Relativistic charge solitons created due to nonlinear Landau damping: A candidate for explaining coherent radio emission in pulsars
arXiv:1808.03657 · doi:10.1093/mnras/sty2152
Abstract
A potential resolution for the generation of coherent radio emission in pulsar plasma is the existence of relativistic charge solitons, which are solutions of nonlinear Schrödinger equation (NLSE). In an earlier study, Melikidze et al. (2000) investigated the nature of these charge solitons; however, their analysis ignored the effect of nonlinear Landau damping, which is inherent in the derivation of the NLSE in the pulsar pair plasma. In this paper we include the effect of nonlinear Landau damping and obtain solutions of the NLSE by applying a suitable numerical scheme. We find that for reasonable parameters of the cubic nonlinearity and nonlinear Landau damping, soliton-like intense pulses emerge from an initial disordered state of Langmuir waves and subsequently propagate stably over sufficiently long times, during which they are capable of exciting the coherent curvature radiation in pulsars. We emphasize that this emergence of {\em stable} intense solitons from a disordered state does not occur in a purely cubic NLSE; thus, it is {\em caused} by the nonlinear Landau damping.
41 pages, 7 figures, accepted for publication in MNRAS
References in corpus (14)
- Time-dependent pair cascades in magnetospheres of neutron stars I. Dynamics of the polar cap cascade with no particle supply from the neutron star surface
- Three-dimensional numerical simulations of the pulsar magentoshere: Preliminary results
- Profile and polarization characteristics of energetic pulsars
- Strongly interacting soliton gas and formation of rogue waves
- Theory of pulsar magnetosphere and wind
- Unraveling the nature of coherent pulsar radio emission
- Altitude-dependent polarization in radio pulsars
- The Nature of Coherent Radio Emission from Pulsars
- On the adiabatic walking of plasma waves in a pulsar magnetosphere
- Core and Conal Component Analysis of Pulsar B1933+16 --- Investigation of the Segregated Modes
- Constraining the Vela Pulsar's Radio Emission Region Using Nyquist-Limited Scintillation Statistics
- Magnetothermal Evolution of Neutron Stars with Emphasis to Radio Pulsars
- Effects of Landau damping on ion-acoustic solitary waves in a semiclassical plasma
- Effects of group velocity and multi-plasmon resonances on the modulation of Langmuir waves in a degenerate plasma
Cited by in corpus (19)
- Pulsar radio emission mechanisms: a critique
- A Mechanism of Spark Motion in Inner Acceleration Region to Investigate Subpulse Drifting in Pulsars
- Rapid Modification of Neutron Star Surface Magnetic Field: A proposed mechanism for explaining Radio Emission State Changes in Pulsars
- A Single spark model for PSR J21443933
- Mode changing, subpulse drifting and nulling in four component conal pulsar PSR J2321+6024
- Radio emission features in different modes of PSR J0826+2637 (B0823+26)
- Meterwavelength Single-pulse Polarimetric Emission Survey. V. Flux density, component spectral variation and emission states
- Investigation of the Mode-Switching Phenomenon in Pulsar B0329+54 Through Polarimetric Analysis
- Two Dimensional Configuration and Temporal Evolution of Sparking discharges in Pulsars
- Evidence for Coherent Curvature Radiation in PSR J16450317 with Disordered Distribution of Polarization Position Angle
- Meterwavelength Single-pulse Polarimetric Emission Survey. VI. Towards understanding the Phenomenon of Pulsar Polarization in Partially Screened Vacuum Gap model
- Pulsar radio emission mechanism II. On the origin of relativistic Langmuir solitons in pulsar plasma
- Radio Emission by Soliton Formation in Relativistically Hot Streaming Pulsar Pair Plasmas
- Spectral variation across Pulsar Profile due to Coherent Curvature Radiation
- Coherent Curvature Radiation Spectrum by Dynamically Fluctuating Bunches in Magnetospheres
- Radio Emission of Pulsars. II. Coherence Catalyzed by Cerenkov-Unstable Shear Alfvén Waves
- Streaming instability in neutron star magnetospheres: No indication of soliton-like waves
- Externally-driven plasma models as candidates for pulsar radio emission
- Pulsar radio emission mechanism I : On the amplification of Langmuir waves in the linear regime