Ultrarelativistic plasma shell collisions in γ-ray burst sources: Dimensional effects on the final steady state magnetic field
Astrophysical Journal, ISSN: 1538-4357, Vol: 618, Issue: 2 I, Page: 822-831
2005
- 61Citations
- 40Usage
- 17Captures
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Metrics Details
- Citations61
- Citation Indexes61
- CrossRef61
- 60
- Usage40
- Downloads38
- Abstract Views2
- Captures17
- Readers17
- 17
Article Description
Ultrarelativistic electron-positron plasma shell collisions as an integral part of generic γ-ray burst (GRB) fireball models are studied in the framework of self-consistent three-dimensional particle-in-cell simulations. We compare scenarios at moderately relativistic (γ ≃10) and ultrarelativistic (γ ≃ 100) energies that directly correspond to the regimes of internal and external shell collisions, respectively, in GRB synchrotron emission models. Simulated systems comprise 5 × 10 particles, applying a relativistic, fully electromagnetic, massively parallelized code. It is found that Weibel-generated, steady state magnetic equipartition ratios in external collisions reach up to ε ∼12%, exceeding the respective internal ratios by nearly a power of 10. Enhanced ε yields can be explained theoretically by the effective reduction of dimensionality in the ultrarelativistic limit, i.e., the energy-dependent confinement of the three-dimensional Weibel instability within quasi-two-dimensional plasma shell slices.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=14544278757&origin=inward; http://dx.doi.org/10.1086/426066; https://iopscience.iop.org/article/10.1086/426066; http://stacks.iop.org/0004-637X/618/i=2/a=822/pdf; https://digitalcommons.dartmouth.edu/facoa/1812; https://digitalcommons.dartmouth.edu/cgi/viewcontent.cgi?article=2815&context=facoa; https://digitalcommons.dartmouth.edu/facoa/1802; https://digitalcommons.dartmouth.edu/cgi/viewcontent.cgi?article=2805&context=facoa; https://dx.doi.org/10.1086/426066; https://validate.perfdrive.com/9730847aceed30627ebd520e46ee70b2/?ssa=2b379ef5-f420-452a-a103-7ff34ca2e890&ssb=25928269120&ssc=https%3A%2F%2Fiopscience.iop.org%2Farticle%2F10.1086%2F426066&ssi=fd28c61d-cnvj-42ed-a021-5e7db5239eab&ssk=botmanager_support@radware.com&ssm=744444320124743116152656223868891425&ssn=5b139034747f21e9a6428449db9f66298c260900c3c4-8990-4f21-acbc1e&sso=84590f8c-bc564dd29dea8eeecf23a04d43128a40e26e2a7b60dc91f4&ssp=64397133171726589791172681346886793&ssq=47621597772597662536029239421328495972627&ssr=NTIuMy4yMTcuMjU0&sst=com.plumanalytics&ssu=&ssv=&ssw=&ssx=eyJfX3V6bWYiOiI3ZjYwMDBkNzYzNGE3Ni05ZTRkLTRjMmMtYjJhMC1mYzAzNGMyZjE1MjkxNzI2NTI5MjM5NDUzMzQ4NDg2MzY1LWU2MmU1MmQzZDc1YTAwZWI2MTUxMjEiLCJ1em14IjoiN2Y5MDAwMGMxZDc2YmItMzk2MS00N2VjLTlkZGItNjdmYTVhZTY2ODdlNi0xNzI2NTI5MjM5NDUzMzQ4NDg2MzY1LTRjNjUyN2NiMDRhYzI5MDY2MTUwNTgiLCJyZCI6ImlvcC5vcmcifQ==
American Astronomical Society
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