Chin. Phys. Lett.  2006, Vol. 23 Issue (10): 2881-2884    DOI:
Original Articles |
One-Dimensional Electric Field Structure of an Outer Gap Accelerator
CHEN Shi-Bo1;ZHANG Li1,2
1Department of Physics, Yunnan University, Kunming 650031 2National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, Kunming 650011
Cite this article:   
CHEN Shi-Bo, ZHANG Li 2006 Chin. Phys. Lett. 23 2881-2884
Download: PDF(257KB)  
Export: BibTeX | EndNote | Reference Manager | ProCite | RefWorks
Abstract We re-study the one-dimensional electric field structure of an outer gap accelerator by considering the physical limit of trans-field height. Inside the outer gap, the charge depletion creates a large electric
field along the magnetic field lines. Electrons and/or positrons are accelerated to ultra-relativistic energies by this longitudinal electric field, and then radiate γ-ray photons by curvature radiation. The collision of these γ-rays and ambient x-ray photons further produce radiating particles, resulting in a stationary gap. We solve the structure of this longitudinal electric field together with the distributions of electrons and positrons and γ-ray photons for an aligned rotator. Our results indicate that the outer gap can extend to the light cylinder using reasonable parameters.
Keywords: 97.60.Gb      95.30.Gv      95.30.Qd     
Published: 01 October 2006
PACS:  97.60.Gb (Pulsars)  
  95.30.Gv (Radiation mechanisms; polarization)  
  95.30.Qd (Magnetohydrodynamics and plasmas)  
TRENDMD:   
URL:  
https://cpl.iphy.ac.cn/       OR      https://cpl.iphy.ac.cn/Y2006/V23/I10/02881
Service
E-mail this article
E-mail Alert
RSS
Articles by authors
CHEN Shi-Bo
ZHANG Li
Related articles from Frontiers Journals
[1] CAI Yan, A. Taani**, WANG Wei, ZHAO Yong-Heng, ZHANG Cheng-Min . Fermi γ-Ray Pulsars: Spectral and Generation Order Parameters[J]. Chin. Phys. Lett., 2011, 28(8): 2881-2884
[2] LI Ming-Jun**, CHEN Liang . Magnetic Fluid Flows in Porous Media*[J]. Chin. Phys. Lett., 2011, 28(8): 2881-2884
[3] JI Zhen, **, ZHOU Yu-Fen, HOU Tian-Xiang . A Modified Third-Order Semi-Discrete Central-Upwind Scheme for MHD Simulation[J]. Chin. Phys. Lett., 2011, 28(7): 2881-2884
[4] TANG Yun-Yong, FANG Jun, ZHANG Li** . Nonthermal Emission of Tycho's Supernova Remnant[J]. Chin. Phys. Lett., 2011, 28(10): 2881-2884
[5] LIU Xiong-Wei**, NA Xue-Sen, XU Ren-Xin, QIAO Guo-Jun . Particle Emission-Dependent Timing Noise of Pulsars[J]. Chin. Phys. Lett., 2011, 28(1): 2881-2884
[6] JI Zhen, ZHOU Yu-Fen. A Comparison Study of Three CESE Schemes in MHD Simulation[J]. Chin. Phys. Lett., 2010, 27(8): 2881-2884
[7] YU Huan, JIANG Ze-Jun,. Multiband Non-Thermal Radiation from the Crab Nebula and the Pulsar Wind Nebula in MSH 15-52[J]. Chin. Phys. Lett., 2010, 27(8): 2881-2884
[8] Shubhra Tiwari, S. N. A. Jaaffrey, Rizwan S. Khan, Sushil K. Gandhi, Santvana Bapna. Timing and Spectral Studies of Pulsar EXO2030+375[J]. Chin. Phys. Lett., 2010, 27(2): 2881-2884
[9] CHEN Liang, **, BAI Jin-Ming, . Is Low-Frequency-Peaked BL Lac Object OJ 287 a TeV Emitter?[J]. Chin. Phys. Lett., 2010, 27(11): 2881-2884
[10] WEI Ying-Chun, A. Taani**, PAN Yuan-Yue, WANG Jing, CAI Yan, LIU Gao-Chao, LUO A-Li, ZHANG Hong-Bo, ZHAO Yong-Heng . Neutron Star Motion in the Disk Galaxy[J]. Chin. Phys. Lett., 2010, 27(11): 2881-2884
[11] LIN Gui-Fang, ZHANG Li. Vacuum Outer-Gap Structure in Pulsar Outer Magnetospheres[J]. Chin. Phys. Lett., 2009, 26(5): 2881-2884
[12] CHEN Wen-Cong. Evolving into Magnetars from Normal Pulsars with a Low Braking Index[J]. Chin. Phys. Lett., 2009, 26(5): 2881-2884
[13] ZHOU Ai-Zhi, TAN Jin-Yu, Ali Esamdin, WU Xin-Ji. Two-Component Model for the Interstellar Scattering along the Line of Sight to the Pulsar PSR B0136+57[J]. Chin. Phys. Lett., 2009, 26(12): 2881-2884
[14] M. Khayrul Hasan, M. Hossain Ali. Dispersion Relations for Isothermal Plasma around the Horizon of Reissner-Nordström-de Sitter Black Hole[J]. Chin. Phys. Lett., 2009, 26(10): 2881-2884
[15] CAI Zhen-Yi, GU Wei-Min, LU Ju-Fu. Constraints on Slim Accretion Discs[J]. Chin. Phys. Lett., 2008, 25(4): 2881-2884
Viewed
Full text


Abstract