Jove
Visualize
Contact Us

Related Concept Videos

Kinetic Energy for a Rigid Body01:13

Kinetic Energy for a Rigid Body

210
Imagine a solid object involved in a general planar movement, with its center of mass pinpointed at a spot labeled G. The object's kinetic energy relative to an arbitrary point A can be quantified for each of its particles - the ith particle in this case. This measurement is achieved through the employment of the relative velocity definition. The position vector, known as rA, extends from point A to the mass element i.
210
Molecular Kinetic Energy01:21

Molecular Kinetic Energy

5.1K
The word "gas" comes from the Flemish word meaning "chaos," first used to describe vapors by the chemist J. B. van Helmont. Consider a container filled with gas, with a continuous and random motion of molecules. During collisions, the velocity component parallel to the wall is unchanged, and the component perpendicular to the wall reverses direction but does not change in magnitude. If the molecule’s velocity changes in the x-direction, then its momentum is changed.
5.1K
Conservation of Linear Momentum for a System of Particles01:28

Conservation of Linear Momentum for a System of Particles

221
In the dynamic realm of billiards, a fascinating interplay of forces governs the motion of cue balls and stationary balls. When the cue ball collides with a stationary ball, linear momentum is exchanged. The cue ball imparts a fraction of its linear momentum to the stationary ball, causing the cue ball to decelerate while initiating the motion of the stationary ball.
The impulsive force at play during this interaction is of extremely short duration, rendering its impulse negligible. When...
221
Equilibrium Conditions for a Particle01:23

Equilibrium Conditions for a Particle

1.1K
When an object is in equilibrium, it is either at rest or moving with a constant velocity. There are two types of equilibrium: static and dynamic. Static equilibrium occurs when an object is at rest, while dynamic equilibrium occurs when an object is moving with a constant velocity. In both cases, there must be a balance of forces acting on the object.
To understand the concept of equilibrium, let us first consider the forces acting on an object. When different forces act on an object, they can...
1.1K
Atomic Nuclei: Nuclear Spin State Population Distribution01:14

Atomic Nuclei: Nuclear Spin State Population Distribution

967
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
967
Kinetic Energy - II00:56

Kinetic Energy - II

6.0K
The kinetic energy of a particle is one-half of the product of the particle’s mass and the square of its speed. Note that just as Newton’s second law can be expressed as either the rate of change of momentum or mass multiplied by the rate of change of velocity, so too can the kinetic energy of a particle be expressed in terms of its mass and momentum, instead of its mass and velocity. 
6.0K

You might also read

Related Articles

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

Sort by
Same author

Stripped-Envelope Supernovae for QCD Axion Detection.

Physical review letters·2026
Same author

Lepton-Number Crossings are Insufficient for Flavor Instabilities.

Physical review letters·2026
Same author

Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae.

Physical review letters·2025
Same author

Leading Bounds on Micrometer to Picometer Fifth Forces from Neutron Star Cooling.

Physical review letters·2025
Same author

Energy Transfer by Feebly Interacting Particles in Supernovae: The Trapping Regime.

Physical review letters·2025
Same author

Collective Flavor Conversions Are Interactions of Neutrinos with Quantized Flavor Waves.

Physical review letters·2025
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: Jun 18, 2025

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

8.5K

Inhomogeneous Kinetic Equation for Mixed Neutrinos: Tracing the Missing Energy.

Damiano F G Fiorillo1, Georg G Raffelt2, Günter Sigl3

  • 1Niels Bohr International Academy, <a href="https://ror.org/035b05819">Niels Bohr Institute</a>, University of Copenhagen, 2100 Copenhagen, Denmark.

Physical Review Letters
|July 29, 2024
PubMed
Summary

Fast flavor conversion in neutrinos leads to exponential growth of inhomogeneities, violating energy conservation. This energy is traded with kinetic energy via flavor coherence gradients, requiring new terms in neutrino transport equations.

More Related Videos

Study of Protein Dynamics via Neutron Spin Echo Spectroscopy
08:03

Study of Protein Dynamics via Neutron Spin Echo Spectroscopy

Published on: April 13, 2022

2.1K
High-Resolution Neutron Spectroscopy to Study Picosecond-Nanosecond Dynamics of Proteins and Hydration Water
08:48

High-Resolution Neutron Spectroscopy to Study Picosecond-Nanosecond Dynamics of Proteins and Hydration Water

Published on: April 28, 2022

1.7K

Related Experiment Videos

Last Updated: Jun 18, 2025

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

8.5K
Study of Protein Dynamics via Neutron Spin Echo Spectroscopy
08:03

Study of Protein Dynamics via Neutron Spin Echo Spectroscopy

Published on: April 13, 2022

2.1K
High-Resolution Neutron Spectroscopy to Study Picosecond-Nanosecond Dynamics of Proteins and Hydration Water
08:48

High-Resolution Neutron Spectroscopy to Study Picosecond-Nanosecond Dynamics of Proteins and Hydration Water

Published on: April 28, 2022

1.7K

Area of Science:

  • Neutrino Physics
  • Astrophysical Plasma Physics

Background:

  • Flavor-dependent neutrino transport is typically modeled using kinetic equations for occupation-number matrices.
  • Fast flavor conversion introduces complex dynamics not fully captured by standard models.

Purpose of the Study:

  • To investigate the implications of fast flavor conversion on neutrino transport.
  • To identify and address the violation of neutrino-neutrino refractive energy conservation.
  • To derive the necessary terms for accurate modeling of neutrino flavor evolution.

Main Methods:

  • Analysis of kinetic equations for occupation-number matrices in flavor space.
  • Theoretical derivation of gradient terms related to neutrino flavor coherence.
  • Comparison with existing models and numerical observations.

Main Results:

  • Identified a violation of neutrino-neutrino refractive energy conservation due to self-induced exponential growth of inhomogeneities.
  • Demonstrated that kinetic energy is traded with flavor coherence gradients.
  • Derived the missing gradient terms essential for describing flavor evolution.

Conclusions:

  • Standard neutrino transport equations require modification to account for energy exchange with flavor coherence.
  • Energy conservation is not a primary factor in explaining the final states of fast flavor conversion phenomena.
  • The derived terms are crucial for accurate simulations of astrophysical environments with fast neutrino oscillations.