Cross-field mass transport driven by instabilities stabilizes magnetic mountains on neutron stars, preserving a nonzero quadrupole moment as accreted mass grows.
Title resolution pending
6 Pith papers cite this work. Polarity classification is still indexing.
citation-role summary
citation-polarity summary
years
2026 6verdicts
UNVERDICTED 6roles
background 1polarities
background 1representative citing papers
K-essence cosmology induces a redshift-dependent effective mass on gravitational waves, causing phase shifts that link scalar field dynamics to GW observables without changing wave speed or luminosity distance.
IMF inclusion adds a cyclotron frequency term to the TSI dispersion relation, changing growth rate with velocity, density and B; PIC runs show background electrons shielding solar wind electrons in vortices and some lunar electrons aligning with solar wind flow.
Coherent structures that self-consistently emerge in strong MHD turbulence serve as the dominant sites for localized electric-field intensification and repeated particle acceleration across cosmic plasmas.
Historical review framing 18th-century electroculture experiments as a precursor to 21st-century plasma agriculture technologies.
This review summarizes the basic principles of electron transport in inhomogeneous and tangled magnetic fields through gyro-centre trajectories, kinetic instabilities, trapping, and diffusion processes.
citing papers explorer
-
Relaxation of magnetically-confined mountains on accreting neutron stars through cross-field mass transport
Cross-field mass transport driven by instabilities stabilizes magnetic mountains on neutron stars, preserving a nonzero quadrupole moment as accreted mass grows.
-
Gravitational Wave Propagation in K-essence Cosmology: Theory and Observational Constraints
K-essence cosmology induces a redshift-dependent effective mass on gravitational waves, causing phase shifts that link scalar field dynamics to GW observables without changing wave speed or luminosity distance.
-
The two-stream instability generation around Moon: Effect of Interplanetary Magnetic Field during Solar Wind - Lunar Plasma Interaction
IMF inclusion adds a cyclotron frequency term to the TSI dispersion relation, changing growth rate with velocity, density and B; PIC runs show background electrons shielding solar wind electrons in vortices and some lunar electrons aligning with solar wind flow.
-
Strong MHD Turbulence and Coherent Structures as Drivers of Cosmic Particle Acceleration
Coherent structures that self-consistently emerge in strong MHD turbulence serve as the dominant sites for localized electric-field intensification and repeated particle acceleration across cosmic plasmas.
-
From Electroculture to Plasma Agriculture: A Three-Century Arc Bridging Bertholon's Legacy with Contemporary Farming Advances
Historical review framing 18th-century electroculture experiments as a precursor to 21st-century plasma agriculture technologies.
-
Transport of electrons in tangled magnetic fields
This review summarizes the basic principles of electron transport in inhomogeneous and tangled magnetic fields through gyro-centre trajectories, kinetic instabilities, trapping, and diffusion processes.