scholarly journals Tagged High-Energy $\bar{n}$, Hyperon and anti-Hyperon Beams at NAL

1968 ◽  
Author(s):  
D. Cline
Keyword(s):  
High Energy ◽  
Energy Bar

Charged hadron multiplicities in high energy $$\bar v_\mu n$$ and $$\bar v_\mu p$$ interactions

1982 ◽  
Vol 11 (4) ◽  
pp. 283-292 ◽  
Author(s):  
◽  
S. Barlag ◽  
P. Dam ◽  
E. Wolf ◽  
B. Jongejans ◽  
...  
Keyword(s):  
High Energy ◽  
Charged Hadron ◽  
Energy Bar

High-Energy bar pp and pp Elastic Scattering and Nucleon Structure

1987 ◽  
Vol 4 (2) ◽  
pp. 189-196 ◽  
Author(s):  
M. M Islam ◽  
V Innocente ◽  
T Fearnley ◽  
G Sanguinetti
Keyword(s):  
Elastic Scattering ◽  
High Energy ◽  
Nucleon Structure ◽  
Energy Bar

OddC exchange in high-energy $$\bar pp$$ andpp scattering

1987 ◽  
Vol 36 (3) ◽  
pp. 495-502 ◽  
Author(s):  
L. L. Jenkovszky ◽  
A. N. Shelkovenko ◽  
B. V. Struminsky
Keyword(s):  
High Energy ◽  
Energy Bar

scholarly journals Charged hadron multiplicities in high energy $$\bar v_\mu n$$ and $$\bar v_\mu p$$ interactions

1982 ◽  
Vol 14 (3) ◽  
pp. 281-281 ◽  
Author(s):  
S. Barlag ◽  
P. Dam ◽  
E. Wolf ◽  
B. Jongejans ◽  
A. Tenner ◽  
...  
Keyword(s):  
High Energy ◽  
Charged Hadron ◽  
Energy Bar

A HYPOTHETICAL, ATTRACTIVE LONG-RANGE FORCE FROM TWO-GLUON EXCHANGE, AND THE MEASUREMENT OF ρ IN HIGH ENERGY $\bar p p$ ELASTIC SCATTERING

1994 ◽  
Vol 09 (20) ◽  
pp. 1835-1844 ◽  
Author(s):  
S. BARSHAY ◽  
J.A. GRIFOLS ◽  
S. TORTOSA
Keyword(s):  
Elastic Scattering ◽  
Long Range ◽  
Scattering Amplitude ◽  
High Energy ◽  
Small Momentum ◽  
Energy Formula ◽  
Nuclear Amplitude ◽  
Energy Bar ◽  
Coulomb Amplitude ◽  
Range Force

The dynamical question is raised of the possible existence of long-range, residual attractive forces between hadrons due to the overall color-neutral exchange of two, massless transverse gluons between their constituents. Such a force between fermionic constituents would behave as 1/R6. We discuss the experiments which measure the real part of the nuclear amplitude, through its interference with the Coulomb amplitude in high energy [Formula: see text] elastic scattering at very small momentum transfers. We show that on-going [Formula: see text] experiments at [Formula: see text] and at 1800 GeV are sensitive to the scattering amplitude from a residual long-range force.

The E-ring: interactions with plasma and implications for its evolution

1984 ◽  
Vol 75 ◽  
pp. 599-602
Author(s):  
T.V. Johnson ◽  
G.E. Morfill ◽  
E. Grun
Keyword(s):  
Time Scale ◽  
Particle Density ◽  
High Energy ◽  
Particle Removal ◽  
Density Region ◽  
Drag Forces ◽  
Orbit Evolution ◽  
History Of ◽  
Ring Particle ◽  
Ring Material

A number of lines of evidence suggest that the particles making up the E-ring are small, on the order of a few microns or less in size (Terrile and Tokunaga, 1980, BAAS; Pang et al., 1982 Saturn meeting; Tucson, AZ). This suggests that a variety of electromagnetic and plasma affects may be important in considering the history of such particles. We have shown (Morfill et al., 1982, J. Geophys. Res., in press) that plasma drags forces from the corotating plasma will rapidly evolve E-ring particle orbits to increasing distance from Saturn until a point is reached where radiation drag forces acting to decrease orbital radius balance this outward acceleration. This occurs at approximately Rhea's orbit, although the exact value is subject to many uncertainties. The time scale for plasma drag to move particles from Enceladus' orbit to the outer E-ring is ~104yr. A variety of effects also act to remove particles, primarily sputtering by both high energy charged particles (Cheng et al., 1982, J. Geophys. Res., in press) and corotating plasma (Morfill et al., 1982). The time scale for sputtering away one micron particles is also short, 102 - 10 yrs. Thus the detailed particle density profile in the E-ring is set by a competition between orbit evolution and particle removal. The high density region near Enceladus' orbit may result from the sputtering yeild of corotating ions being less than unity at this radius (e.g. Eviatar et al., 1982, Saturn meeting). In any case, an active source of E-ring material is required if the feature is not very ephemeral - Enceladus itself, with its geologically recent surface, appears still to be the best candidate for the ultimate source of E-ring material.

Analysis of electron-diffraction intensity profiles using a photodiode-array detection system

1983 ◽  
Vol 41 ◽  
pp. 322-323
Author(s):  
J. B. Warren
Keyword(s):  
Electron Diffraction ◽  
Diffraction Pattern ◽  
Detection System ◽  
High Energy ◽  
Photographic Emulsion ◽  
Diffraction Intensity ◽  
Silicon Photodiode ◽  
Photodiode Array Detection ◽  
Analog To Digital ◽  
Photodiode Array

Electron diffraction intensity profiles have been used extensively in studies of polycrystalline and amorphous thin films. In previous work, diffraction intensity profiles were quantitized either by mechanically scanning the photographic emulsion with a densitometer or by using deflection coils to scan the diffraction pattern over a stationary detector. Such methods tend to be slow, and the intensities must still be converted from analog to digital form for quantitative analysis. The Instrumentation Division at Brookhaven has designed and constructed a electron diffractometer, based on a silicon photodiode array, that overcomes these disadvantages. The instrument is compact (Fig. 1), can be used with any unmodified electron microscope, and acquires the data in a form immediately accessible by microcomputer.Major components include a RETICON 1024 element photodiode array for the de tector, an Analog Devices MAS-1202 analog digital converter and a Digital Equipment LSI 11/2 microcomputer. The photodiode array cannot detect high energy electrons without damage so an f/1.4 lens is used to focus the phosphor screen image of the diffraction pattern on to the photodiode array.

Observation of Superlattice Dislocations on Cube Planes in Ni3Al

1973 ◽  
Vol 31 ◽  
pp. 174-175 ◽  
Author(s):  
J. M. Oblak ◽  
W. H. Rand
Keyword(s):  
Nearest Neighbor ◽  
Antiphase Boundary ◽  
Nearest Neighbors ◽  
High Energy ◽  
Cross Slip ◽  
Octahedral Plane ◽  
Trapping Mechanism ◽  
Slip Traces

The energy of an a/2 <110> shear antiphase. boundary in the Ll2 expected to be at a minimum on {100} cube planes because here strue ture is there is no violation of nearest-neighbor order. The latter however does involve the disruption of second nearest neighbors. It has been suggested that cross slip of paired a/2 <110> dislocations from octahedral onto cube planes is an important dislocation trapping mechanism in Ni3Al; furthermore, slip traces consistent with cube slip are observed above 920°K.Due to the high energy of the {111} antiphase boundary (> 200 mJ/m2), paired a/2 <110> dislocations are tightly constricted on the octahedral plane and cannot be individually resolved.

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