The braking indices in pulsar emission models Export

@article{citeulike:2709733, abstract = {Using the method proposed in a previous paper, we calculate pulsar braking indices in the models with torque contributions from both inner and outer accelerating regions, assuming that the interaction between them is negligible. We suggest that it is likely that the inverse Compton scattering induced polar vacuum gap and the outer gap coexist in the pulsar magnetosphere. We include the new near threshold vacuum gap models with curvature-radiation and inverse Compton scattering induced cascades, respectively; and find that these models can well reproduce the measured values of the braking indices.}, archivePrefix = {arXiv}, author = {Wu, F. and Xu, R. X. and Gil, J.}, citeulike-article-id = {2709733}, citeulike-linkout-0 = {http://arxiv.org/abs/astro-ph/0307359}, citeulike-linkout-1 = {http://arxiv.org/pdf/astro-ph/0307359}, citeulike-linkout-2 = {http://dx.doi.org/10.1051/0004-6361:20031188}, citeulike-linkout-3 = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003A&A...409..641W}, doi = {10.1051/0004-6361:20031188}, eprint = {astro-ph/0307359}, journal = {Astron. Astrophys.}, keywords = {brakingindex, emissionmechanism, pulsar, theory}, month = {October}, pages = {641--645}, posted-at = {2008-04-23 19:34:12}, priority = {2}, title = {The braking indices in pulsar emission models}, url = {http://dx.doi.org/10.1051/0004-6361:20031188}, volume = {409}, year = {2003} }

TY - JOUR ID - citeulike:2709733 L3 - citeulike-article-id:2709733 N2 - Using the method proposed in a previous paper, we calculate pulsar braking indices in the models with torque contributions from both inner and outer accelerating regions, assuming that the interaction between them is negligible. We suggest that it is likely that the inverse Compton scattering induced polar vacuum gap and the outer gap coexist in the pulsar magnetosphere. We include the new near threshold vacuum gap models with curvature-radiation and inverse Compton scattering induced cascades, respectively; and find that these models can well reproduce the measured values of the braking indices. JF - Astron. Astrophys. EP - 645 TI - The braking indices in pulsar emission models VL - 409 SP - 641 KW - brakingindex KW - emissionmechanism KW - pulsar KW - theory AU - Wu, F AU - Xu, RX AU - Gil, J PY - 2003/October// UR - http://dx.doi.org/10.1051/0004-6361:20031188 ER -