Jove
Visualize
Contact Us

Related Concept Videos

Electromagnetic Waves in Matter01:30

Electromagnetic Waves in Matter

3.5K
Electromagnetic waves can travel in the vacuum as well as in matter. For example light, which is an electromagnetic wave, can travel through air, water, or glass.
Consider the electromagnetic wave passing through a dielectric medium. In such a case, Maxwell's equations get modified. In Ampere's law, ε0 , the dielectric permittivity of free space is replaced with ε, the permittivity of dielectric. Also, the vacuum permeability μ0 is replaced by the permeability of the...
3.5K
Electromagnetic Waves01:30

Electromagnetic Waves

9.9K
James Clerk Maxwell formulated a single theory combining all the electric and magnetic effects scientists knew during that time, calling the phenomena his theory predicted “Electromagnetic waves”. He brought together all the work that had been done by brilliant physicists such as Oersted, Coulomb, Gauss, and Faraday and added his own insights to develop the overarching theory of electromagnetism. Maxwell’s equations, combined with the Lorentz force law, encompass all the laws...
9.9K
Dual Nature of Electromagnetic (EM) Radiation01:10

Dual Nature of Electromagnetic (EM) Radiation

2.8K
Electromagnetic (EM) radiation consists of electric and magnetic field components oscillating in planes perpendicular to each other and mutually perpendicular to radiation propagation through space. EM radiation can be classified as a wave, characterized by the properties of waves such as wavelength (denoted as λ) and frequency (represented by ν).
Wavelength is the distance between two consecutive peaks (the highest point) or troughs (the lowest point) in the wave. Frequency is the...
2.8K
Generating Electromagnetic Radiations01:10

Generating Electromagnetic Radiations

5.0K
The German physicist Heinrich Hertz (1857–1894) was the first to generate and detect certain types of electromagnetic waves in the laboratory. Starting in 1887, he performed a series of experiments that confirmed the existence of electromagnetic waves and verified that they travel at the speed of light. Hertz used an alternating-current RLC (resistor-inductor-capacitor) circuit that resonated at a known frequency and connected it to a loop of wire. High voltages induced across the gap in...
5.0K
Potential Due to a Magnetized Object01:24

Potential Due to a Magnetized Object

411
Magnetic dipoles in magnetic materials are aligned when placed under an external magnetic field. For paramagnets and ferromagnets, dipole alignment occurs in the direction of the magnetic field. However, the dipoles align opposite to the field in the case of diamagnets. This state of magnetic polarization due to the external field is called magnetization. Magnetization is defined as the dipole moment per unit volume. It plays a similar role to polarization in electrostatics.
The vector...
411
Energy Carried By Electromagnetic Waves01:22

Energy Carried By Electromagnetic Waves

3.3K
Anyone who has used a microwave oven knows there is energy in electromagnetic waves. Sometimes, this energy is obvious, such as in the summer sun's warmth. At other times, it is subtle, such as the unfelt energy of gamma rays, which can destroy living cells. Electromagnetic waves bring energy into a system through their electric and magnetic fields. These fields can exert forces and move charges in the system and, thus, do work on them. However, there is energy in an electromagnetic wave,...
3.3K

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Radiative plasma simulations of black hole accretion flow coronae in the hard and soft states.

Nature communications·2024
Same author

Radiative Particle-in-Cell Simulations of Turbulent Comptonization in Magnetized Black-Hole Coronae.

Physical review letters·2024
Same author

Repeated Cyclogenesis on Hot-Exoplanet Atmospheres with Deep Heating.

Physical review letters·2023
Same author

Strongly interacting matter exhibits deconfined behavior in massive neutron stars.

Nature communications·2023
Same author

Generation of Near-Equipartition Magnetic Fields in Turbulent Collisionless Plasmas.

Physical review letters·2023
Same author

Scattering of Ultrastrong Electromagnetic Waves by Magnetized Particles.

Physical review letters·2022
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Experiment Video

Updated: Oct 26, 2025

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

15.2K

Coherent Electromagnetic Emission from Relativistic Magnetized Shocks.

Lorenzo Sironi1, Illya Plotnikov2, Joonas Nättilä3

  • 1Department of Astronomy and Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027, USA.

Physical Review Letters
|July 30, 2021
PubMed
Summary

Relativistic magnetized shocks can explain fast radio bursts (FRBs) through coherent emission. Simulations reveal emission efficiency scales with magnetization and detail the spectrum and polarization of X and O modes.

More Related Videos

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
11:47

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

9.3K
How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters
08:42

How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters

Published on: April 16, 2015

20.0K

Related Experiment Videos

Last Updated: Oct 26, 2025

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

15.2K
A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
11:47

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

9.3K
How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters
08:42

How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters

Published on: April 16, 2015

20.0K

Area of Science:

  • Plasma physics
  • Astrophysics
  • Computational physics

Background:

  • Relativistic magnetized shocks are theorized to produce coherent emission.
  • This emission is a potential mechanism for Fast Radio Bursts (FRBs).
  • Understanding shock properties is crucial for FRB models.

Purpose of the Study:

  • To investigate the emission efficiency, spectrum, and polarization from relativistic magnetized shocks.
  • To provide essential data for shock-based FRB models.
  • To elucidate the emission mechanisms of X and O modes.

Main Methods:

  • First-principles 3D particle-in-cell simulations.
  • Simulations of shocks propagating in electron-positron (e^{±}) plasma.
  • Analysis of plasma magnetization (σ>1) effects on emission.

Main Results:

  • Emission efficiency is approximately 10^{-3}σ^{-1} of shock energy.
  • Energy-carrying wave number of the spectrum is around 4ω_{c}/c.
  • O-mode to X-mode energy flux ratio is approximately 0.4σ^{-1}, with X-mode dominance at high σ.

Conclusions:

  • Relativistic magnetized shocks are a viable source for FRB emission.
  • Simulation results quantify key emission properties.
  • The dominance of X-mode emission at high magnetization is a significant finding for FRB models.