Excitation and conversion of electromagnetic waves in pulsar magnetospheres Export

@misc{citeulike:2605148, abstract = {We demonstrate that nonlinear decay of obliquely propagating Langmuir waves into Langmuir and Alfven waves (L --\> L'+A) is possible in a one-dimensional, highly relativistic, streaming, pair plasma. Such a plasma may be in the magnetospheres of pulsars. It is shown that the characteristic frequency of generated Alfven waves is much less than the frequency of Langmuir waves and may be consistent with the observational data on the radio emission of pulsars.}, archivePrefix = {arXiv}, author = {Gogoberidze, G. and Machabeli, G. Z. and Usov, V. V.}, citeulike-article-id = {2605148}, citeulike-linkout-0 = {http://arxiv.org/abs/astro-ph/0702195}, citeulike-linkout-1 = {http://arxiv.org/pdf/astro-ph/0702195}, day = {26}, eprint = {astro-ph/0702195}, keywords = {emissionmechanism, pulsar}, month = {Mar}, posted-at = {2008-03-28 06:41:21}, priority = {2}, title = {Excitation and conversion of electromagnetic waves in pulsar magnetospheres}, url = {http://arxiv.org/abs/astro-ph/0702195}, year = {2008} }

TY - ELEC ID - citeulike:2605148 L3 - citeulike-article-id:2605148 N2 - We demonstrate that nonlinear decay of obliquely propagating Langmuir waves into Langmuir and Alfven waves (L --> L'+A) is possible in a one-dimensional, highly relativistic, streaming, pair plasma. Such a plasma may be in the magnetospheres of pulsars. It is shown that the characteristic frequency of generated Alfven waves is much less than the frequency of Langmuir waves and may be consistent with the observational data on the radio emission of pulsars. TI - Excitation and conversion of electromagnetic waves in pulsar magnetospheres KW - emissionmechanism KW - pulsar AU - Gogoberidze, G AU - Machabeli, GZ AU - Usov, VV PY - 2008/Mar/26/ UR - http://arxiv.org/abs/astro-ph/0702195 ER -