130 research outputs found
Monetary policy and economic activity: a postwar review
Monetary policy ; Financial markets ; Economic conditions
From Earth to Orbit: An assessment of transportation options
The report assesses the requirements, benefits, technological feasibility, and roles of Earth-to-Orbit transportation systems and options that could be developed in support of future national space programs. Transportation requirements, including those for Mission-to-Planet Earth, Space Station Freedom assembly and operation, human exploration of space, space science missions, and other major civil space missions are examined. These requirements are compared with existing, planned, and potential launch capabilities, including expendable launch vehicles (ELV's), the Space Shuttle, the National Launch System (NLS), and new launch options. In addition, the report examines propulsion systems in the context of various launch vehicles. These include the Advanced Solid Rocket Motor (ASRM), the Redesigned Solid Rocket Motor (RSRM), the Solid Rocket Motor Upgrade (SRMU), the Space Shuttle Main Engine (SSME), the Space Transportation Main Engine (STME), existing expendable launch vehicle engines, and liquid-oxygen/hydrocarbon engines. Consideration is given to systems that have been proposed to accomplish the national interests in relatively cost effective ways, with the recognition that safety and reliability contribute to cost-effectiveness. Related resources, including technology, propulsion test facilities, and manufacturing capabilities are also discussed
On the Back Reaction Problem for Gravitational Perturbations
We derive the effective energy-momentum tensor for cosmological perturbations
and prove its gauge-invariance. The result is applied to study the influence of
perturbations on the behaviour of the Friedmann background in inflationary
Universe scenarios. We found that the back reaction of cosmological
perturbations on the background can become important already at energies below
the self-reproduction scale.Comment: 4 pages, uses LATE
The AdS/CFT Correspondence and a New Positive Energy Conjecture for General Relativity
We examine the AdS/CFT correspondence when the gauge theory is considered on
a compactified space with supersymmetry breaking boundary conditions. We find
that the corresponding supergravity solution has a negative energy, in
agreement with the expected negative Casimir energy in the field theory.
Stability of the gauge theory would imply that this supergravity solution has
minimum energy among all solutions with the same boundary conditions. Hence we
are lead to conjecture a new positive energy theorem for asymptotically locally
Anti-de Sitter spacetimes. We show that the candidate minimum energy solution
is stable against all quadratic fluctuations of the metric.Comment: 25 pages, harvma
The Energy-Momentum Tensor for Cosmological Perturbations
We study the effective energy-momentum tensor (EMT) for cosmological
perturbations and formulate the gravitational back-reaction problem in a gauge
invariant manner. We analyze the explicit expressions for the EMT in the cases
of scalar metric fluctuations and of gravitational waves and derive the
resulting equations of state. The formalism is applied to investigate the
back-reaction effects in chaotic inflation. We find that for long wavelength
scalar and tensor perturbations, the effective energy density is negative and
thus counteracts any pre-existing cosmological constant. For scalar
perturbations during an epoch of inflation, the equation of state is de
Sitter-like.Comment: 29 pages, LaTex; to appear in Phys. Rev.
Taub--NUT Dyons in Heterotic String Theory
Starting with the Taub--NUT solution to Einstein's equations, together with a
constant dilaton, a dyonic Taub--NUT solution of low energy heterotic string
theory with non--trivial dilaton, axion and gauge fields is constructed
by employing transformations. The electromagnetic dual of this
solution is constructed, using SL(2,\rline) transformations. By an
appropriate change to scaled variables, the extremal limit of the dual solution
is shown to correspond to the low energy limit of an exact conformal field
theory presented previously.Comment: 16 pages (plain TEX), (Revised version has curvature singularities
correctly identified), IASSNS-HEP-94/50, McGill/94-2
Pathologies in Asymptotically Lifshitz Spacetimes
There has been significant interest in the last several years in studying
possible gravitational duals, known as Lifshitz spacetimes, to anisotropically
scaling field theories by adding matter to distort the asymptotics of an AdS
spacetime. We point out that putative ground state for the most heavily studied
example of such a spacetime, that with a flat spatial section, suffers from a
naked singularity and further point out this singularity is not resolvable by
any known stringy effect. We review the reasons one might worry that
asymptotically Lifshitz spacetimes are unstable and employ the initial data
problem to study the stability of such systems. Rather surprisingly this
question, and even the initial value problem itself, for these spacetimes turns
out to generically not be well-posed. A generic normalizable state will evolve
in such a way to violate Lifshitz asymptotics in finite time. Conversely,
enforcing the desired asymptotics at all times puts strong restrictions not
just on the metric and fields in the asymptotic region but in the deep interior
as well. Generically, even perturbations of the matter field of compact support
are not compatible with the desired asymptotics.Comment: 36 pages, 1 figure, v2: Enhanced discussion of singularity, including
relationship to Gubser's conjecture and singularity in RG flow solution, plus
minor clarification
Back Reaction And Local Cosmological Expansion Rate
We calculate the back reaction of cosmological perturbations on a general
relativistic variable which measures the local expansion rate of the Universe.
Specifically, we consider a cosmological model in which matter is described by
a single field. We analyze back reaction both in a matter dominated Universe
and in a phase of scalar field-driven chaotic inflation. In both cases, we find
that the leading infrared terms contributing to the back reaction vanish when
the local expansion rate is measured at a fixed value of the matter field which
is used as a clock, whereas they do not appear to vanish if the expansion rate
is evaluated at a fixed value of the background time. We discuss possible
implications for more realistic models with a more complicated matter sector.Comment: 7 pages, No figure
Can the Acceleration of Our Universe Be Explained by the Effects of Inhomogeneities?
No. It is simply not plausible that cosmic acceleration could arise within
the context of general relativity from a back-reaction effect of
inhomogeneities in our universe, without the presence of a cosmological
constant or ``dark energy.'' We point out that our universe appears to be
described very accurately on all scales by a Newtonianly perturbed FLRW metric.
(This assertion is entirely consistent with the fact that we commonly encounter
.) If the universe is accurately described by a
Newtonianly perturbed FLRW metric, then the back-reaction of inhomogeneities on
the dynamics of the universe is negligible. If not, then it is the burden of an
alternative model to account for the observed properties of our universe. We
emphasize with concrete examples that it is {\it not} adequate to attempt to
justify a model by merely showing that some spatially averaged quantities
behave the same way as in FLRW models with acceleration. A quantity
representing the ``scale factor'' may ``accelerate'' without there being any
physically observable consequences of this acceleration. It also is {\it not}
adequate to calculate the second-order stress energy tensor and show that it
has a form similar to that of a cosmological constant of the appropriate
magnitude. The second-order stress energy tensor is gauge dependent, and if it
were large, contributions of higher perturbative order could not be neglected.
We attempt to clear up the apparent confusion between the second-order stress
energy tensor arising in perturbation theory and the ``effective stress energy
tensor'' arising in the ``shortwave approximation.''Comment: 20 pages, 1 figure, several footnotes and references added, version
accepted for publication in CQG;some clarifying comments adde
Large N Phases, Gravitational Instantons and the Nuts and Bolts of AdS Holography
Recent results in the literature concerning holography indicate that the
thermodynamics of quantum gravity (at least with a negative cosmological
constant) can be modeled by the large N thermodynamics of quantum field theory.
We emphasize that this suggests a completely unitary evolution of processes in
quantum gravity, including black hole formation and decay; and even more
extreme examples involving topology change. As concrete examples which show
that this correspondence holds even when the space-time is only locally
asymptotically AdS, we compute the thermodynamical phase structure of the
AdS-Taub-NUT and AdS-Taub-Bolt spacetimes, and compare them to a 2+1
dimensional conformal field theory (at large N) compactified on a squashed
three sphere, and on the twisted plane.Comment: 20 pages, three figures. (uses harvmac.tex and epsf.tex
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