One-dimensional finite motion of a particle in the field of a weak gravitational wave

1997 ◽  
Vol 40 (8) ◽  
pp. 717-720
Author(s):  
V. I. Babetskii ◽  
G. N. Izmailov
Keyword(s):  
Gravitational Wave ◽  
One Dimensional ◽  
Finite Motion ◽  
Weak Gravitational Wave

Weak Gravitational Wave and Casimir Energy of a Scalar Field

2016 ◽  
Vol 55 (9) ◽  
pp. 4100-4108
Author(s):  
F. Tavakoli ◽  
R. Pirmoradian ◽  
I. Parsabod
Keyword(s):  
Scalar Field ◽  
Gravitational Wave ◽  
Casimir Energy ◽  
Weak Gravitational Wave

scholarly journals Deviation and precession effects in the field of a weak gravitational wave

2017 ◽  
Vol 95 (10) ◽  
Author(s):  
Donato Bini ◽  
Andrea Geralico ◽  
Antonello Ortolan
Keyword(s):  
Gravitational Wave ◽  
Weak Gravitational Wave

scholarly journals COSMIC SUPERSTRINGS REVISITED

2005 ◽  
Vol 20 (15) ◽  
pp. 3413-3415 ◽  
Author(s):  
JOSEPH POLCHINSKI
Keyword(s):  
Gauge Theory ◽  
Gravitational Wave ◽  
Early Universe ◽  
Cosmic Strings ◽  
One Dimensional ◽  
Network Properties

It is possible that superstrings, as well as other one-dimensional branes, could have been produced in the early universe and then expanded to cosmic size today. I discuss the conditions under which this will occur, and the signatures of these strings. Such cosmic superstrings could be the brightest objects visible in gravitational wave astronomy, and might be distinguishable from gauge theory cosmic strings by their network properties.

A one-dimensional self-gravitating stellar gas

1966 ◽  
Vol 25 ◽  
pp. 46-48 ◽  
Author(s):  
M. Lecar
Keyword(s):  
Gravitational Field ◽  
Phase Space ◽  
Motion Picture ◽  
Space Distribution ◽  
Two Dimensional ◽  
One Dimensional ◽  
Phase Space Distribution ◽  
Dimensional Phase Space ◽  
The Mean

“Dynamical mixing”, i.e. relaxation of a stellar phase space distribution through interaction with the mean gravitational field, is numerically investigated for a one-dimensional self-gravitating stellar gas. Qualitative results are presented in the form of a motion picture of the flow of phase points (representing homogeneous slabs of stars) in two-dimensional phase space.

Electron-Mirror Microscopic Aspects of Ferroelectric Domains of BaTiO3 And Ca2Sr (C2H5CO2)6

1970 ◽  
Vol 28 ◽  
pp. 478-479
Author(s):  
Teruo Someya ◽  
Jinzo Kobayashi
Keyword(s):  
Surface Layer ◽  
Electric Fields ◽  
Quantitative Study ◽  
Recent Progress ◽  
Ferroelectric Domain ◽  
Resolving Power ◽  
Surface Pattern ◽  
Crystal Surfaces ◽  
One Dimensional ◽  
Ferroelectric Domains

Recent progress in the electron-mirror microscopy (EMM), e.g., an improvement of its resolving power together with an increase of the magnification makes it useful for investigating the ferroelectric domain physics. English has recently observed the domain texture in the surface layer of BaTiO3. The present authors ) have developed a theory by which one can evaluate small one-dimensional electric fields and/or topographic step heights in the crystal surfaces from their EMM pictures. This theory was applied to a quantitative study of the surface pattern of BaTiO3).

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