共查询到20条相似文献,搜索用时 10 毫秒
1.
采用洛伦兹变换推导出左旋椭圆偏振强激光在磁化等离子体中的非线性色散关系,根据Karpman方法推导出激光场包络的非线性控制方程,分析了在磁化等离子体中左旋椭圆偏振激光的调制不稳定性,得到了调制不稳定的时间增长率。分析结果表明,磁化等离子体中自调制不稳定的极大增长率较非磁化情况明显减小,且在激光等离子体临界面附近处调制不稳定性的时间增长率显著增大。 相似文献
2.
竹锦霞 《原子与分子物理学报》2014,31(6):941-944
利用ECE电子回旋辐射和Ha线辐射等托卡马克物理诊断系统,研究了Slide-away放电过程中提高等离子体密度对非麦克斯维尔分布的逃逸电子所激发的逃逸电子束不稳定性影响作用。实验结果表明:在Slide-away放电模式下,提高等离子体密度能有效抑制逃逸电子束的不稳定性。 相似文献
3.
竹锦霞 《原子与分子物理学报》2015,32(6)
利用ECE电子回旋辐射和Ha线辐射等托卡马克物理诊断系统,研究了Slide-away放电过程中提高等离子体密度对非麦克斯维尔分布的逃逸电子所激发的逃逸电子束不稳定性影响作用.实验结果表明:在Slide-away放电模式下,提高等离子体密度能有效抑制逃逸电子束的不稳定性. 相似文献
4.
采用洛伦兹变换推导出左旋椭圆偏振强激光在磁化等离子体中的非线性色散关系,根据Karpman方法推导出激光场包络的非线性控制方程,分析了在磁化等离子体中左旋椭圆偏振激光的调制不稳定性,得到了调制不稳定的时间增长率。分析结果表明,磁化等离子体中自调制不稳定的极大增长率较非磁化情况明显减小,且在激光等离子体临界面附近处调制不稳定性的时间增长率显著增大。 相似文献
5.
Results for solar neutrino detection from the SuperKamiokande collaboration have been presented recently while those from
the Sudbury Neutrino Observatory are expected in the near future. These experiments are sensitive to the8B neutrinos from the sun, the shape of whose spectrum is well-known but the normalization is less certain. We propose several
variables, insensitive to the absolute flux of the incident beam, which probe the shape of the observed spectrum and can sensitively
signal neutrino oscillations. They provide methods to extract the neutrino mixing angle and mass splitting from the data and
also to distinguish oscillation to sequential neutrinos from those to a sterile neutrino. 相似文献
6.
R. Szafron 《Progress in Particle and Nuclear Physics》2010,64(2):210-212
A short review of the theory of neutrino oscillation for non-standard neutrino interaction (NSI) which may exist at low energy is presented. Depending on the NSI, initial neutrino states can be mixed and final oscillation rates not necessarily factorize. 相似文献
7.
A. Ianni 《Progress in Particle and Nuclear Physics》2011,66(2):405-411
8.
The collisional current-filamentation instability (CFI) is studied for a nonrelativistic electron beam penetrating an infinite uniform plasma. It is analytically shown that the CFI is driven by the drift-anisotropy rather than the classical anisotropy of the beam and the background plasma. Therefore, collisional effects can either attenuate or enhance the CFI depending on the drift-anisotropy of the beam-plasma system. Numerical results are given for some typical parameters, which show that collisional effects cannot stabilize but enhance the CFI in a dense plasma. Thus, the CFI may play a dominant role in the fast electron transport and deposition relevant to the fast ignition scenario (FIS). 相似文献
9.
The collisional current-filamentation instability (CFI) is studied for a nonrelativistic electron beam penetrating an infinite uniform plasma. It is analytically shown that the CFI is driven by the drift-anisotropy rather than the classical anisotropy of the beam and the background plasma. Therefore, collisional effects can either attenuate or enhance the CFI depending on the drift-anisotropy of the beam-plasma system. Numerical results are given for some typical parameters, which show that collisional effects cannot stabilize but enhance the CFI in a dense plasma. Thus, the CFI may play a dominant role in the fast electron transport and deposition relevant to the fast ignition scenario (FIS). 相似文献
10.
Absolute electron beam-plasma instability is suggested as a means of energy compression for pellet and liner inertial confinement
fusion systems. 相似文献
11.
Sandhya Choubey D. Indumathi S. Agarwalla A. Bandyopadhyay G. Bhattacharyya E. J. Chun B. Dasgupta A. Dighe P. Ghoshal A. K. Giri S. Goswami M. Hirsch T. Kajita M. Kaplinghat H. S. Mani R. Mohanta M. V. N. Murthy S. Pakvasa M. K. Parida G. Rajasekaran S. Ray W. Rodejohann P. Roy S. Uma Sankar T. Schwetz N. Sinha 《Pramana》2009,72(1):269-275
This is the report of the neutrino physics working group at WHEPP-X. We summarize the problems selected and discussed at the
workshop and the papers which have resulted subsequently.
相似文献
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13.
R. Mickeviius A. Reklaitis 《International Journal of Infrared and Millimeter Waves》1985,6(3):235-248
The possibility of the excitation of impact-ionized electron-hole plasma oscillatory instability in GaAs with frequency up to 1012 Hz is shown. The linear and nonlinear stages of the instability are investigated. 相似文献
14.
We present a simple but general treatment of neutrino oscillations in the framework of quantum mechanics, using plane waves and intuitive wave packet principles when necessary. We attempt to clarify some confusing statements that have recently appeared in the literature. 相似文献
15.
Srubabati Goswami Raghavan Rangarajan K. Agashe A. Bandyopadhyay K. Bhattacharya B. Brahmachari C. Burgess E. J. Chun D. Choudhury P. K. Das A. Dighe R. Godbole S. Goswami N. Gupta M. Kaplinghat D. Indumathi J. Forshaw Y. Y. Keum B. Layek D. Majumdar N. Mahajan P. Mehta R. N. Mohapatra N. Mondai S. More Y. Nir S. Pakvasa M. K. Parida M. Ravikumar G. Rajasekaran P. Ramadevi R. Rangarajan S. D. Rindani D. P. Roy P. Roy N. Sahu A. Samanta Y. Shadmi A. M. Srivastava S. Uma Sankar R. Vaidya U. Yajnik 《Pramana》2004,63(6):1391-1405
This is the report of neutrino and astroparticle physics working group at WHEPP-8. We present the discussions carried out
during the workshop on selected topics in the above fields and also indicate progress made subsequently. The neutrino physics
subgroup studied the possibilities of constraining neutrino masses, mixing and CPT violation in lepton sector from future
experiments. Neutrino mass models in the context of Abelian horizontal symmetries, warped extra dimensions and in the presence
of triplet Higgs were studied. Effect of threshold corrections on radiative magnification of mixing angles was investigated.
The astroparticle physics subgroup focused on how various particle physics inputs affect the CMBR fluctuation spectrum, and
on brane cosmology. This report also contains an introduction on how to use the publicly available code CMBFAST to calculate
the CMBR fluctuations. 相似文献
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A.L. Hallin 《Progress in Particle and Nuclear Physics》2010,64(2):199-201
20.
Sandip Pakvasa 《Pramana》2000,54(1):65-77
I review explanations for the three neutrino anomalies (solar, atmospheric and LSND) which go beyond the ‘conventional’ neutrino
oscillations induced by mass-mixing. Several of these require non-zero neutrino masses as well. 相似文献