225 research outputs found
Dynamical dark energy from extra dimensions
We consider multidimensional cosmological model with a higher-dimensional
product manifold M = R x R^{d_0} x H^{d_1}/\Gamma where R^{d_0} is
d_0-dimensional Ricci-flat external (our) space and H^{d_1}/\Gamma is
d_1-dimensional compact hyperbolic internal space. M2-brane solution for this
model has the stage of accelerating expansion of the external space. We apply
this model to explain the late time acceleration of our Universe. Recent
observational data (the Hubble parameter at the present time and the redshift
when the deceleration parameter changes its sign) fix fully all free parameters
of the model. As a result, we find that considered model has too big size of
the internal space at the present time and variation of the effective
four-dimensional fine structure constant strongly exceeds the observational
limits.Comment: 5 pages, 3 figures, LaTex, a few remarks and reference adde
Integrable Multicomponent Perfect Fluid Multidimensional Cosmology II: Scalar Fields
We consider anisotropic cosmological models with an universe of dimension 4
or more, factorized into n>1 Ricci-flat spaces, containing an m-component
perfect fluid of m non-interacting homogeneous minimally coupled scalar fields
under special conditions. We describe the dynamics of the universe: It has a
Kasner-like behaviour near the singularity and isotropizes during the expansion
to infinity.
Some of the considered models are integrable, and classical as well as
quantum solutions are found. Some solutions produce inflation from "nothing".
There exist classical asymptotically anti-de Sitter wormholes, and quantum
wormholes with discrete spectrum.Comment: 28 pages, LaTeX, subm. to Gen. Rel. Gra
Woodworking facilities: Driving efficiency through Automation applied to major process steps
The investment scenario applied to forestry development analyzes the fundamental changes in the production structure, among other things. These changes refer to the priority development of the pulp and paper industry through the chain of large-scale woodworking facilities, where pulp, paper and cardboard manufacturing plants are the key links. Such facilities include sawmilling facilities, wood-processing factories, and timber factories. Those provide a significant economic benefit, so improving them is one of the top priorities. Considering this priority is the purpose of this article. The goal was achieved using common and scientific research methods, including mathematical modeling. Theoretical research resulted in three sets of formulas adapted for evaluating the pulpwood barking from theoretical findings on image recognition. Β© 2018 Authors
On new gravitational instantons describing creation of brane-worlds
By considering 5--dimensional cosmological models with a bulk filled with a
pressureless scalar field; equivalently dust matter, and a negative
cosmological constant, we have found a regular instantonic solution which is
free from any singularity at the origin of the extra--coordinate. This
instanton describes 5--dimensional asymptotically anti de Sitter wormhole, when
the bulk has a topology R times S^4. Compactified brane-world instantons which
are built up from such instantonic solution describe either a single brane or a
string of branes. Their analytical continuation to the pseudo--Riemannian
metric can give rise to either 4-dimensional inflating branes or solutions with
the same dynamical behaviour for extra--dimension and branes, in addition to
multitemporal solutions. Dust brane-world models with arbitrary dimensions (D
>= 5) as well as other spatial topologies are also briefly discussed.Comment: 11 pages, 3 figures, LaTeX2e, accepted for publication in Classical
and Quantum Gravit
Π‘ΠΠΠ‘ΠΠ ΠΠ ΠΠ’ΠΠΠΠΠ ΠΠΠΠΠΠΠΠ ΠΠΠ ΠΠΠΠ’ΠΠ ΠΠΠ§ΠΠ«
Water-retaining roughnesses (holes, non-continuous furrows, micro-lagoons) come into being on the field surface at its tillage. They prevent a backflow, an erosion on slope lands and improve moisture content the soil. However, in the last decades such methods of a soil tillage are not used and the equipment for them are not manufactured. The author offered a new method of soil tillge with strips interchange (subsoil tilled and with the vegetable remains which are covered by the soil) in which cutout spherical disks form water-retaining non-continuous furrows. For this purpose harrows with two-disk and three-disk sections were developed. Two-disk sections in a front row contain needle disks and one spherical, and in a back row - needle and cutout spherical ones, forming a stank in a furrow. Three-disk sections in a front row contain needle disks, and in a back row - two needle and cutout spherical ones. A furrow part limited to its stanks is 4-5 times longer than a stank. A nonmoldboard loosened strip is wider than a strip with the covered vegetable remains and a non-continuous furrow. However, the general width does not exceed 0.4 m. In case of conservation tillage by a harrow with two-disk sections with spaces between disks 180 and 250 mm and 10 cm deep spherical disk non-continuous furrows can save up 216 and 155 cub. m of water per 1 hectare, and with three-disk at the same spaces - 144 and 103.7 cub. m respectively. At a disk approach angle of 20 degrees and 14 cm deep disks the capacity of furrows increases by 1.6 times.ΠΠΎΠ΄ΠΎΡΠ΄Π΅ΡΠΆΠΈΠ²Π°ΡΡΠΈΠ΅ Π½Π΅ΡΠΎΠ²Π½ΠΎΡΡΠΈ (Π»ΡΠ½ΠΊΠΈ, ΠΏΡΠ΅ΡΡΠ²ΠΈΡΡΡΠ΅ Π±ΠΎΡΠΎΠ·Π΄Ρ, ΠΌΠΈΠΊΡΠΎΠ»ΠΈΠΌΠ°Π½Ρ), ΡΠΎΠ·Π΄Π°Π½Π½ΡΠ΅ Π½Π° ΠΏΠΎΠ²Π΅ΡΡ
Π½ΠΎΡΡΠΈ ΠΏΠΎΠ»Ρ ΠΏΡΠΈ Π΅Π³ΠΎ ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠ΅, ΠΏΡΠ΅Π΄ΠΎΡΠ²ΡΠ°ΡΠ°ΡΡ ΡΡΠΎΠΊ, ΠΏΡΠΎΡΠ²Π»Π΅Π½ΠΈΡ ΡΡΠΎΠ·ΠΈΠΈ Π½Π° ΡΠΊΠ»ΠΎΠ½ΠΎΠ²ΡΡ
Π·Π΅ΠΌΠ»ΡΡ
ΠΈ ΡΠ»ΡΡΡΠ°ΡΡ Π²Π»Π°Π³ΠΎΠΎΠ±Π΅ΡΠΏΠ΅ΡΠ΅Π½Π½ΠΎΡΡΡ ΠΏΠΎΡΠ²Ρ. ΠΠ΄Π½Π°ΠΊΠΎ Π² ΠΏΠΎΡΠ»Π΅Π΄Π½ΠΈΠ΅ Π΄Π΅ΡΡΡΠΈΠ»Π΅ΡΠΈΡ ΡΠ°ΠΊΠΈΠ΅ ΠΏΡΠΈΠ΅ΠΌΡ ΠΏΠΎΡΠ²ΠΎΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠΈ Π½Π΅ ΠΏΡΠΈΠΌΠ΅Π½ΡΡΡ ΠΈ ΡΠ΅Ρ
Π½ΠΈΠΊΡ Π΄Π»Ρ Π½ΠΈΡ
Π½Π΅ ΠΏΡΠΎΠΈΠ·Π²ΠΎΠ΄ΡΡ. ΠΡΠ΅Π΄Π»ΠΎΠΆΠΈΠ»ΠΈ Π½ΠΎΠ²ΡΠΉ ΡΠΏΠΎΡΠΎΠ± ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠΈ ΠΏΠΎΡΠ²Ρ Ρ ΡΠ΅ΡΠ΅Π΄ΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΏΠΎΠ»ΠΎΡ (Π±Π΅Π·ΠΎΡΠ²Π°Π»ΡΠ½ΠΎ ΡΠ°Π·ΡΡΡ
Π»Π΅Π½Π½ΡΡ
ΠΈ Ρ Π·Π°Π΄Π΅Π»Π°Π½Π½ΡΠΌΠΈ Π² ΠΏΠΎΡΠ²Ρ ΡΠ°ΡΡΠΈΡΠ΅Π»ΡΠ½ΡΠΌΠΈ ΠΎΡΡΠ°ΡΠΊΠ°ΠΌΠΈ), Π² ΠΊΠΎΡΠΎΡΡΡ
ΡΡΠ΅ΡΠΈΡΠ΅ΡΠΊΠΈΠΌΠΈ Π΄ΠΈΡΠΊΠ°ΠΌΠΈ Ρ Π²ΡΡΠ΅Π·ΠΎΠΌ ΡΠΎΡΠΌΠΈΡΡΡΡ Π²ΠΎΠ΄ΠΎΡΠ΄Π΅ΡΠΆΠΈΠ²Π°ΡΡΠΈΠ΅ ΠΏΡΠ΅ΡΡΠ²ΠΈΡΡΡΠ΅ Π±ΠΎΡΠΎΠ·Π΄Ρ. ΠΠ»Ρ Π²ΡΠΏΠΎΠ»Π½Π΅Π½ΠΈΡ ΡΡΠΎΠ³ΠΎ ΡΠΏΠΎΡΠΎΠ±Π° ΡΠ°Π·ΡΠ°Π±ΠΎΡΠ°Π»ΠΈ Π±ΠΎΡΠΎΠ½Ρ Ρ Π΄Π²ΡΡ
Π΄ΠΈΡΠΊΠΎΠ²ΡΠΌΠΈ ΠΈ ΡΡΠ΅Ρ
Π΄ΠΈΡΠΊΠΎΠ²ΡΠΌΠΈ ΡΠ΅ΠΊΡΠΈΡΠΌΠΈ. ΠΠ²ΡΡ
Π΄ΠΈΡΠΊΠΎΠ²ΡΠ΅ ΡΠ΅ΠΊΡΠΈΠΈ ΠΏΠ΅ΡΠ΅Π΄Π½Π΅Π³ΠΎ ΡΡΠ΄Π° ΡΠΎΠ΄Π΅ΡΠΆΠ°Ρ ΠΈΠ³ΠΎΠ»ΡΡΠ°ΡΡΠ΅ Π΄ΠΈΡΠΊΠΈ ΠΈ ΠΎΠ΄ΠΈΠ½ ΡΡΠ΅ΡΠΈΡΠ΅ΡΠΊΠΈΠΉ, Π° Π·Π°Π΄Π½Π΅Π³ΠΎ - ΠΈΠ³ΠΎΠ»ΡΡΠ°ΡΡΠΉ ΠΈ ΡΡΠ΅ΡΠΈΡΠ΅ΡΠΊΠΈΠΉ Ρ Π²ΡΡΠ΅Π·ΠΎΠΌ, ΡΠΎΡΠΌΠΈΡΡΡΡΠΈΠΉ ΠΏΠ΅ΡΠ΅ΠΌΡΡΠΊΡ Π² Π±ΠΎΡΠΎΠ·Π΄Π΅. Π’ΡΠ΅Ρ
Π΄ΠΈΡΠΊΠΎΠ²ΡΠ΅ ΡΠ΅ΠΊΡΠΈΠΈ ΠΏΠ΅ΡΠ΅Π΄Π½Π΅Π³ΠΎ ΡΡΠ΄Π° ΡΠΎΠ΄Π΅ΡΠΆΠ°Ρ ΠΈΠ³ΠΎΠ»ΡΡΠ°ΡΡΠ΅ Π΄ΠΈΡΠΊΠΈ, Π° Π·Π°Π΄Π½Π΅Π³ΠΎ ΡΡΠ΄Π° - Π΄Π²Π° ΠΈΠ³ΠΎΠ»ΡΡΠ°ΡΡΡ
ΠΈ ΡΡΠ΅ΡΠΈΡΠ΅ΡΠΊΠΈΠΉ Ρ Π²ΡΡΠ΅Π·ΠΎΠΌ. Π£ΡΠ°ΡΡΠΎΠΊ Π±ΠΎΡΠΎΠ·Π΄Ρ, ΠΎΠ³ΡΠ°Π½ΠΈΡΠ΅Π½Π½ΡΠΉ Π΅Π΅ ΠΏΠ΅ΡΠ΅ΠΌΡΡΠΊΠ°ΠΌΠΈ, Π² 4-5 ΡΠ°Π· Π΄Π»ΠΈΠ½Π½Π΅Π΅ ΠΏΠ΅ΡΠ΅ΠΌΡΡΠΊΠΈ. ΠΠ΅Π·ΠΎΡΠ²Π°Π»ΡΠ½ΠΎ ΡΠ°Π·ΡΡΡ
Π»Π΅Π½Π½Π°Ρ ΠΏΠΎΠ»ΠΎΡΠ° ΡΠΈΡΠ΅ ΠΏΠΎΠ»ΠΎΡΡ Ρ Π·Π°Π΄Π΅Π»Π°Π½Π½ΡΠΌΠΈ ΡΠ°ΡΡΠΈΡΠ΅Π»ΡΠ½ΡΠΌΠΈ ΠΎΡΡΠ°ΡΠΊΠ°ΠΌΠΈ ΠΈ ΠΏΡΠ΅ΡΡΠ²ΠΈΡΡΠΎΠΉ Π±ΠΎΡΠΎΠ·Π΄ΠΎΠΉ. ΠΠ΄Π½Π°ΠΊΠΎ ΠΎΠ±ΡΠ°Ρ ΡΠΈΡΠΈΠ½Π° Π½Π΅ ΠΏΡΠ΅Π²ΡΡΠ°Π΅Ρ 0,4 ΠΌ. ΠΡΠΈ ΠΏΡΠΎΡΠΈΠ²ΠΎΡΡΠΎΠ·ΠΈΠΎΠ½Π½ΠΎΠΉ ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠ΅ Π±ΠΎΡΠΎΠ½ΠΎΠΉ Ρ Π΄Π²ΡΡ
Π΄ΠΈΡΠΊΠΎΠ²ΡΠΌΠΈ ΡΠ΅ΠΊΡΠΈΡΠΌΠΈ Ρ ΠΈΠ½ΡΠ΅ΡΠ²Π°Π»Π°ΠΌΠΈ ΠΌΠ΅ΠΆΠ΄Ρ Π΄ΠΈΡΠΊΠ°ΠΌΠΈ 180 ΠΈ 250 ΠΌΠΌ ΠΈ Π·Π°Π³Π»ΡΠ±Π»Π΅Π½ΠΈΠ΅ΠΌ ΡΡΠ΅ΡΠΈΡΠ΅ΡΠΊΠΈΡ
Π΄ΠΈΡΠΊΠΎΠ² Π½Π° 10 ΡΠΌ ΠΏΡΠ΅ΡΡΠ²ΠΈΡΡΡΠ΅ Π±ΠΎΡΠΎΠ·Π΄Ρ ΠΌΠΎΠ³ΡΡ Π½Π°ΠΊΠΎΠΏΠΈΡΡ 216 ΠΈ 155 ΠΊΡΠ±. ΠΌ Π²ΠΎΠ΄Ρ Π½Π° 1 Π³Π°, Π° Ρ ΡΡΠ΅Ρ
Π΄ΠΈΡΠΊΠΎΠ²ΡΠΌΠΈ ΠΏΡΠΈ ΡΠ°ΠΊΠΈΡ
ΠΆΠ΅ ΠΈΠ½ΡΠ΅ΡΠ²Π°Π»Π°Ρ
- 144 ΠΈ 103,7 ΠΊΡΠ±. ΠΌ ΡΠΎΠΎΡΠ²Π΅ΡΡΡΠ²Π΅Π½Π½ΠΎ. ΠΡΠΈ ΡΠ³Π»Π΅ Π°ΡΠ°ΠΊΠΈ 20 Π³ΡΠ°Π΄ΡΡΠΎΠ² ΠΈ Π·Π°Π³Π»ΡΠ±Π»Π΅Π½ΠΈΠΈ Π΄ΠΈΡΠΊΠΎΠ² Π½Π° 14 ΡΠΌ Π²ΠΌΠ΅ΡΡΠΈΠΌΠΎΡΡΡ Π±ΠΎΡΠΎΠ·Π΄ ΡΠ²Π΅Π»ΠΈΡΠΈΠ²Π°Π΅ΡΡΡ Π² 1,6 ΡΠ°Π·Π°
Slow-roll inflation in (R+R*4) gravity
We reconsider the toy-model of topological inflation, based on the
R*4-modified gravity. By using its equivalence to the certain scalar-tensor
gravity model in four space-time dimensions, we compute the inflaton scalar
potential and investigate a possibility of inflation. We confirm the existence
of the slow-roll inflation with an exit. However, the model suffers from the
eta-problem that gives rise to the unacceptable value of the spectral index n_s
of scalar perturbations.Comment: 12 pages, 3 figures, LaTeX, misprints corrected and references
update
Π ΠΠΠΠΠ©ΠΠΠΠ Π‘Π€ΠΠ ΠΠ§ΠΠ‘ΠΠΠ₯ ΠΠΠ‘ΠΠΠ Π€Π ΠΠΠ’ΠΠΠ¬ΠΠ«Π₯ ΠΠΠ ΠΠ
Disk-type spherical working tools are widely used in soil-cultivating machines, where they serve as an element base for combined units and disk harrows, including the multi-row ones with disks on individual racks. The tools are used in the implementation of traditional technologies based on reversible plowing, with surface tillage after late-harvested predecessors, for example, corn, sunflower, and also in NO-TIL technologies. (Research purpose) To determine the arrangement of working tools on the disk harrow frame, which reduces the required number of disks and improves the quality of soil cultivation. (Materials and methods) The authors have analyzed the arrangement of disk harrow working tools and determined their rational arrangement and mutual positions in the rows, which increases the tillage width between adjacent soil strips, thus improving the completeness of soil shearing and loosening over the entire operating width with simultaneous decreasing of the required number of disks. (Results and discussion) The authors have determined the interrelated arrangement of disks in their rows, aimed at improving soil shearing, so that the number of strips tilled into a ridge by adjacent disks increases. It has been shown that the arrangement of working tools of the consecutive row determined by the orientation of the adjacent disks of the previous row, allows to economize one working tool for every 400 mm of its operating width when shearing the soil all the way across the entire width of the disk harrow. (Conclusions) It has been established that when soil is tilled with a disk and moved toward the already processed adjacent strip, the technological width of the disk coverage increases due to the deformation of soil tearing and shearing. The authors have proposed the arrangement order of spherical disks and their mutual orientation, which improves the quality of soil cultivation, the completeness of soil shearing along the entire operating width, and leads to a reduction in the number of disks.Π ΠΏΠΎΡΠ²ΠΎΠΎΠ±ΡΠ°Π±Π°ΡΡΠ²Π°ΡΡΠΈΡ
Β ΠΌΠ°ΡΠΈΠ½Π°Ρ
ΡΠΈΡΠΎΠΊΠΎ ΠΈΡΠΏΠΎΠ»ΡΠ·ΡΡΡ Π΄ΠΈΡΠΊΠΎΠ²ΡΠ΅ ΡΡΠ΅ΡΠΈΡΠ΅ΡΠΊΠΈΠ΅ ΡΠ°Π±ΠΎΡΠΈΠ΅ ΠΎΡΠ³Π°Π½Ρ, ΠΊΠΎΡΠΎΡΡΠ΅ ΡΠ»ΡΠΆΠ°Ρ ΡΠ»Π΅ΠΌΠ΅Π½ΡΠ½ΠΎΠΉ Π±Π°Π·ΠΎΠΉ ΠΊΠΎΠΌΠ±ΠΈΠ½ΠΈΡΠΎΠ²Π°Π½Π½ΡΡ
Π°Π³ΡΠ΅Π³Π°ΡΠΎΠ² ΠΈ Π΄ΠΈΡΠΊΠΎΠ²ΡΡ
Π±ΠΎΡΠΎΠ½, Π² ΡΠΎΠΌ ΡΠΈΡΠ»Π΅ ΠΌΠ½ΠΎΠ³ΠΎΡΡΠ΄Π½ΡΡ
Ρ Π΄ΠΈΡΠΊΠ°ΠΌΠΈ Π½Π° ΠΈΠ½Π΄ΠΈΠ²ΠΈΠ΄ΡΠ°Π»ΡΠ½ΡΡ
ΡΡΠΎΠΉΠΊΠ°Ρ
. ΠΡΡΠ΄ΠΈΡ ΠΏΡΠΈΠΌΠ΅Π½ΡΡΡ ΠΏΡΠΈ Π²ΡΠΏΠΎΠ»Π½Π΅Π½ΠΈΠΈ ΡΡΠ°Π΄ΠΈΡΠΈΠΎΠ½Π½ΠΎΠΉ ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΠΈ Π½Π° ΠΎΡΠ½ΠΎΠ²Π΅ ΠΎΡΠ²Π°Π»ΡΠ½ΠΎΠΉ Π²ΡΠΏΠ°ΡΠΊΠΈ ΠΏΡΠΈ ΠΌΠ΅Π»ΠΊΠΎΠΉ ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠ΅ ΠΏΠΎΡΠ»Π΅ ΠΏΠΎΠ·Π΄Π½ΠΎ ΡΠ±ΡΠ°Π½Π½ΡΡ
ΠΏΡΠ΅Π΄ΡΠ΅ΡΡΠ²Π΅Π½Π½ΠΈΠΊΠΎΠ², Π½Π°ΠΏΡΠΈΠΌΠ΅Ρ, ΠΊΡΠΊΡΡΡΠ·Ρ, ΠΏΠΎΠ΄ΡΠΎΠ»Π½Π΅ΡΠ½ΠΈΠΊΠ°, Π° ΡΠ°ΠΊΠΆΠ΅ Π² ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΡΡ
NO-TIL. (Π¦Π΅Π»Ρ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ) ΠΠ±ΠΎΡΠ½ΠΎΠ²Π°ΡΡΒ ΡΠ°Π·ΠΌΠ΅ΡΠ΅Π½ΠΈΠ΅ ΡΠ°Π±ΠΎΡΠΈΡ
ΠΎΡΠ³Π°Π½ΠΎΠ² Π½Π° ΡΠ°ΠΌΠ΅ Π΄ΠΈΡΠΊΠΎΠ²ΠΎΠΉ Π±ΠΎΡΠΎΠ½Ρ, ΠΎΠ±Π΅ΡΠΏΠ΅ΡΠΈΠ²Π°ΡΡΠ΅Π΅ ΡΠΌΠ΅Π½ΡΡΠ΅Π½ΠΈΠ΅ Π½Π΅ΠΎΠ±Ρ
ΠΎΠ΄ΠΈΠΌΠΎΠ³ΠΎ ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²Π° Π΄ΠΈΡΠΊΠΎΠ² ΠΈ ΠΏΠΎΠ²ΡΡΠ΅Π½ΠΈΠ΅ ΠΊΠ°ΡΠ΅ΡΡΠ²Π° ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠΈ ΠΏΠΎΡΠ²Ρ. (ΠΠ°ΡΠ΅ΡΠΈΠ°Π»Ρ ΠΈ ΠΌΠ΅ΡΠΎΠ΄Ρ) ΠΡΠΏΠΎΠ»Π½ΠΈΠ»ΠΈ Π°Π½Π°Π»ΠΈΠ· ΡΠ°Π·ΠΌΠ΅ΡΠ΅Π½ΠΈΡ Π΄ΠΈΡΠΊΠΎΠ²ΡΡ
ΡΠ°Π±ΠΎΡΠΈΡ
ΠΎΡΠ³Π°Π½ΠΎΠ² Π±ΠΎΡΠΎΠ½Ρ ΠΈ Π²ΡΡΠ²ΠΈΠ»ΠΈ ΠΈΡ
ΡΠ°ΡΠΈΠΎΠ½Π°Π»ΡΠ½ΠΎΠ΅ ΡΠ°ΡΠΏΠΎΠ»ΠΎΠΆΠ΅Π½ΠΈΠ΅ ΠΈ Π²Π·Π°ΠΈΠΌΠ½ΡΡ ΠΎΡΠΈΠ΅Π½ΡΠ°ΡΠΈΡ Π² ΡΡΠ΄Π°Ρ
, ΡΠ²Π΅Π»ΠΈΡΠΈΠ²Π°ΡΡΠΈΠ΅ ΡΠΈΡΠΈΠ½Ρ ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠΈ ΡΠΌΠ΅ΠΆΠ½ΡΡ
ΠΏΠΎΠ»ΠΎΡ ΠΏΠΎΡΠ²Ρ, ΡΠ»ΡΡΡΠ°ΡΡΠΈΠ΅ ΠΏΠΎΠ»Π½ΠΎΡΡ ΠΏΠΎΠ΄ΡΠ΅Π·Π°Π½ΠΈΡ ΠΈ ΡΡΡ
Π»Π΅Π½ΠΈΡ ΠΏΠ»Π°ΡΡΠ° ΠΏΠΎ Π²ΡΠ΅ΠΉ ΡΠΈΡΠΈΠ½Π΅ Π·Π°Ρ
Π²Π°ΡΠ° ΠΏΡΠΈ ΡΠΌΠ΅Π½ΡΡΠ΅Π½ΠΈΠΈ Π½Π΅ΠΎΠ±Ρ
ΠΎΠ΄ΠΈΠΌΠΎΠ³ΠΎ ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²Π° Π΄ΠΈΡΠΊΠΎΠ². (Π Π΅Π·ΡΠ»ΡΡΠ°ΡΡ ΠΈ ΠΎΠ±ΡΡΠΆΠ΄Π΅Π½ΠΈΠ΅) Π£ΡΡΠ°Π½ΠΎΠ²ΠΈΠ»ΠΈ ΡΠ°ΠΊΠΎΠ΅ Π²Π·Π°ΠΈΠΌΠ½ΠΎΠ΅ ΡΠ°Π·ΠΌΠ΅ΡΠ΅Π½ΠΈΠ΅ Π΄ΠΈΡΠΊΠΎΠ² Π² ΠΈΡ
ΡΡΠ΄Π°Ρ
, ΠΏΡΠΈ ΠΊΠΎΡΠΎΡΠΎΠΌ ΡΠ»ΡΡΡΠ°Π΅ΡΡΡ ΡΠ΄Π²ΠΈΠ³ ΠΏΠΎΡΠ²Ρ, ΠΏΠΎΠ²ΡΡΠ°Π΅ΡΡΡ ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²ΠΎ ΠΏΠΎΠ»ΠΎΡΠΎΠΊ, ΠΎΠ±ΡΠ°Π±Π°ΡΡΠ²Π°Π΅ΠΌΡΡ
Π² ΡΠ²Π°Π» ΡΠΌΠ΅ΠΆΠ½ΡΠΌΠΈ Π΄ΠΈΡΠΊΠ°ΠΌΠΈ. ΠΠΎΠΊΠ°Π·Π°Π»ΠΈ, ΡΡΠΎ ΡΠ°Π·ΠΌΠ΅ΡΠ΅Π½ΠΈΠ΅ ΡΠ°Π±ΠΎΡΠΈΡ
ΠΎΡΠ³Π°Π½ΠΎΠ² ΠΏΠΎΡΠ»Π΅Π΄ΡΡΡΠ΅Π³ΠΎ ΡΡΠ΄Π° Ρ ΡΡΠ΅ΡΠΎΠΌ ΠΎΡΠΈΠ΅Π½ΡΠ°ΡΠΈΠΈ ΡΠΌΠ΅ΠΆΠ½ΡΡ
Π΄ΠΈΡΠΊΠΎΠ² ΠΏΡΠ΅Π΄ΡΠ΄ΡΡΠ΅Π³ΠΎ ΠΏΠΎΠ·Π²ΠΎΠ»ΡΠ΅Ρ ΠΏΡΠΈ ΠΏΠΎΠ»Π½ΠΎΠΌ ΠΏΠΎΠ΄ΡΠ΅Π·Π°Π½ΠΈΠΈ ΠΏΠΎΡΠ²Ρ ΠΏΠΎ Π²ΡΠ΅ΠΉ ΡΠΈΡΠΈΠ½Π΅ Π·Π°Ρ
Π²Π°ΡΠ° Π΄ΠΈΡΠΊΠΎΠ²ΠΎΠΉ Π±ΠΎΡΠΎΠ½Ρ ΡΠΊΠΎΠ½ΠΎΠΌΠΈΡΡ ΠΎΠ΄ΠΈΠ½ ΡΠ°Π±ΠΎΡΠΈΠΉ ΠΎΡΠ³Π°Π½ Π½Π° ΠΊΠ°ΠΆΠ΄ΡΠ΅ 400 ΠΌΠΈΠ»Π»ΠΈΠΌΠ΅ΡΡΠΎΠ²Β ΡΠΈΡΠΈΠ½Ρ Π΅Π΅ Π·Π°Ρ
Π²Π°ΡΠ°. (ΠΡΠ²ΠΎΠ΄Ρ) ΠΡΡΠ²ΠΈΠ»ΠΈ, ΡΡΠΎ ΠΏΡΠΈ ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠ΅ ΠΏΠΎΡΠ²Ρ Π΄ΠΈΡΠΊΠΎΠΌ Ρ ΠΏΠ΅ΡΠ΅ΠΌΠ΅ΡΠ΅Π½ΠΈΠ΅ΠΌ Π΅Π΅ Π² ΡΡΠΎΡΠΎΠ½Ρ ΡΠΆΠ΅ ΠΎΠ±ΡΠ°Π±ΠΎΡΠ°Π½Π½ΠΎΠΉ ΡΠΌΠ΅ΠΆΠ½ΠΎΠΉ ΠΏΠΎΠ»ΠΎΡΡ ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠ°Ρ ΡΠΈΡΠΈΠ½Π° Π·Π°Ρ
Π²Π°ΡΠ° Π΄ΠΈΡΠΊΠ° ΡΠ²Π΅Π»ΠΈΡΠΈΠ²Π°Π΅ΡΡΡ Π·Π° ΡΡΠ΅Ρ ΠΏΡΠΎΡΠ²Π»Π΅Π½ΠΈΡ Π΄Π΅ΡΠΎΡΠΌΠ°ΡΠΈΠΈ ΠΎΡΡΡΠ²Π° ΠΈ ΡΠ΄Π²ΠΈΠ³Π° ΠΏΠΎΡΠ²Ρ. ΠΡΠ΅Π΄Π»ΠΎΠΆΠΈΠ»ΠΈ ΠΏΠΎΡΡΠ΄ΠΎΠΊ ΡΠ°ΡΠΏΠΎΠ»ΠΎΠΆΠ΅Π½ΠΈΡ ΡΡΠ΅ΡΠΈΡΠ΅ΡΠΊΠΈΡ
Π΄ΠΈΡΠΊΠΎΠ² ΠΈ ΠΈΡ
Π²Π·Π°ΠΈΠΌΠ½ΡΡ ΠΎΡΠΈΠ΅Π½ΡΠ°ΡΠΈΡ, ΠΏΠΎΠ²ΡΡΠ°ΡΡΠΈΠ΅ ΠΊΠ°ΡΠ΅ΡΡΠ²ΠΎ ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠΈ ΠΏΠΎΡΠ²Ρ, ΠΏΠΎΠ»Π½ΠΎΡΡ ΠΏΠΎΠ΄ΡΠ΅Π·Π°Π½ΠΈΡ ΠΏΠΎ Π²ΡΠ΅ΠΉ ΡΠΈΡΠΈΠ½Π΅ Π·Π°Ρ
Π²Π°ΡΠ°, Π° ΡΠ°ΠΊΠΆΠ΅ Π²ΠΎΠ·ΠΌΠΎΠΆΠ½ΠΎΡΡΡ ΡΠΌΠ΅Π½ΡΡΠ΅Π½ΠΈΡ ΠΈΡ
ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²Π°
Hilbert space of wormholes
Wormhole boundary conditions for the Wheeler--DeWitt equation can be derived
from the path integral formulation. It is proposed that the wormhole wave
function must be square integrable in the maximal analytic extension of
minisuperspace. Quantum wormholes can be invested with a Hilbert space
structure, the inner product being naturally induced by the minisuperspace
metric, in which the Wheeler--DeWitt operator is essentially self--adjoint.
This provides us with a kind of probabilistic interpretation. In particular,
giant wormholes will give extremely small contributions to any wormhole state.
We also study the whole spectrum of the Wheeler--DeWitt operator and its role
in the calculation of Green's functions and effective low energy interactions.Comment: 23 pages, 2 figures available upon request, REVTE
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