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The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
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James Clerk Maxwell (1831–1879) was one of the significant contributors to physics in the nineteenth century. He is probably best known for having combined existing knowledge of the laws of electricity and the laws of magnetism with his insights to form a complete overarching electromagnetic theory, represented by Maxwell's equations. The four basic laws of electricity and magnetism were discovered experimentally through the work of physicists such as Oersted, Coulomb, Gauss, and...
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A neutral atom consists of a positively charged nucleus surrounded by a negatively charged electron cloud. When placed in an external electric field, the external electric force pulls the electrons and nucleus apart, opposite to the intrinsic attraction between the nucleus and the electrons. The opposing forces balance each other with a slight shift between the center of masses of the nucleus and the electron cloud, resulting in a polarized atom. On the other hand, a few molecules, like water,...
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Updated: Sep 25, 2025

Picoinjection of Microfluidic Drops Without Metal Electrodes
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Nonideal fields are crucial for injecting particles into high-energy acceleration during magnetic reconnection in relativistic plasmas. Without this initial step in nonideal regions, particles achieve only low energies, impacting astrophysical flare models.

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Area of Science:

  • Plasma physics
  • Astrophysics
  • High-energy particle acceleration

Background:

  • Relativistic plasma phenomena, such as astrophysical flares, are driven by magnetic reconnection.
  • Magnetic reconnection is known to accelerate particles efficiently.
  • The role of nonideal field effects in particle acceleration remains an active area of research.

Purpose of the Study:

  • To investigate the role of nonideal fields in the initial stages of particle acceleration during magnetic reconnection in relativistic plasmas.
  • To determine the necessity of nonideal field regions for achieving high-energy particle acceleration.

Main Methods:

  • Utilizing particle-in-cell (PIC) simulations to model magnetic reconnection in relativistic plasmas.
  • Analyzing particle trajectories and energy gains within both ideal and nonideal magnetic field regions.

Main Results:

  • Demonstrated that nonideal fields are essential for the injection and subsequent acceleration of particles to high energies.
  • Showed that particles accelerated to high energies (near or above mean magnetic energy) must traverse nonideal regions (where E>B or E∥≠0).
  • Observed that particles not experiencing nonideal fields reach only Lorentz factors of order unity.

Conclusions:

  • Injection into particle acceleration by nonideal fields is a necessary prerequisite for achieving high energies in relativistic plasmas.
  • These findings have significant implications for understanding the origin of nonthermal particles in energetic astrophysical sources.
  • The study highlights the limitations of ideal magnetohydrodynamics in describing particle acceleration processes.