin^2
The oscillation spectra of solar-type stars may in the not-too- distant future be used to constrain certain properties of the
I summarize the recent advances in our understanding of the Soft Gamma Repeaters: in particular their spin behavior, persistent emission
The Relativistic Heavy Ion Collider (RHIC) will experience increasing longitudinal and transverse heavy ion emittances, mostly due to intra-beam scattering
We present the preliminary results of a sub-mm imaging survey of ultracompact HII regions, conducted with the SCUBA bolometer array
The success of the Hubble Deep Field (HDF) data in identifying galaxies at redshifts up to ~3 has been quite
The Milagro detector is an air shower array which uses the water Cherenkov technique and is capable of continuously monitoring
The rate of the beta decay of neutral kaons is calculated within the meson dominance approach taking into account the
The EGRET telescope aboard NASAs Compton GRO has repeatedly detected 3EG J1835+5918, a bright and steady source of high-energy gamma-ray
The National Fusion Collaboratory (NFC) project was created to advance scientific understanding and innovation in magnetic fusion research by enabling
We present the results of a narrowband search for forming galaxies at high redshifts. Given the coverage of 276 square
Bulk polycrystalline HgBa(2)Ca(2)Cu(3)O(x) materials were irradiated with 0.8 GeV protons to form randomly oriented columnar defects, by induced fission of