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- Blakiston’s Fish Owl (1)
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It is proposed to install an experimental setup in the fixed-target hall of the Nuclotron with the final goal to perform a research program focused on the production of strange matter in heavyion collisions at beam energies between 2 and 6 A GeV. The basic setup will comprise a large acceptance dipole magnet with inner tracking detector modules based on double-sided Silicon micro-strip sensors and GEMs. The outer tracking will be based on the drift chambers and straw tube detector. Particle identification will be based on the time-of-flight measurements. This setup will be sufficient perform a comprehensive study of strangeness production in heavy-ion collisions, including multi-strange hyperons, multi-strange hypernuclei, and exotic multi-strange heavy objects. These pioneering measurements would provide the first data on the production of these particles in heavy-ion collisions at Nuclotron beam energies, and would open an avenue to explore the third (strangeness) axis of the nuclear chart. The extension of the experimental program is related with the study of in-medium effects for vector mesons decaying in hadronic modes. The studies of the NN and NA reactions for the reference is assumed.
The nucleosynthesis of elements beyond iron is dominated by neutron captures in the s and r processes. However, 32 stable, proton-rich isotopes cannot be formed during those processes, because they are shielded from the s-process flow and r-process β-decay chains. These nuclei are attributed to the p and rp process.
For all those processes, current research in nuclear astrophysics addresses the need for more precise reaction data involving radioactive isotopes. Depending on the particular reaction, direct or inverse kinematics, forward or time-reversed direction are investigated to determine or at least to constrain the desired reaction cross sections.
The Facility for Antiproton and Ion Research (FAIR) will offer unique, unprecedented opportunities to investigate many of the important reactions. The high yield of radioactive isotopes, even far away from the valley of stability, allows the investigation of isotopes involved in processes as exotic as the r or rp processes.
New data on the distribution were the reported: Buksendya river (153º15’E, 59º12’N), Yama valley (152º59’E, 60º00’N) and Nayakhan river (158º15’E, 62º33’N), mostly single birds in late summer, autumn or early winter. Resident breeding pairs regularly occur only in the Chelomdzha and further to the west – in Inya and Ulbeya valleys, and upper heads of the Kava valley (Fig. 1). New observations in the Inya valley (July-August 1999) and in the Chelomdzha valley (July 2003) have proved that the Blakiston’s Fish Owl dwells in lush flood-plain woods along the middle and lower streams of both of these valleys. Currently, the Blakiston’s Fish Owl steadily occurs within the limits of Kava-Chelomdza forestry of the Magadansky State Reserve (Tarkhov & Potapov 1986), and, most likely, the Chelomdzha valley forms currently the north-eastern limit of the species range. In the Chelomdzha valley the regular duet singing of the Blakiston’s Fish Owl begins from early February. Usually the birds display in the evenings, 20-40 min after sunset. The longevity of evening vocalizations increases from 3-5 min in first week of February to 30-50 min in mid-March. The intervals between strophes vary from 14-55 s, 27 s on average (n = 48). The chicks hatched between 2nd and 5th of May. Daytime hours the parents spend nearby the nest in the crowns of larches. During intense chick’s growth the parents visit the nest 4-5 times in a night. Search for food and hunting takes from 40-60 min. According to photo documents, the parents feed the chicks with sculpins and graylings (18–30 cm in length). The parents spend midnight hours nearby the nest. Becoming 50 days old the chicks leave the nest and roams around supervised by the parents.
Ultra-intense MeV photon and neutron beams are indispensable tools in many research fields such as nuclear, atomic and material science as well as in medical and biophysical applications. For applications in laboratory nuclear astrophysics, neutron fluxes in excess of 1021 n/(cm2 s) are required. Such ultra-high fluxes are unattainable with existing conventional reactor- and accelerator-based facilities. Currently discussed concepts for generating high-flux neutron beams are based on ultra-high power multi-petawatt lasers operating around 1023 W/cm2 intensities. Here, we present an efficient concept for generating γ and neutron beams based on enhanced production of direct laser-accelerated electrons in relativistic laser interactions with a long-scale near critical density plasma at 1019 W/cm2 intensity. Experimental insights in the laser-driven generation of ultra-intense, well-directed multi-MeV beams of photons more than 1012 ph/sr and an ultra-high intense neutron source with greater than 6 × 1010 neutrons per shot are presented. More than 1.4% laser-to-gamma conversion efficiency above 10 MeV and 0.05% laser-to-neutron conversion efficiency were recorded, already at moderate relativistic laser intensities and ps pulse duration. This approach promises a strong boost of the diagnostic potential of existing kJ PW laser systems used for Inertial Confinement Fusion (ICF) research.
Ultra-intense MeV photon and neutron beams are indispensable tools in many research fields such as nuclear, atomic and material science as well as in medical and biophysical applications. For astrophysical applications aimed on laboratory investigations of the r-processes responsible for the production of heavy elements in explosive supernova scenarios, neutron fluxes in excess of 1021 n/(cm2 s) are required. These ultra-high fluxes are unattainable with existing conventional reactor- and accelerator-based facilities. Currently discussed concepts for the generation of high-flux neutron beams are based on ultra-high-power multi-petawatt lasers operating at >1023 W/cm2 intensities. Here, we present a novel concept for the efficient generation of γ and neutron beams based on relativistic laser interactions with a long-scale near critical density plasma at 1019 W/cm2 intensity. New experimental insights in the laser-driven generation of ultra-intense well-directed multi-MeV beams of photons with fluences of >1012 ph/sr and a ultra-high intense neutron source with >1010 neutrons per shot are presented. Optimization of the target-set based on the gamma-driven nuclear reactions promises an ultra-high neutron fluence of >1011 n/cm2 and corresponding neutron peak-fluxes of ∼1022 n/(cm2 s) already at moderate relativistic laser intensities.