50 research outputs found
A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model
We discuss various aspects of the inner structure formation in virialized
dark matter (DM) halos that form as primordial density inhomogeneities evolve
in the cosmological standard model. The main focus is on the study of central
cusps/cores and of the profiles of DM halo rotation curves, problems that
reveal disagreements among the theory, numerical simulations, and observations.
A method that was developed by the authors to describe equilibrium DM systems
is presented, which allows investigating these complex nonlinear structures
analytically and relating density distribution profiles within a halo both to
the parameters of the initial small-scale inhomogeneity field and to the
nonlinear relaxation characteristics of gravitationally compressed matter. It
is shown that cosmological random motions of matter `heat up' the DM particles
in collapsing halos, suppressing cusp-like density profiles within developing
halos, facilitating the formation of DM cores in galaxies, and providing an
explanation for the difference between observed and simulated galactic rotation
curves. The analytic conclusions obtained within this approach can be confirmed
by the N-body model simulation once improved spatial resolution is achieved for
central halo regions.Comment: 44 pages, 16 figures, 1 tabl
Current-induced highly dissipative domains in high Tc thin films
We have investigated the resistive response of high Tc thin films submitted
to a high density of current. For this purpose, current pulses were applied
into bridges made of Nd(1.15)Ba(1.85)Cu3O7 and Bi2Sr2CaCu2O8. By recording the
time dependent voltage, we observe that at a certain critical current j*, a
highly dissipative domain develops somewhere along the bridge. The successive
formation of these domains produces stepped I-V characteristics. We present
evidences that these domains are not regions with a temperature above Tc, as
for hot spots. In fact this phenomenon appears to be analog to the nucleation
of phase-slip centers observed in conventional superconductors near Tc, but
here in contrast they appear in a wide temperature range. Under some
conditions, these domains will propagate and destroy the superconductivity
within the whole sample. We have measured the temperature dependence of j* and
found a similar behavior in the two investigated compounds. This temperature
dependence is just the one expected for the depairing current, but the
amplitude is about 100 times smaller.Comment: 9 pages, 9 figures, Revtex, to appear in Phys. Rev.
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Energetic particle influence on the Earth's atmosphere
This manuscript gives an up-to-date and comprehensive overview of the effects of energetic particle precipitation (EPP) onto the whole atmosphere, from the lower thermosphere/mesosphere through the stratosphere and troposphere, to the surface. The paper summarizes the different sources and energies of particles, principally
galactic cosmic rays (GCRs), solar energetic particles (SEPs) and energetic electron precipitation (EEP). All the proposed mechanisms by which EPP can affect the atmosphere
are discussed, including chemical changes in the upper atmosphere and lower thermosphere, chemistry-dynamics feedbacks, the global electric circuit and cloud formation. The role of energetic particles in Earthβs atmosphere is a multi-disciplinary problem that requires expertise from a range of scientific backgrounds. To assist with this synergy, summary tables are provided, which are intended to evaluate the level of current knowledge of the effects of energetic particles on processes in the entire atmosphere
Mitral insufficiency: systematization, conservative and surgical treatment
The article concerns mechanisms, clinical features, diagnostics, possible complications and treatment of mitral insufficiency. Much attention is given to modern diagnostic methods, principles for case management and indications for surgical treatment
ΠΡΠΎΠ±Π΅Π½Π½ΠΎΡΡΠΈ ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΠΈ ΠΊΠΎΠ»Π»Π°Π³Π΅Π½Π° IV ΡΠΈΠΏΠ° Π² Π±Π°Π·Π°Π»ΠΈΠΎΠΌΠ΅ ΠΊΠΎΠΆΠΈ
Rationale: Type IV collagen is the main component of the basal membrane ensuring its integrity. Basal membrane destruction is associated with absent type IV collagen expression being directly related to an increased tumor invasion risk. Specifics of the protein expression in various morphological types of basal cell carcinoma have not been well described. Aim: To study the association between type IV collagen expression and basal cell carcinoma morphological structure and invasion potential. Materials and methods: We performed an immunohistochemistry analysis with anti-type IV collagen antibodies on 30 biopsy specimens of the skin involved with basal cell carcinoma. Results: The superficial multicentric type of basal cell carcinoma differed from the solid, micronodular, and infiltrative types by linear continuous type IV collagen expression (Ρ 0.0083). Most often, there was no type IV collagen expression in the micronodular and infiltrative basal cell carcinomas; however, no significant difference of the solid type and each of the abovementioned types was found. Aggressive basal cell carcinoma types (micronodular and infiltrative, taken together) were significantly different (Ρ = 0.033) from the solid type by the absence of type IV collagen expression. Linear continuous expression was seen exclusively in basal cell carcinomas with the invasion of 0.825 mm. Conclusion: We have identified the difference in type IV collagen expression depending on the morphological type of basal cell skin carcinoma, prevailing linear continuous expression in the superficial multicentric type and its absence in the micronodular and infiltrative types.ΠΠΊΡΡΠ°Π»ΡΠ½ΠΎΡΡΡ. ΠΠΎΠ»Π»Π°Π³Π΅Π½ IV ΡΠΈΠΏΠ° - ΠΎΡΠ½ΠΎΠ²Π½ΠΎΠΉ ΠΊΠΎΠΌΠΏΠΎΠ½Π΅Π½Ρ Π±Π°Π·Π°Π»ΡΠ½ΠΎΠΉ ΠΌΠ΅ΠΌΠ±ΡΠ°Π½Ρ, ΠΎΠ±Π΅ΡΠΏΠ΅ΡΠΈΠ²Π°ΡΡΠΈΠΉ Π΅Π΅ ΡΠ΅Π»ΠΎΡΡΠ½ΠΎΡΡΡ. ΠΡΠΈ ΡΠ°Π·ΡΡΡΠ΅Π½ΠΈΠΈ Π±Π°Π·Π°Π»ΡΠ½ΠΎΠΉ ΠΌΠ΅ΠΌΠ±ΡΠ°Π½Ρ ΠΎΡΠΌΠ΅ΡΠ°Π΅ΡΡΡ ΠΈΡΡΠ΅Π·Π½ΠΎΠ²Π΅Π½ΠΈΠ΅ ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΠΈ ΠΊΠΎΠ»Π»Π°Π³Π΅Π½Π° IV ΡΠΈΠΏΠ°, ΡΡΠΎ Π½Π°ΠΏΡΡΠΌΡΡ ΡΠ²ΡΠ·Π°Π½ΠΎ Ρ Π²ΠΎΠ·ΡΠ°ΡΡΠ°Π½ΠΈΠ΅ΠΌ ΠΈΠ½Π²Π°Π·ΠΈΠ²Π½ΠΎΠ³ΠΎ ΠΏΠΎΡΠ΅Π½ΡΠΈΠ°Π»Π° ΠΎΠΏΡΡ
ΠΎΠ»ΠΈ. Π ΠΏΠΎΠ»Π½ΠΎΠΉ ΠΌΠ΅ΡΠ΅ Π½Π΅ ΠΎΠΏΡΠ΅Π΄Π΅Π»Π΅Π½Ρ ΠΎΡΠΎΠ±Π΅Π½Π½ΠΎΡΡΠΈ ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΠΈ ΡΡΠΎΠ³ΠΎ Π±Π΅Π»ΠΊΠ° ΠΏΡΠΈ ΡΠ°Π·Π»ΠΈΡΠ½ΡΡ
ΠΌΠΎΡΡΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΈΡ
ΡΠΈΠΏΠ°Ρ
Π±Π°Π·Π°Π»ΠΈΠΎΠΌΡ. Π¦Π΅Π»Ρ - ΠΈΠ·ΡΡΠ΅Π½ΠΈΠ΅ Π²Π·Π°ΠΈΠΌΠΎΡΠ²ΡΠ·ΠΈ ΠΌΠ΅ΠΆΠ΄Ρ ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΠ΅ΠΉ ΠΊΠΎΠ»Π»Π°Π³Π΅Π½Π° IV ΡΠΈΠΏΠ°, ΠΌΠΎΡΡΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΈΠΌ ΡΡΡΠΎΠ΅Π½ΠΈΠ΅ΠΌ ΠΈ ΠΈΠ½Π²Π°Π·ΠΈΠ²Π½ΡΠΌ ΠΏΠΎΡΠ΅Π½ΡΠΈΠ°Π»ΠΎΠΌ Π±Π°Π·Π°Π»ΠΈΠΎΠΌΡ. ΠΠ°ΡΠ΅ΡΠΈΠ°Π» ΠΈ ΠΌΠ΅ΡΠΎΠ΄Ρ. ΠΡΠΎΠ²Π΅Π΄Π΅Π½ΠΎ ΠΈΠΌΠΌΡΠ½ΠΎΠ³ΠΈΡΡΠΎΡ
ΠΈΠΌΠΈΡΠ΅ΡΠΊΠΎΠ΅ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΠ΅ Ρ Π°Π½ΡΠΈΡΠ΅Π»Π°ΠΌΠΈ ΠΊ ΠΊΠΎΠ»Π»Π°Π³Π΅Π½Ρ IV ΡΠΈΠΏΠ° Π±ΠΈΠΎΠΏΡΠΈΠΉΠ½ΠΎΠ³ΠΎ ΠΌΠ°ΡΠ΅ΡΠΈΠ°Π»Π° 30 Π±Π°Π·Π°Π»ΠΈΠΎΠΌ ΠΊΠΎΠΆΠΈ. Π Π΅Π·ΡΠ»ΡΡΠ°ΡΡ. ΠΠΈΠ½Π΅ΠΉΠ½Π°Ρ Π½Π΅ΠΏΡΠ΅ΡΡΠ²Π½Π°Ρ ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΡ ΠΊΠΎΠ»Π»Π°Π³Π΅Π½Π° IV ΡΠΈΠΏΠ° ΠΎΡΠ»ΠΈΡΠ°Π»Π° (Ρ 0,0083) ΠΏΠΎΠ²Π΅ΡΡ
Π½ΠΎΡΡΠ½ΡΠΉ ΠΌΡΠ»ΡΡΠΈ-ΡΠ΅Π½ΡΡΠΈΡΠ΅ΡΠΊΠΈΠΉ ΡΠΈΠΏ ΠΎΡ ΡΠΎΠ»ΠΈΠ΄Π½ΠΎΠ³ΠΎ, ΠΌΠΈΠΊΡΠΎΠ½ΠΎΠ΄ΡΠ»ΡΡΠ½ΠΎΠ³ΠΎ ΠΈ ΠΈΠ½ΡΠΈΠ»ΡΡΡΠ°ΡΠΈΠ²Π½ΠΎΠ³ΠΎ. Π ΠΌΠΈΠΊΡΠΎΠ½ΠΎΠ΄ΡΠ»ΡΡΠ½ΠΎΠΌ ΠΈ ΠΈΠ½ΡΠΈΠ»ΡΡΡΠ°ΡΠΈΠ²Π½ΠΎΠΌ ΡΠΈΠΏΠ°Ρ
Π±Π°Π·Π°Π»ΠΈΠΎΠΌΡ ΡΠ°ΡΠ΅ Π²ΡΠ΅Π³ΠΎ ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΡ ΠΊΠΎΠ»Π»Π°Π³Π΅Π½Π° IV ΠΎΡΡΡΡΡΡΠ²ΠΎΠ²Π°Π»Π°, ΠΎΠ΄Π½Π°ΠΊΠΎ ΡΡΠ°ΡΠΈΡΡΠΈΡΠ΅ΡΠΊΠΈ Π·Π½Π°ΡΠΈΠΌΠΎΠ³ΠΎ ΠΎΡΠ»ΠΈΡΠΈΡ ΡΠΎΠ»ΠΈΠ΄Π½ΠΎΠ³ΠΎ ΠΎΡ ΠΊΠ°ΠΆΠ΄ΠΎΠ³ΠΎ ΠΈΠ· ΡΡΠΈΡ
ΡΠΈΠΏΠΎΠ² ΠΏΠΎΠ»ΡΡΠ΅Π½ΠΎ Π½Π΅ Π±ΡΠ»ΠΎ. Π‘ΡΠΌΠΌΠ°ΡΠ½ΠΎ Π°Π³ΡΠ΅ΡΡΠΈΠ²Π½ΡΠ΅ ΡΠΈΠΏΡ Π±Π°Π·Π°Π»ΠΈΠΎΠΌΡ (ΠΌΠΈΠΊΡΠΎΠ½ΠΎΠ΄ΡΠ»ΡΡΠ½ΡΠΉ ΠΈ ΠΈΠ½ΡΠΈΠ»ΡΡΡΠ°ΡΠΈΠ²Π½ΡΠΉ) Π·Π½Π°ΡΠΈΠΌΠΎ (Ρ = 0,033) ΠΎΡΠ»ΠΈΡΠ°Π»ΠΈΡΡ ΠΎΡ ΡΠΎΠ»ΠΈΠ΄Π½ΠΎΠ³ΠΎ ΡΠ΅ΠΌ, ΡΡΠΎ Π² Π½ΠΈΡ
ΠΏΡΠ΅ΠΈΠΌΡΡΠ΅ΡΡΠ²Π΅Π½Π½ΠΎ ΠΎΡΡΡΡΡΡΠ²ΠΎΠ²Π°Π»Π° ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΡ ΠΊΠΎΠ»Π»Π°Π³Π΅Π½Π° IV ΡΠΈΠΏΠ°. ΠΡΠΊΠ»ΡΡΠΈΡΠ΅Π»ΡΠ½ΠΎ Π»ΠΈΠ½Π΅ΠΉΠ½Π°Ρ Π½Π΅ΠΏΡΠ΅ΡΡΠ²Π½Π°Ρ ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΡ Π½Π°Π±Π»ΡΠ΄Π°Π»Π°ΡΡ Π² Π±Π°Π·Π°Π»ΠΈΠΎΠΌΠ°Ρ
Π³Π»ΡΠ±ΠΈΠ½ΠΎΠΉ 0,825 ΠΌΠΌ. ΠΠ°ΠΊΠ»ΡΡΠ΅Π½ΠΈΠ΅. Π£ΡΡΠ°Π½ΠΎΠ²Π»Π΅Π½Ρ ΡΠ°Π·Π»ΠΈΡΠΈΡ Π² ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΠΈ ΠΊΠΎΠ»Π»Π°Π³Π΅Π½Π° IV ΡΠΈΠΏΠ° Π² Π·Π°Π²ΠΈΡΠΈΠΌΠΎΡΡΠΈ ΠΎΡ ΠΌΠΎΡΡΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΎΠ³ΠΎ ΡΠΈΠΏΠ° Π±Π°Π·Π°Π»ΠΈΠΎΠΌΡ, ΠΏΡΠ΅ΠΎΠ±Π»Π°Π΄Π°Π½ΠΈΠ΅ Π»ΠΈΠ½Π΅ΠΉΠ½ΠΎΠΉ Π½Π΅ΠΏΡΠ΅ΡΡΠ²Π½ΠΎΠΉ ΡΠΊΡΠΏΡΠ΅ΡΡΠΈΠΈ Π² ΠΏΠΎΠ²Π΅ΡΡ
Π½ΠΎΡΡΠ½ΠΎΠΌ ΠΌΡΠ»ΡΡΠΈΡΠ΅Π½ΡΡΠΈΡΠ΅ΡΠΊΠΎΠΌ ΡΠΈΠΏΠ΅ ΠΈ Π΅Π΅ ΠΎΡΡΡΡΡΡΠ²ΠΈΠ΅ Π² ΠΌΠΈ-ΠΊΡΠΎΠ½ΠΎΠ΄ΡΠ»ΡΡΠ½ΠΎΠΌ ΠΈ ΠΈΠ½ΡΠΈΠ»ΡΡΡΠ°ΡΠΈΠ²Π½ΠΎΠΌ