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Reduced Mass Coordinates: Isolated Two-body Problem01:12

Reduced Mass Coordinates: Isolated Two-body Problem

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In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...
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Symmetry in Maxwell's Equations01:28

Symmetry in Maxwell's Equations

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Once the fields have been calculated using Maxwell's four equations, the Lorentz force equation gives the force that the fields exert on a charged particle moving with a certain velocity. The Lorentz force equation combines the force of the electric field and of the magnetic field on the moving charge. Maxwell's equations and the Lorentz force law together encompass all the laws of electricity and magnetism. The symmetry that Maxwell introduced into his mathematical framework may not be...
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Gravitation Between Spherically Symmetric Masses01:14

Gravitation Between Spherically Symmetric Masses

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The gravitational potential energy between two spherically symmetric bodies can be calculated from the masses and the distance between the bodies, assuming that the center of mass is concentrated at the respective centers of the bodies.
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Detection of Black Holes01:10

Detection of Black Holes

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Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
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Gauss's Law: Planar Symmetry01:27

Gauss's Law: Planar Symmetry

10.2K
A planar symmetry of charge density is obtained when charges are uniformly spread over a large flat surface. In planar symmetry, all points in a plane parallel to the plane of charge are identical with respect to the charges. Suppose the plane of the charge distribution is the xy-plane, and the electric field at a space point P with coordinates (x, y, z) is to be determined. Since the charge density is the same at all (x, y) - coordinates in the z = 0 plane, by symmetry, the electric field at P...
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Gauss's Law: Cylindrical Symmetry01:20

Gauss's Law: Cylindrical Symmetry

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A charge distribution has cylindrical symmetry if the charge density depends only upon the distance from the axis of the cylinder and does not vary along the axis or with the direction about the axis. In other words, if a system varies if it is rotated around the axis or shifted along the axis, it does not have cylindrical symmetry. In real systems, we do not have infinite cylinders; however, if the cylindrical object is considerably longer than the radius from it that we are interested in,...
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Related Experiment Video

Updated: Apr 1, 2026

Setting Limits on Supersymmetry Using Simplified Models
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Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

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Minimal Left-Right Symmetric Dark Matter.

Julian Heeck1, Sudhanwa Patra2,3

  • 1Service de Physique Théorique, Université Libre de Bruxelles, Boulevard du Triomphe, CP225, 1050 Brussels, Belgium.

Physical Review Letters
|October 3, 2015
PubMed
Summary

Left-right symmetric models offer a straightforward path to stable TeV-scale dark matter. This stability is achieved without special symmetries, utilizing existing or accidental symmetries within the model framework.

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Area of Science:

  • Particle Physics
  • Cosmology
  • High Energy Physics

Background:

  • Dark matter remains a significant mystery in cosmology, with its particle nature yet to be identified.
  • Left-right symmetric models provide a theoretical framework for extending the Standard Model of particle physics.
  • Previous models often required ad hoc symmetries to stabilize dark matter candidates.

Purpose of the Study:

  • To demonstrate that left-right symmetric models can naturally accommodate stable dark matter particles at the TeV scale.
  • To explore minimal dark matter frameworks within these models.
  • To investigate the implications for recent experimental anomalies, such as the diboson excess at ATLAS.

Main Methods:

  • Investigating the stability of dark matter candidates within the context of left-right symmetry.
  • Analyzing minimal examples using left-right fermion triplets and quintuplets.
  • Examining the role of the unbroken Z_{2} subgroup of B-L symmetry.

Main Results:

  • Stable TeV-scale dark matter particles can be accommodated without additional stabilizing symmetries.
  • The stability arises either accidentally or from the residual Z_{2} symmetry.
  • Minimal examples like fermion triplets and quintuplets form viable two-component dark matter.
  • The framework is consistent with SU(2)×SU(2)×U(1) models explaining the ATLAS diboson excess.

Conclusions:

  • Left-right symmetric models offer a compelling and economical solution for dark matter.
  • The proposed mechanism simplifies dark matter model building by reducing the need for fine-tuning or extra symmetries.
  • This approach provides a testable framework with direct implications for ongoing and future high-energy physics experiments.