EFTA01141162Set 9
2013-10-046p3,224w
period of
gravitational field. That would be ironic, not to say pathetic, quasi-de Sitter expansion associated with a scalar field
since the apparent tension between quantum mechanics ... full quantum treatment of general relativity has been one approximately massless scalar field in de Sitter space,
of the driving forces in much of fundamental particle theory expanded into Fourier ... this case, is the expanding
Universe. where a is the scale factor during the de Sitter expansion
Let us emphasize at the start that such a cosmological
https://www.justice.gov/epstein/files/DataSet%209/EFTA01141162.pdf
EFTA00316650Set 9
3p2,026w
period of inflation in the early universe results
from a period of quasi-de Sitter expansion associated with a scalar field in an almost flat potential. If one considers ... quantized approximately massless scalar field in de-Sitter space, expanded into Fourier components with quantized
mode functions, vk then it is straightforward to calculate the zero-point quantum fluctuations ... approaches
3(aH)2
= r 1t.1
where a is the scale factor during the de-Sitter expansion, and H is the Hubble expansion parameter associated with
the de Sitter phase
https://www.justice.gov/epstein/files/DataSet%209/EFTA00316650.pdf
EFTA01114598Set 9
12p10,178w
known that there are only three such manifolds: the flat
space and the (anti-) de Sitter spaces. On all three of these ... relativistic
minimum-length, Phys. Len. B 510. 255 (2001) [arXiv:hep- particle with de Sitter momentum space, arXiv:1008.2962 [hep-
th/0012238]. thl.
[29] G. Amelino-Camelia. Relativity in space-times ... Glikman, S. Nowak. Doubly special relativity and
distance structure governed by art observer-independent de Sitter space, Class. Quant. Gray. 20 (2003)4799-4816. [hep-
(Planckian) length scale
https://www.justice.gov/epstein/files/DataSet%209/EFTA01114598.pdf
EFTA00752719Set 9
2010-11-0821p2,633w
theoretical physics stuff out... :-( For example, when I wrote about finding
applications of Anti de Sitter Space and Conformal Field Theory to other areas of physics, such as
nuclear physics ... given to robust original research proposals in the
following areas:
Finding applications of Anti de Sitter space and conformal field theory to
other areas of physics, such as nuclear physics
https://www.justice.gov/epstein/files/DataSet%209/EFTA00752719.pdf
EFTA02403023Set 11
2010-07-0528p12,345w
terms of these variables the metric on the de Sitter momentum space is
dso _ 20 MA) PidPidPo dpidpi (27)
dpo —
4:11)
Ea
9
EFTA_R1_01441421
EFTA02403031
The Casimir ... Arzano and J. Kowalski-Glilunan, Kinematics of particles with de Sitter momentum space,
preprint in preparation.
[13[ M. Arzano and J. Kowalski-Glilunan, Deformations of spacetime symmetries, unpublished book
manuscript
https://www.justice.gov/epstein/files/DataSet%2011/EFTA02403023.pdf
EFTA01805311Set 10
2010-07-0720p10,141w
symmetry, arXiv:1006.2126.
[23] M. Arzano and J. Kowalski-Glikman, Kinematics of particles with de Sitter momentum space,
preprint in preparation.
[24] M. Arzano and J. Kowalski-Glikman, Deformations
https://www.justice.gov/epstein/files/DataSet%2010/EFTA01805311.pdf
EFTA00614975Set 9
2015-06-3033p14,601w
Mezincescu and P. K. Townsend, "Stability at a Local Maximum in Higher Dimensional
Anti-De Sitter Space and Applications to Supergravity", Annals Phys. 160, 406-419,
(1985).
L. Mezincescu
https://www.justice.gov/epstein/files/DataSet%209/EFTA00614975.pdf
EFTA02403003Set 11
2010-07-0720p10,140w
symmetry, arXiv:1006.2126.
[23] M. Arzano and J. Kowalski-Glikman, Kinematics of particles with de Sitter momentum space,
preprint in preparation.
[24] M. Arzano and J. Kowalski-Glikman, Deformations
https://www.justice.gov/epstein/files/DataSet%2011/EFTA02403003.pdf
EFTA01157239Set 9
2015-06-3033p14,596w
Mezincescu and P. K. Townsend, "Stability at a Local Maximum in Higher Dimensional
Anti-De Sitter Space and Applications to Supergravity", Annals Phys. 160, 406-419,
(1985).
L. Mezincescu
https://www.justice.gov/epstein/files/DataSet%209/EFTA01157239.pdf