12,984 research outputs found
SCR Blocking Pulse Gate Amplifier-Patent
Silicon controlled rectifier pulse gate amplifier for blocking false gating caused by negative transient voltage
The nuclear matter equation of state with consistent two- and three-body perturbative chiral interactions
We compute the energy per particle of infinite symmetric nuclear matter from
chiral N3LO (next-to-next-to-next-to-leading order) two-body potentials plus
N2LO three-body forces. The low-energy constants of the chiral three-nucleon
force that cannot be constrained by two-body observables are fitted to
reproduce the triton binding energy and the 3H-3He Gamow-Teller transition
matrix element. In this way, the saturation properties of nuclear matter are
reproduced in a parameter-free approach. The equation of state is computed up
to third order in many-body perturbation theory, with special emphasis on the
role of the third-order particle-hole diagram. The dependence of these results
on the cutoff scale and regulator function is studied. We find that the
inclusion of three-nucleon forces consistent with the applied two-nucleon
interaction leads to a reduced dependence on the choice of the regulator only
for lower values of the cutoff.Comment: 9 pages, 12 figures, 3 tables, to be published in Physical Review C.
arXiv admin note: text overlap with arXiv:1209.553
MOXE: An X-ray all-sky monitor for Soviet Spectrum-X-Gamma Mission
A Monitoring Monitoring X-Ray Equipment (MOXE) is being developed for the Soviet Spectrum-X-Gamma Mission. MOXE is an X-ray all-sky monitor based on array of pinhole cameras, to be provided via a collaboration between Goddard Space Flight Center and Los Alamos National Laboratory. The objectives are to alert other observers on Spectrum-X-Gamma and other platforms of interesting transient activity, and to synoptically monitor the X-ray sky and study long-term changes in X-ray binaries. MOXE will be sensitive to sources as faint as 2 milliCrab (5 sigma) in 1 day, and cover the 2 to 20 KeV band
THE DEVELOPMENT OF MULTIPLE LINEAR REGRESSION EQUATIONS TO PREDICT ACCURACY IN BASKETBALL JUMP SHOOTING
Chiral nucleon-nucleon forces in nuclear structure calculations
Realistic nuclear potentials, derived within chiral perturbation theory, are
a major breakthrough in modern nuclear structure theory, since they provide a
direct link between nuclear physics and its underlying theory, namely the QCD.
As a matter of fact, chiral potentials are tailored on the low-energy regime of
nuclear structure physics, and chiral perturbation theory provides on the same
footing two-nucleon forces as well as many-body ones. This feature fits well
with modern advances in ab-initio methods and realistic shell-model. Here, we
will review recent nuclear structure calculations, based on realistic chiral
potentials, for both finite nuclei and infinite nuclear matter.Comment: 10 pages, 8 figures, plenary talk presented at "Nucleus-Nucleus 2015"
Conference, 21-26 June 2015, Catania, to be published in the "Conference
Proceedings" Series of the Italian Physical Societ
Long-term studies with the Ariel 5 ASM. 2: The strong Cygnus sources
The three bright 3-6 keV X-ray sources in Cygnus are examined for regular temporal variability with a 1300-day record from the Ariel 5 All Sky Monitor. The only periods consistently observed are 5.6 days for Cyg X-1, 11.23 days for Cyg X-2, and 4.8 hours for Cyg X-3
Recurrent X-ray outbursts from Aquila X-1
Aquila X-1 observations by the All Sky Monitor on Ariel 5 are presented. Data is compared with that obtained by rocket survey, and by the Uhuru, OSO 7, and OAO 3 satellites. The variability of brightness is discussed as a connection between dwarf novae and long term transient X ray sources
Satellite material contaminant optical properties
The Air Force Wright Research and Development Center and the Arnold Engineering Development Center are continuing a program for measuring optical effects of satellite material outgassing products on cryo-optic surfaces. Presented here are infrared (4000 to 700 cm(-1)) transmittance data for contaminant films condensed on a 77 K geranium window. From the transmittance data, the contaminant film refractive and absorptive indices (n, k) were derived using an analytical thin-film interference model with a nonlinear least-squares algorithm. To date 19 materials have been studied with the optical contents determined for 13 of those. The materials include adhesives, paints, composites, films, and lubricants. This program is continuing and properties for other materials will be available in the future
Evidence for a 16d.6 period from Circinus X-1
Analysis of All-Sky Monitor observations of Cir X-1 (3U1516-56) over the period October 1975 - April 1976 revealed a well-defined modulation of the 3-6 keV flux at a period of 16.585 + or - 0.01. The light-curve is characterized by an abrupt drop in emission occurring on a timescale of 0.07, with epoch JD 2,442,877.181 + or - 0.07. No clear correspondingly sharp increase in emission is observed during the cycle, so that a noneclipse origin for this effect cannot be ruled out
Long-term X-ray studies of Sco X-1
No modulation of the 3-6 keV X-ray intensity of Sco X-1 at a level of excess of 1% was observed at the optical period of .787313d. Evidence is found for shot-noise character in a large fraction of the X-ray emission. Almost all of the Sco X-1 emission can be synthesized in terms of approximately 200 shots per day, each with a duration of approximately 1/3 day. A pinhole camera was used to obtain data and the data were statistically analyzed
- …