Promising lines of investigations in the realms of laboratory astrophysics with the aid of powerful lasers

被引:8
|
作者
Belyaev, V. S. [1 ]
Batishchev, P. A. [1 ]
Bolshakov, V. V. [1 ]
Elkin, K. S. [1 ]
Karabadzhak, G. F. [1 ]
Kovkov, D. V. [1 ]
Matafonov, A. P. [1 ]
Raykunov, G. G. [1 ]
Yakhin, R. A. [1 ]
Pikuz, S. A. [2 ]
Skobelev, I. Yu [2 ]
Faenov, A. Ya [2 ]
Fortov, V. E. [2 ]
Krainov, V. P. [3 ]
Rozanov, V. B. [4 ]
机构
[1] Russian Space Agcy, Cent Res Inst Machine Bldg TsNIIMash, Korolev 141070, Moscow Oblast, Russia
[2] Russian Acad Sci IVTAN, Joint Inst High Temp, Moscow 125412, Russia
[3] Moscow Inst Phys & Technol, Dolgoprudnyi 141700, Moscow Oblast, Russia
[4] Russian Acad Sci, Lebedev Inst Phys, Moscow 119991, Russia
基金
俄罗斯基础研究基金会;
关键词
GAMMA-RAY BURSTS; CORE COLLAPSE SUPERNOVAE; LOW-MASS STARS; NEUTRON-STARS; MAGNETIC-FIELDS; NUCLEAR-REACTIONS; OPTICAL PULSES; EXTREME STATES; BROWN DWARFS; ZN IONS;
D O I
10.1134/S1063778813030046
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The results of work on choosing and substantiating promising lines of research in the realms of laboratory astrophysics with the aid of powerful lasers are presented. These lines of research are determined by the possibility of simulating, under laboratory conditions, problematic processes of presentday astrophysics, such as (i) the generation and evolution of electromagnetic fields in cosmic space and the role of magnetic fields there at various spatial scales; (ii) the mechanisms of formation and evolution of cosmic gamma-ray bursts and relativistic jets; (iii) plasma instabilities in cosmic space and astrophysical objects, plasma jets, and shock waves; (iv) supernova explosions and mechanisms of the explosion of supernovae featuring a collapsing core; (v) nuclear processes in astrophysical objects; (vi) cosmic rays and mechanisms of their production and acceleration to high energies; and (vii) astrophysical sources of x-ray radiation. It is shown that the use of existing powerful lasers characterized by an intensity in the range of 10(18)-10(22) W/cm(2) and a pulse duration of 0.1 to 1 ps and high-energy lasers characterized by an energy in excess of 1 kJ and a pulse duration of 1 to 10 ns makes it possible to perform investigations in laboratory astrophysics along all of the chosen promising lines. The results obtained by experimentally investigating laser plasma with the aid of the laser facility created at Central Research Institute of Machine Building (TsNIIMash) and characterized by a power level of 10 TW demonstrate the potential of such facilities for performing a number of experiments in the realms of laboratory astrophysics. DOI: 10.1134/S1063778813030046
引用
收藏
页码:404 / 422
页数:19
相关论文
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    P. A. Batishchev
    V. V. Bolshakov
    K. S. Elkin
    G. F. Karabadzhak
    D. V. Kovkov
    A. P. Matafonov
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    I. Yu. Skobelev
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    V. P. Krainov
    V. B. Rozanov
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