47 research outputs found
PP-waves in AdS Gauged Supergravities and Supernumerary Supersymmetry
Purely gravitational pp-waves in AdS backgrounds are described by the
generalised Kaigorodov metrics, and they generically preserve 1/4 of the
maximum supersymmetry allowed by the AdS spacetimes. We obtain 1/2
supersymmetric purely gravitational pp-wave solutions, in which the Kaigorodov
component is set to zero. We construct pp-waves in AdS gauged supergravities
supported by a vector field. We find that the solutions in D=4 and D=5 can then
preserve 1/2 of the supersymmetry. Like those in ungauged supergravities, the
supernumerary supersymmetry imposes additional constraints on the harmonic
function associated with the pp-waves. These new backgrounds provide
interesting novel features of the supersymmetry enhancement for the dual
conformal field theory in the infinite-momentum frame.Comment: Latex, 27 pages, minor typos corrected and reference added, to appear
in Phys. Rev.
Supersymmetric gyratons in five dimensions
We obtain the gravitational and electromagnetic field of a spinning radiation
beam-pulse (a gyraton) in minimal five-dimensional gauged supergravity and show
under which conditions the solution preserves part of the supersymmetry. The
configurations represent generalizations of Lobatchevski waves on AdS with
nonzero angular momentum, and possess a Siklos-Virasoro reparametrization
invariance. We compute the holographic stress-energy tensor of the solutions
and show that it transforms without anomaly under these reparametrizations.
Furthermore, we present supersymmetric gyratons both in gauged and ungauged
five-dimensional supergravity coupled to an arbitrary number of vector
supermultiplets, which include gyratons on domain walls.Comment: 25 pages, no figures, uses JHEP3.cls. Final version to appear in CQ
Mass and angular momentum of asymptotically AdS or flat solutions in the topologically massive gravity
We study the conserved charges of supersymmetric solutions in the
topologically massive gravity theory for both asymptotically flat and constant
curvature geometries.Comment: REVTEX4, 8 pages, no figures, added 2 references and a few clarifying
remark
Peculiarities of acid-base properties of peat formed in various agroclimatic zones of the Altai mountainous region
The results of the study of acid-base indicators of peat in the Altai mountainous region are presented. The natural factors that in the aggregate determine the peculiarities of the physicochemical properties of mountain peat of different agro-climatic zones of the Altai Mountains have been revealed. The variation in the acid values, total absorbed bases, adsorption capacity and the degree of saturation of raised-bog, transitional, fen peat, the number of exchangeable ions Π‘Π°2+ and Mg2+ has been estimated. The interrelation among these indicators has been presented. For the first time, regression equations of the relationship between exchangeable acidity ΡΠKCl and the degree of peat base saturation V, between total absorbed bases S and the degree of peat base saturation V have been obtained using nonlinear regression analysis. The adequacy and stability of the developed models have been verified. The calculated mean errors of approximation of regression models characterise the high accuracy of the forecast and are indicative of a good selection of models for the initial data
Kaigorodov spaces and their Penrose limits
Kaigorodov spaces arise, after spherical compactification, as near horizon
limits of M2, M5, and D3-branes with a particular pp-wave propagating in a
world volume direction. We show that the uncompactified near horizon
configurations K\times S are solutions of D=11 or D=10 IIB supergravity which
correspond to perturbed versions of their AdS \times S analogues. We derive the
Penrose-Gueven limits of the Kaigorodov space and the total spaces and analyse
their symmetries. An Inonu-Wigner contraction of the Lie algebra is shown to
occur, although there is a symmetry enhancement. We compare the results to the
maximally supersymmetric CW spaces found as limits of AdS\times S spacetimes:
the initial gravitational perturbation on the brane and its near horizon
geometry remains after taking non-trivial Penrose limits, but seems to
decouple. One particuliar limit yields a time-dependent homogeneous plane-wave
background whose string theory is solvable, while in the other cases we find
inhomogeneous backgrounds.Comment: latex2e, 24 page
Embeddings in Non-Vacuum Spacetimes
A scheme is discussed for embedding n-dimensional, Riemannian manifolds in an
(n+1)-dimensional Einstein space. Criteria for embedding a given manifold in a
spacetime that represents a solution to Einstein's equations sourced by a
massless scalar field are also discussed. The embedding procedures are
illustrated with a number of examples.Comment: 17 pages, Plain Latex. Extended discussion on embeddings with scalar
fields and further examples included. In press, Classical and Quantum Gravit
Shockwaves and deep inelastic scattering within the gauge/gravity duality
Within the gauge/gravity correspondence, we discuss the general formulation
of the shockwave metric which is dual to a 'nucleus' described by the
strongly-coupled N=4 SYM theory in the limit where the number of colors Nc is
arbitrarily large. We emphasize that the 'nucleus' must possess Nc^2 degrees of
freedom per unit volume, so like a finite-temperature plasma, in order for a
supergravity description to exist. We critically reassess previous proposals
for introducing transverse inhomogeneity in the shockwave and formulate a new
proposal in that sense, which involves no external source but requires the
introduction of an 'infrared' cutoff which mimics confinement. This cutoff
however plays no role when the shockwave is probed by a highly virtual
projectile, so like in deep inelastic scattering. We consider two such
projectiles, the dilaton and the R-current, and compute the respective
structure functions including unitarity corrections. We find that there are no
leading-twist contributions to the structure functions at high virtuality,
meaning that there are no point-like constituents in the strongly coupled
'nucleus'. In the black-disk regime at low virtuality, the structure functions
are suggestive of parton saturation with occupation numbers of order one. The
saturation momentum Qs grows with the energy like Qs^2 ~ 1/x (with x the
Bjorken variable), which is the hallmark of graviton exchanges and is also
necessary for the fulfillment of the energy-momentum sum rules.Comment: 43 page
Universal time-dependent deformations of Schrodinger geometry
We investigate universal time-dependent exact deformations of Schrodinger
geometry. We present 1) scale invariant but non-conformal deformation, 2)
non-conformal but scale invariant deformation, and 3) both scale and conformal
invariant deformation. All these solutions are universal in the sense that we
could embed them in any supergravity constructions of the Schrodinger invariant
geometry. We give a field theory interpretation of our time-dependent
solutions. In particular, we argue that any time-dependent chemical potential
can be treated exactly in our gravity dual approach.Comment: 24 pages, v2: references adde
Π Π°Π΄ΠΈΠΊΠ°Π»ΡΠ½Π°Ρ ΡΠΎΠΏΠΎΠ»ΠΈΠΌΠ΅ΡΠΈΠ·Π°ΡΠΈΡ ΡΡΠΈΡΠΎΠ»Π° ΠΈ Ξ±-Π°Π½Π³Π΅Π»ΠΈΠΊΠ°Π»Π°ΠΊΡΠΎΠ½Π°: ΡΠΈΠ½ΡΠ΅Π· ΠΈ ΡΠ²ΠΎΠΉΡΡΠ²Π° ΠΏΠΎΠ»ΡΡΠ΅Π½Π½ΡΡ ΡΠΎΠΏΠΎΠ»ΠΈΠΌΠ΅ΡΠΎΠ²
Biodegradation ability of synthetic polymer materials is an urgent problem of modern ecology
situation. A known new biodegradable polymer is polyangelicalactone (PAL). In this paper, styrene-Ξ±-
angelicalactone copolymers were obtained by radical polymerization. The resulting copolymers have
physical and mechanical properties similar to those of polystyrene and its graft-copolymers
with PAL.
Both they were mechanically destroyed when incubated in gray forest soil over 28 weeks. The obtained
results show that the modification of polystyrene with the impurities of Ξ±-angelicalactone
does not
worsen the mechanical properties of the copolymers but instead gives them biodegradation abilitiesΠ Π½Π°ΡΡΠΎΡΡΠ΅ΠΉ ΡΠ°Π±ΠΎΡΠ΅ ΠΏΠΎΠ»ΡΡΠ΅Π½Ρ ΡΠΎΠΏΠΎΠ»ΠΈΠΌΠ΅ΡΡ ΡΡΠΈΡΠΎΠ»Π° ΠΈ Ξ±-Π°Π½Π³Π΅Π»ΠΈΠΊΠ°Π»Π°ΠΊΡΠΎΠ½Π°
ΠΌΠ΅ΡΠΎΠ΄ΠΎΠΌ
ΡΠ°Π΄ΠΈΠΊΠ°Π»ΡΠ½ΠΎΠΉ ΠΏΠΎΠ»ΠΈΠΌΠ΅ΡΠΈΠ·Π°ΡΠΈΠΈ. ΠΠΎΠ»ΡΡΠ΅Π½Π½ΡΠ΅ ΡΠΎΠΏΠΎΠ»ΠΈΠΌΠ΅ΡΡ ΠΈΠΌΠ΅ΡΡ ΡΠΈΠ·ΠΈΠΊΠΎ-ΠΌΠ΅Ρ
Π°Π½ΠΈΡΠ΅ΡΠΊΠΈΠ΅
ΡΠ²ΠΎΠΉΡΡΠ²Π°,
Π°Π½Π°Π»ΠΎΠ³ΠΈΡΠ½ΡΠ΅ ΡΠ²ΠΎΠΉΡΡΠ²Π°ΠΌ
ΠΏΠΎΠ»ΠΈΡΡΠΈΡΠΎΠ»Π° ΠΈ Π΅Π³ΠΎ ΠΏΡΠΈΠ²ΠΈΡΡΡ
ΡΠΎΠΏΠΎΠ»ΠΈΠΌΠ΅ΡΠΎΠ² Ρ ΠΏΠΎΠ»ΠΈΠ°Π½Π³Π΅Π»ΠΈΠΊΠ°Π»Π°ΠΊΡΠΎΠ½ΠΎΠΌ. ΠΠ±Π°
ΠΏΠΎΠ»ΠΈΠΌΠ΅ΡΠ° ΠΌΠ΅Ρ
Π°Π½ΠΈΡΠ΅ΡΠΊΠΈ ΡΠ°Π·ΡΡΡΠ°ΡΡΡΡ ΠΏΡΠΈ ΠΈΠ½ΠΊΡΠ±Π°ΡΠΈΠΈ Π² ΡΠ΅ΡΠΎΠΉ Π»Π΅ΡΠ½ΠΎΠΉ ΠΏΠΎΡΠ²Π΅ Π² ΡΠ΅ΡΠ΅Π½ΠΈΠ΅ 28 Π½Π΅Π΄Π΅Π»Ρ.
ΠΠΎΠ»ΡΡΠ΅Π½Π½ΡΠ΅ ΡΠ΅Π·ΡΠ»ΡΡΠ°ΡΡ ΠΏΠΎΠΊΠ°Π·ΡΠ²Π°ΡΡ, ΡΡΠΎ ΠΌΠΎΠ΄ΠΈΡΠΈΠΊΠ°ΡΠΈΡ ΠΏΠΎΠ»ΠΈΡΡΠΈΡΠΎΠ»Π° ΠΏΡΠΈΠΌΠ΅ΡΡΠΌΠΈ Ξ±-Π°Π½Π³Π΅Π»ΠΈΠΊΠ°Π»Π°ΠΊΡΠΎΠ½Π°
Π½Π΅ ΡΡ
ΡΠ΄ΡΠ°Π΅Ρ ΠΌΠ΅Ρ
Π°Π½ΠΈΡΠ΅ΡΠΊΠΈΠ΅ ΡΠ²ΠΎΠΉΡΡΠ²Π°
ΡΠΎΠΏΠΎΠ»ΠΈΠΌΠ΅ΡΠΎΠ² ΠΈ ΠΏΡΠΈΠ΄Π°Π΅Ρ ΠΈΠΌ ΡΠΏΠΎΡΠΎΠ±Π½ΠΎΡΡΡ ΠΊ Π±ΠΈΠΎΡΠ°Π·Π»ΠΎΠΆΠ΅Π½ΠΈ