ЭКСПЕРИМЕНТАЛЬНАЯ ОЦЕНКА КОМПОЗИЦИОННОГО МАТЕРИАЛА НА ОСНОВЕ БЕЛКОВО-МИНЕРАЛЬНЫХ КОМПОНЕНТОВ И РЕКОМБИНАНТНОГО КОСТНОГО МОРФОГЕНЕТИЧЕСКОГО БЕЛКА-2 В КАЧЕСТВЕ ПОКРЫТИЯ ТИТАНОВЫХ ИМПЛАНТАТОВ

The influence of both, the composite material based on the protein-mineral components including the prolonged form of the recombinant human bone morphogenetic protein 2 (rhBMP-2) and the method of the titanium implant’s surface treatment, on the reparative osteogenesis and adhesion strength of the bone tissue – implant’s surface contact was evaluated. Covering of implants with the composite coating promotes significant acceleration of the bone tissue regeneration processes in the site of implants loading. The composition coating with prolonged form of the rhBMP-2 promoted increasing of the neogenic bone tissue’s adhesion with the implants, as compared with the coating without recombinant human bone morphogenetic protein. The implants treated with microarc oxidation demonstrated higher values of the breakout force during the separation of the implants from the bone than the implants treated with sandblasting method.Проведена оценка влияния композиционного материала на основе белково-минеральных компонентов, содержащего пролонгированную форму рекомбинантного костного морфогенетического белка-2 человека (rhВМР-2), и способа обработки поверхности титанового имплантата на репаративный остеогенез и адгезионную прочность контакта костной ткани с поверхностью имплантата. Нанесение на имплантаты композиционного препарата/покрытия способствовало значительному ускорению процессов регенерации костной ткани в месте введения имплантатов. Композиционное покрытие с пролонгированной формой rhBMP-2, способствовало увеличению адгезионных связей новообразованной костной ткани с поверхностью образцов по сравнению с покрытием, не содержащим рекомбинантного костного морфогенетического белка. Имплантаты с поверхностью, обработанной с помощью микродугового оксидирования, демонстрировали более высокие значения величины усилия отрыва имплантата от кости, чем модифицированные пескоструйной обработкой

Gamma-ray families with halos: Main characteristics and possibilities of using them to estimate the p+He fraction in the mass composition of cosmic rays at energies 1–100 PeV

Characteristics of γ-ray families with halos (XREC, Pamir) and data of experiments with EAS are analyzed to estimate the proton and helium (p+He) fractions in the primary cosmic radiation at E0 = 1–100 PeV. It is shown that at energies E0 ∼ 1–100 PeV the fraction of p+He remains significant, namely, the fraction of p+He is near 40% at E0 = 10 PeV

Observation Of Very High Energy Cosmic-ray Families In Emulsion Chambers At High Mountain Altitudes (i)

Characteristics of cosmic-ray hadronic interactions in the 1015 - 1017 eV range are studied by observing a total of 429 cosmic-ray families of visible energy greater than 100 TeV found in emulsion chamber experiments at high mountain altitudes, Chacaltaya (5200 m above sea level) and the Pamirs (4300 m above sea level). Extensive comparisons were made with simulated families based on models so far proposed, concentrating on the relation between the observed family flux and the behaviour of high-energy showers in the families, hadronic and electromagnetic components. It is concluded that there must be global change in characteristics of hadronic interactions at around 1016 eV deviating from thise known in the accelerator energy range, specially in the forwardmost angular region of the collision. A detailed study of a new shower phenomenon of small-pT particle emissions, pT being of the order of 10 MeV/c, is carried out and its relation to the origin of huge "halo" phenomena associated with extremely high energy families is discussed as one of the possibilities. General characteristics of such super-families are surveyed. © 1992.3702365431Borisov, (1981) Nucl. Phys., 191 BBaybrina, (1984) Trudy FIAN 154, p. 1. , [in Russian], Nauka, MoscowLattes, Hadronic interactions of high energy cosmic-ray observed by emulsion chambers (1980) Physics Reports, 65, p. 151Hasegawa, ICR-Report-151-87-5 (1987) presented at FNAL CDF Seminar, , Inst. for Cosmic Ray Research, Univ. of TokyoCHACALTAYA Emulsion Chamber Experiment (1971) Progress of Theoretical Physics Supplement, 47, p. 1Yamashita, Ohsawa, Chinellato, (1984) Proc. 3rd Int. Symp. on Cosmic Rays and Particle Physics, p. 30. , Tokyo, 1984, Inst. for Cosmic Ray Research, Univ. of Tokyo(1984) Proc. 3rd Int. Symp. on Cosmic Rays and Particle Physics, p. 1. , Tokyo, 1984Baradzei, (1984) Proc. 3rd Int. Symp. on Cosmic Rays and Particle Physics, p. 136. , Tokyo, 1984Yamashita, (1985) J. Phys. Soc. Jpn., 54, p. 529Bolisov, (1984) Proc. 3rd Int. Symp. on Cosmic rays and Particle Physics, p. 248. , Tokyo, 1984, Inst. for Cosmic Ray Research, Univ. of TokyoTamada, Tomaszewski, (1988) Proc. 5th Int. Symp. on Very High Energy Cosmic-Ray Interactions, p. 324. , Lodz, 1988, Inst. for Cosmic Ray Research, Univ. of Tokyo, PolandHasegawa, (1989) ICR-Report-197-89-14, , Inst. for Cosmic Ray Research, Univ. of TokyoCHACALTAYA Emulsion Chamber Experiment (1971) Progress of Theoretical Physics Supplement, 47, p. 1Okamoto, Shibata, (1987) Nucl. Instrum. Methods, 257 A, p. 155Zhdanov, (1980) FIAN preprint no. 45, , Lebedev Physical Institute, MoscowSemba, Gross Features of Nuclear Interactions around 1015eV through Observation of Gamma Ray Families (1983) Progress of Theoretical Physics Supplement, 76, p. 111Nikolsky, (1975) Izv. Akad. Nauk. USSR Ser. Fis., 39, p. 1160Burner, Energy spectra of cosmic rays above 1 TeV per nucleon (1990) The Astrophysical Journal, 349, p. 25Takahashi, (1990) 6th Int. Symp. on Very High Energy Cosmic-ray Interactions, , Tarbes, FranceRen, (1988) Phys. Rev., 38 D, p. 1404Alner, The UA5 high energy simulation program (1987) Nuclear Physics B, 291 B, p. 445Bozzo, Measurement of the proton-antiproton total and elastic cross sections at the CERN SPS collider (1984) Physics Letters B, 147 B, p. 392Wrotniak, (1985) Proc. 19th Cosmic-Ray Conf. La Jolla, 1985, 6, p. 56. , NASA Conference Publication, Washington, D.CWrotniak, (1985) Proc. 19th Cosmic-Ray Conf. La Jolla, 1985, 6, p. 328. , NASA Conference Publication, Washington, D.CMukhamedshin, (1984) Trudy FIAN, 154, p. 142. , Nauka, Moscow, [in Russian]Dunaevsky, Pluta, Slavatinsky, (1988) Proc. 5th Int. Symp. on Very High Energy Cosmic-Ray Interactions, p. 143. , Lodz, 1988, Inst. of Physics, Univ. of Lodz, PolandKaidalov, Ter-Martirosyan, (1987) Proc. 20th Int. Cosmic-Ray Conf., Moscow, 1987, 5, p. 141. , Nauka, MoscowShabelsky, (1985) preprints LNPI-1113Shabelsky, (1986) preprints LNPI-1224, , Leningrad [in Russian]Hillas, (1979) Proc. 16th Int. Cosmic-Ray Conf., Kyoto, 6, p. 13. , Inst. for Cosmic Ray Research, Univ. of TokyoBorisov, (1987) Phys. Lett., 190 B, p. 226Hasegawa, Tamada, (1990) 6th Int. Symp. on Very High Energy Cosmic-Ray Interactions, , Tarbes, FranceSemba, Gross Features of Nuclear Interactions around 1015eV through Observation of Gamma Ray Families (1983) Progress of Theoretical Physics Supplement, p. 111Ren, (1988) Phys. Rev., 38 D, p. 1404Dynaevsky, Zimin, (1988) Proc. 5th Int. Symp. on Very High Energy Cosmic-Ray Interaction, p. 93. , Lodz, 1988, Inst. of Physics, Univ. of Lodz, PolandDynaevsky, (1990) Proc. 6th Int. Symp. on Very High Energy Cosmic-Ray Interactions, , Tarbes, France(1989) FIAN preprint no. 208, , Lebedev Physical Institute, Moscow(1990) Proc. 21st Int. Cosmic-Ray Conf., Adelaide, 8, p. 259. , Dept. Physics and Mathematical Physics, Univ. of Adelaide, AustraliaHasegawa, (1990) ICR-Report-216-90-9, , Inst. for Cosmic-Ray Research, Univ. of TokyoTamada, (1990) Proc. 21st Int. Cosmic-Ray Conf., Adelaide, 1990, 8. , Dept. Physics and Mathematical Physics, Univ. of Adelaide, AustraliaTamada, (1990) ICR-Report-216-90-9(1981) Proc. 17th Int. Cosmic-Ray Conf., Paris, 5, p. 291(1990) Proc. Int. Cosmic-Ray Conf., Adelaide, 1990, 8, p. 267. , Dept. Physics and Mathematical Physics, Univ. of Adelaide, Australia(1989) Inst. Nucl. Phys. 89-67/144, , preprint, Inst. Nucl. 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Cosmic-Ray Conf., Moscow, 1987, 5, p. 326. , Nauka, Mosco

Biochemical properties of fodder additives based on fermented poultry wastes and their effects on broiler productivity

The wastes of broiler slaughter and carcass processing – poultry by-products (feathers, blood, bones, meat trimmings, etc.) – are the substantial part of the initial live bodyweight of slaughtered broilers (up to 30%); these by-products, with hydrolysates being especially promising, can serve as a source of animal protein in diets for poultry. In this study, we determined the biochemical properties of the fermented protein additives produced by short-term thermal treatment and subsequent enzymatic hydrolysis of collagen- and keratin-containing poultry wastes. The dry protein additive based on the keratin-containing wastes featured average moisture content 4.57%, crude protein content 86.52%, crude fat content 2.25%, ash content 2.04%; the respective parameters in the dry additive based on the collagen-containing wastes after high-temperature treatment and enzymatic hydrolysis were 2.57, 45.4, 23.29, and 24.04%. The digestibility of the dry keratin- and collagen-based additives after the two-stage productive cycle was 92.0 and 85.0%, respectively. Certain biochemical parameters of these two additives were determined (antioxidative capacity, molecular weight distribution of peptides, profile of volatiles). The analysis of volatiles profile in the keratin-based additive showed that it contained 37 main ingredients, including aliphatic acids and their amides, indole and its derivatives, alcohols, amides of aromatic acids and their derivatives, sulphur-containing substances. The latter are probably responsible for the characteristic odor of the keratin-based product. It was found that the fermented keratin- and collagen-based additives contain primarily peptides with low (< 5 KDa) and medium (10–25 KDa) molecular weights. The antioxidative capacity of the additives in relation to peroxide radical varied in the range of 250–300 μmoles of trolox equivalent per 1 g; over 99.9% of this capacity was presented by hydrophilic antioxidants. Trials on broilers with the substitution of the fermented additives for fish meal in the diets proved that the additives do not compromise the growth efficiency and productive performance