793 research outputs found
Quark-diquark model for p(\bar p)-p elastic scattering at high energies
A model for elastic scattering of protons at high energies based on the
quark-diquark representation of the proton is discussed. The predictions of the
model are compared with experimental data for the differential elastic
cross-sections from available databasesComment: 4 pages, 5 figure
Study of non-collinear parton dynamics in the prompt photon photoproduction at HERA
We investigate the prompt photon photoproduction at HERA within the framework
of kt-factorization QCD approach. Our consideration is based on the off-shell
matrix elements for the underlying partonic subprocesses. The unintegrated
parton densities in a proton and in a photon are determined using the
Kimber-Martin-Ryskin (KMR) prescription. Additionally, we use the CCFM-evolved
unintegrated gluon as well as valence and sea quark distributions in a proton.
A conservative error analisys is performed. Both inclusive and associated with
the hadronic jet production rates are investigated. The theoretical results are
compared with the recent experimental data taken by the H1 and ZEUS
collaborations. We study also the specific kinematical properties of the
photon-jet system which are strongly sensitive to the transverse momentum of
incoming partons. Using the KMR scheme, the contribution from the quarks
emerging from the earlier steps of the parton evolution is estimated and found
to be of 15 - 20 approximately.Comment: 22 pages, 13 figures, 2 tabl
ΠΠΎΠ²ΡΠ΅ ΡΠ΅Ρ Π½ΠΎΠ»ΠΎΠ³ΠΈΠΈ ΡΠΏΡΠ°Π²Π»Π΅Π½ΠΈΡ ΡΠΈΠ½Π°Π½ΡΠΈΡΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΈΠ½Π½ΠΎΠ²Π°ΡΠΈΠΉ Π² ΠΏΡΠΎΠΌΡΡΠ»Π΅Π½Π½ΠΎΡΡΠΈ
The subject of the study is new technologies for managing industrial innovation funding. The aim of the article is to form an optimal mechanism for the application of technologies for managing industrial innovation funding based on the use of new financial instruments. The relevance of the research is due to the increasing role of innovation in ensuring competitive advantages and market stability of industrial enterprises, as well as the growing need to attract funding. The scientific novelty consists in grouping the existing financing technologies into three main groups: traditional, modern and new. The research methods are analysis, systematization, synthesis, induction, deduction, modeling. The authors built a model of the mutual influence of innovative industrial development and the subsequent development of financing technologies in the financial sector. In the course of the study, the author obtained the following results: a mechanism for applying new technologies to manage innovation funding was developed, a priority financial instrument was identified for use within the framework of the developed mechanism. The authors conclude that the role of digital technologies in the activities of an industrial enterprise and, accordingly, in innovation funding is increasing. At the same time, the activities of an enterprise in attracting resources by issuing digital securities (shares) to finance innovations are of the greatest practical interest.ΠΡΠ΅Π΄ΠΌΠ΅ΡΠΎΠΌ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ Π²ΡΡΡΡΠΏΠ°ΡΡ Π½ΠΎΠ²ΡΠ΅ ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΠΈ ΡΠΏΡΠ°Π²Π»Π΅Π½ΠΈΡ ΡΠΈΠ½Π°Π½ΡΠΈΡΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΈΠ½Π½ΠΎΠ²Π°ΡΠΈΠΉ Π² ΠΏΡΠΎΠΌΡΡΠ»Π΅Π½Π½ΠΎΡΡΠΈ. Π¦Π΅Π»ΡΡ ΡΠ°Π±ΠΎΡΡ ΡΠ²Π»ΡΠ΅ΡΡΡ ΡΠΎΡΠΌΠΈΡΠΎΠ²Π°Π½ΠΈΠ΅ ΠΎΠΏΡΠΈΠΌΠ°Π»ΡΠ½ΠΎΠ³ΠΎ ΠΌΠ΅Ρ
Π°Π½ΠΈΠ·ΠΌΠ° ΠΏΡΠΈΠΌΠ΅Π½Π΅Π½ΠΈΡ ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΠΉ ΡΠΏΡΠ°Π²Π»Π΅Π½ΠΈΡ ΡΠΈΠ½Π°Π½ΡΠΈΡΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΈΠ½Π½ΠΎΠ²Π°ΡΠΈΠΉ Π² ΠΏΡΠΎΠΌΡΡΠ»Π΅Π½Π½ΠΎΡΡΠΈ Π½Π° ΠΎΡΠ½ΠΎΠ²Π΅ ΠΏΡΠΈΠΌΠ΅Π½Π΅Π½ΠΈΡ Π½ΠΎΠ²ΡΡ
ΡΠΈΠ½Π°Π½ΡΠΎΠ²ΡΡ
ΠΈΠ½ΡΡΡΡΠΌΠ΅Π½ΡΠΎΠ². ΠΠΊΡΡΠ°Π»ΡΠ½ΠΎΡΡΡ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ ΠΎΠ±ΡΡΠ»ΠΎΠ²Π»Π΅Π½Π° Π²ΠΎΠ·ΡΠ°ΡΡΠ°Π½ΠΈΠ΅ΠΌ ΡΠΎΠ»ΠΈ ΠΈΠ½Π½ΠΎΠ²Π°ΡΠΈΠΉ Π² ΠΎΠ±Π΅ΡΠΏΠ΅ΡΠ΅Π½ΠΈΠΈ ΠΊΠΎΠ½ΠΊΡΡΠ΅Π½ΡΠ½ΡΡ
ΠΏΡΠ΅ΠΈΠΌΡΡΠ΅ΡΡΠ² ΠΈ ΡΡΠ½ΠΎΡΠ½ΠΎΠΉ ΡΡΡΠΎΠΉΡΠΈΠ²ΠΎΡΡΠΈ ΠΏΡΠΎΠΌΡΡΠ»Π΅Π½Π½ΡΡ
ΠΏΡΠ΅Π΄ΠΏΡΠΈΡΡΠΈΠΉ, Π° ΡΠ°ΠΊΠΆΠ΅ Π²ΠΎΠ·ΡΠ°ΡΡΠ°Π½ΠΈΠ΅ΠΌ ΠΏΠΎΡΡΠ΅Π±Π½ΠΎΡΡΠΈ Π² ΠΏΡΠΈΠ²Π»Π΅ΡΠ΅Π½ΠΈΠΈ ΡΠΈΠ½Π°Π½ΡΠΈΡΠΎΠ²Π°Π½ΠΈΡ. ΠΠ°ΡΡΠ½Π°Ρ Π½ΠΎΠ²ΠΈΠ·Π½Π° ΡΠΎΡΡΠΎΠΈΡ Π² Π³ΡΡΠΏΠΏΠΈΡΠΎΠ²ΠΊΠ΅ ΠΏΡΠΈΠΌΠ΅Π½ΡΠ΅ΠΌΡΡ
Π½Π° Π½Π°ΡΡΠΎΡΡΠΈΠΉ ΠΌΠΎΠΌΠ΅Π½Ρ ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΠΉ ΡΠΈΠ½Π°Π½ΡΠΈΡΠΎΠ²Π°Π½ΠΈΡ Π½Π° ΡΡΠΈ ΠΎΡΠ½ΠΎΠ²Π½ΡΠ΅ Π³ΡΡΠΏΠΏΡ: ΡΡΠ°Π΄ΠΈΡΠΈΠΎΠ½Π½ΡΠ΅, ΡΠΎΠ²ΡΠ΅ΠΌΠ΅Π½Π½ΡΠ΅ ΠΈ Π½ΠΎΠ²ΡΠ΅. ΠΠ΅ΡΠΎΠ΄Π°ΠΌΠΈ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ Π²ΡΡΡΡΠΏΠ°ΡΡ: Π°Π½Π°Π»ΠΈΠ·, ΡΠΈΡΡΠ΅ΠΌΠ°ΡΠΈΠ·Π°ΡΠΈΡ, ΡΠΈΠ½ΡΠ΅Π·, ΠΈΠ½Π΄ΡΠΊΡΠΈΡ, Π΄Π΅Π΄ΡΠΊΡΠΈΡ, ΠΌΠΎΠ΄Π΅Π»ΠΈΡΠΎΠ²Π°Π½ΠΈΠ΅. ΠΡΠΈ ΡΡΠΎΠΌ ΡΠ°Π·ΡΠ°Π±ΠΎΡΠ°Π½Π° ΠΌΠΎΠ΄Π΅Π»Ρ Π²Π·Π°ΠΈΠΌΠ½ΠΎΠ³ΠΎ Π²Π»ΠΈΡΠ½ΠΈΡ ΠΈΠ½Π½ΠΎΠ²Π°ΡΠΈΠΎΠ½Π½ΠΎΠ³ΠΎ ΡΠ°Π·Π²ΠΈΡΠΈΡ Π² ΠΏΡΠΎΠΌΡΡΠ»Π΅Π½Π½ΠΎΡΡΠΈ ΠΈ ΠΏΠΎΡΠ»Π΅Π΄ΡΡΡΠ΅Π³ΠΎ ΡΠ°Π·Π²ΠΈΡΠΈΡ ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΠΉ ΡΠΈΠ½Π°Π½ΡΠΈΡΠΎΠ²Π°Π½ΠΈΡ Π² ΡΠΈΠ½Π°Π½ΡΠΎΠ²ΠΎΠΌ ΡΠ΅ΠΊΡΠΎΡΠ΅. Π Ρ
ΠΎΠ΄Π΅ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ Π°Π²ΡΠΎΡΡ ΠΏΠΎΠ»ΡΡΠΈΠ»ΠΈ ΡΠ»Π΅Π΄ΡΡΡΠΈΠ΅ ΡΠ΅Π·ΡΠ»ΡΡΠ°ΡΡ: ΡΠ°Π·ΡΠ°Π±ΠΎΡΠ°Π½ ΠΌΠ΅Ρ
Π°Π½ΠΈΠ·ΠΌ ΠΏΡΠΈΠΌΠ΅Π½Π΅Π½ΠΈΡ Π½ΠΎΠ²ΡΡ
ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΠΉ ΡΠΏΡΠ°Π²Π»Π΅Π½ΠΈΡ ΡΠΈΠ½Π°Π½ΡΠΈΡΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΈΠ½Π½ΠΎΠ²Π°ΡΠΈΠΉ, ΠΎΠΏΡΠ΅Π΄Π΅Π»Π΅Π½ ΠΏΡΠΈΠΎΡΠΈΡΠ΅ΡΠ½ΡΠΉ ΡΠΈΠ½Π°Π½ΡΠΎΠ²ΡΠΉ ΠΈΠ½ΡΡΡΡΠΌΠ΅Π½Ρ Π΄Π»Ρ ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½ΠΈΡ Π² ΡΠ°ΠΌΠΊΠ°Ρ
ΡΠ°Π·ΡΠ°Π±ΠΎΡΠ°Π½Π½ΠΎΠ³ΠΎ ΠΌΠ΅Ρ
Π°Π½ΠΈΠ·ΠΌΠ°. ΠΠ²ΡΠΎΡΡ Π΄Π΅Π»Π°ΡΡ Π²ΡΠ²ΠΎΠ΄ ΠΎ Π²ΠΎΠ·ΡΠ°ΡΡΠ°Π½ΠΈΠΈ ΡΠΎΠ»ΠΈ ΡΠΈΡΡΠΎΠ²ΡΡ
ΡΠ΅Ρ
Π½ΠΎΠ»ΠΎΠ³ΠΈΠΉ Π² Π΄Π΅ΡΡΠ΅Π»ΡΠ½ΠΎΡΡΠΈ ΠΏΡΠΎΠΌΡΡΠ»Π΅Π½Π½ΠΎΠ³ΠΎ ΠΏΡΠ΅Π΄ΠΏΡΠΈΡΡΠΈΡ ΠΈ, ΡΠΎΠΎΡΠ²Π΅ΡΡΡΠ²Π΅Π½Π½ΠΎ, Π² ΡΠΈΠ½Π°Π½ΡΠΈΡΠΎΠ²Π°Π½ΠΈΠΈ ΠΈΠ½Π½ΠΎΠ²Π°ΡΠΈΠΎΠ½Π½ΠΎΠΉ Π΄Π΅ΡΡΠ΅Π»ΡΠ½ΠΎΡΡΠΈ. ΠΡΠΈ ΡΡΠΎΠΌ Π½Π°ΠΈΠ±ΠΎΠ»ΡΡΠΈΠΉ ΠΏΡΠ°ΠΊΡΠΈΡΠ΅ΡΠΊΠΈΠΉ ΠΈΠ½ΡΠ΅ΡΠ΅Ρ ΠΏΡΠ΅Π΄ΡΡΠ°Π²Π»ΡΠ΅Ρ Π΄Π΅ΡΡΠ΅Π»ΡΠ½ΠΎΡΡΡ ΠΏΡΠ΅Π΄ΠΏΡΠΈΡΡΠΈΡ ΠΏΠΎ ΠΏΡΠΈΠ²Π»Π΅ΡΠ΅Π½ΠΈΡ ΡΠ΅ΡΡΡΡΠΎΠ² ΠΏΠΎΡΡΠ΅Π΄ΡΡΠ²ΠΎΠΌ Π²ΡΠΏΡΡΠΊΠ° ΡΠΈΡΡΠΎΠ²ΡΡ
ΡΠ΅Π½Π½ΡΡ
Π±ΡΠΌΠ°Π³ (Π°ΠΊΡΠΈΠΉ) Π΄Π»Ρ ΡΠΈΠ½Π°Π½ΡΠΈΡΠΎΠ²Π°Π½ΠΈΡ ΠΈΠ½Π½ΠΎΠ²Π°ΡΠΈΠΉ
Region of Excessive Flux of PeV Cosmic Rays in the Direction Toward Pulsars PSR J1840+5640 and LAT PSR J1836+5925
An analysis of arrival directions of extensive air showers (EAS) registered
with the EAS MSU and EAS-1000 prototype arrays has revealed a region of
excessive flux of PeV cosmic rays in the direction toward pulsars PSR
J1840+5640 and LAT PSR J1836+5925 at significance level up to 4.5sigma. The
first of the pulsars was discovered almost 30 years ago and is a well-studied
old radio pulsar located at the distance of 1.7pc from the Solar system. The
second pulsar belongs to a new type of pulsars, discovered by the space
gamma-ray observatory Fermi, pulsations of which are not observed in optical
and radio wavelengths but only in the gamma-ray range of energies
(gamma-ray-only pulsars). In our opinion, the existence of the region of
excessive flux of cosmic rays registered with two different arrays provides a
strong evidence that isolated pulsars can give a noticeable contribution to the
flux of Galactic cosmic rays in the PeV energy range.Comment: 14 pages; v.2: a few remarks to match a version accepted for
Astronomy Letters added. They can be found by redefining the \NEW command in
the preamble of the LaTeX fil
Strong-Pinning Effects in Low-Temperature Creep: Charge-Density Waves in TaS_3
Nonlinear conduction in the quasi-one dimensional conductor o-TaS_3 has been
studied in the low-temperature region down to 30 mK. It was found that at
temperatures below a few Kelvins the current-voltage (I-V) characteristics
consist of several branches. The temperature evolution of the I-V curve
proceeds through sequential freezing-out of the branches. The origin of each
branch is attributed to a particular strong pinning impurity type.
Similar behavior is expected for other physical systems with collective
transport (spin-density waves, Wigner crystals, vortex lattices in type-II
superconductors etc.) in the presence of strong pinning centers.Comment: 11 pages, 3 ps figures, Revtex, To be published in Phys. Rev. Letters
(1997
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