Inverse Compton scattering: Gap parameters, energy loss of the particles, and possible implications for pulsar radio emission
文献类型：期刊论文
| 作者 | Zhang, B ; Qiao, GJ; Han, JL
|
| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 1997-12-20 |
| 卷号 | 491期号:2页码:891-902 |
| 关键词 | acceleration of particles pulsars, general pulsars, individual (Geminga) radiation mechanisms, nonthermal |
| 英文摘要 | The process of inverse Compton scattering (ICS) of high-energy particles off the thermal photons above the pulsar polar cap is the dominant mechanism causing polar gap breakdown. In this paper, an approximate analytic description of the parameters of the two modes of the ICS gap, namely, the "resonant ICS gap" and the "thermal ICS gap," are derived under the assumption of a multipolar magnetic field configuration in the neutron star's vicinity. For typical values of P, B, and T, the thermal ICS gap usually has a lower height and smaller potential drop but results in larger Lorentz factors for the secondary particles ejected from the gap. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000071152600038 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/8322]  |
| 专题 | 国家天文台_光学天文研究部 |
| 作者单位 | 1.Peking Univ, Dept Geophys, Beijing 100871, Peoples R China 2.Chinese Ctr Adv Sci & Technol, World Lab, Beijing 100080, Peoples R China 3.Chinese Acad Sci, Beijing Astron Observ, Beijing 100080, Peoples R China |
| 推荐引用方式 GB/T 7714 | Zhang, B,Qiao, GJ,Han, JL. Inverse Compton scattering: Gap parameters, energy loss of the particles, and possible implications for pulsar radio emission[J]. ASTROPHYSICAL JOURNAL,1997,491(2):891-902. |
| APA | Zhang, B,Qiao, GJ,&Han, JL.(1997).Inverse Compton scattering: Gap parameters, energy loss of the particles, and possible implications for pulsar radio emission.ASTROPHYSICAL JOURNAL,491(2),891-902. |
| MLA | Zhang, B,et al."Inverse Compton scattering: Gap parameters, energy loss of the particles, and possible implications for pulsar radio emission".ASTROPHYSICAL JOURNAL 491.2(1997):891-902. |
入库方式： OAI收割
来源：国家天文台
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