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Ultra high energy electrons powered by pulsar rotation.
Sci Rep. 2013;3:1262. doi: 10.1038/srep01262. Epub 2013 Feb 12.
Sci Rep. 2013.
PMID: 23405276
Free PMC article.
Millisecond newly born pulsars as efficient accelerators of electrons.
Osmanov Z, Mahajan S, Machabeli G, Chkheidze N.
Osmanov Z, et al. Among authors: machabeli g.
Sci Rep. 2015 Sep 25;5:14443. doi: 10.1038/srep14443.
Sci Rep. 2015.
PMID: 26403155
Free PMC article.
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Excitation and conversion of electromagnetic waves in pulsar magnetospheres.
Gogoberidze G, Machabeli GZ, Usov VV.
Gogoberidze G, et al. Among authors: machabeli gz.
Phys Rev E Stat Nonlin Soft Matter Phys. 2008 Mar;77(3 Pt 2):037402. doi: 10.1103/PhysRevE.77.037402. Epub 2008 Mar 11.
Phys Rev E Stat Nonlin Soft Matter Phys. 2008.
PMID: 18517567
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Quasilinear theory of Cherenkov-drift instability.
Shapakidze D, Machabeli G, Melikidze G, Khechinashvili D.
Shapakidze D, et al. Among authors: machabeli g.
Phys Rev E Stat Nonlin Soft Matter Phys. 2003 Feb;67(2 Pt 2):026407. doi: 10.1103/PhysRevE.67.026407. Epub 2003 Feb 7.
Phys Rev E Stat Nonlin Soft Matter Phys. 2003.
PMID: 12636822
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Quasilinear diffusion as a result of modulational instability in the pulsar plasma.
Machabeli GZ, Luo Q, Vladimirov SV, Melrose DB.
Machabeli GZ, et al.
Phys Rev E Stat Nonlin Soft Matter Phys. 2002 Mar;65(3 Pt 2B):036408. doi: 10.1103/PhysRevE.65.036408. Epub 2002 Feb 21.
Phys Rev E Stat Nonlin Soft Matter Phys. 2002.
PMID: 11909263
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Centrifugal force: A gedanken experiment.
Machabeli GZ, Rogava AD.
Machabeli GZ, et al.
Phys Rev A. 1994 Jul;50(1):98-103. doi: 10.1103/physreva.50.98.
Phys Rev A. 1994.
PMID: 9910872
No abstract available.
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