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Related Concept Videos

Gravitation Between Spherically Symmetric Masses01:14

Gravitation Between Spherically Symmetric Masses

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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Gravity between Spherical Bodies

Newton's law of gravitation describes the gravitational force between any two point masses. However, for extended spherical objects like the Earth, the Moon, and other planets, the law holds with an assumption that masses of spherical objects are concentrated at their respective centers.
This assumption can be proved easily by showing that the expression for gravitational potential energy between a hollow sphere of mass (M) and a point mass (m) is the same as it would be for a pair of extended...
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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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The Principle of Superposition and the Gravitational Field

The principle of superposition applies to gravitational forces of objects that are sufficiently far apart. It states that the net gravitational force on a point object is the vector sum of the gravitational forces on it due to various objects. The principle helps calculate the force by listing the individual forces and then vectorially summing them up. However, it should be noted that the principle of superposition is not always apparent. In the presence of a second force, the first force could...
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Newton's Law of Gravitation

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The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
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Gravitational wave forms for two- and three-body gravitating systems.

Yuji Torigoe1, Keisuke Hattori, Hideki Asada

  • 1Faculty of Science and Technology, Hirosaki University, Hirosaki 036-8561, Japan.

Physical Review Letters
|August 8, 2009
PubMed
Summary

Different particle systems create unique gravitational waves, but some wave forms can appear similar. A new chirp mass for triple systems helps distinguish these sources, suggesting higher multipoles are key for classification.

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Area of Science:

  • Astrophysics
  • Gravitational Wave Astronomy
  • Dynamical Systems

Background:

  • Self-gravitating particle systems exhibit diverse periodic motions.
  • Gravitational wave (GW) signals from these systems can exhibit similarities.
  • Distinguishing between different astrophysical sources of GWs is crucial for interpretation.

Purpose of the Study:

  • To investigate the potential for similar gravitational wave (GW) shapes from systems with different numbers of self-gravitating particles.
  • To develop a method for tracking and differentiating these similar GW waveforms.
  • To explore the utility of higher-order multipoles in classifying GW sources.

Main Methods:

  • Analysis of gravitational wave generation from self-gravitating particles in periodic motion.
  • Definition of a novel chirp mass applicable to triple systems.
  • Comparison of quadrupole waveforms from binary and three-body systems.
  • Investigation of higher-order multipole waveforms for source discrimination.

Main Results:

  • Quadrupole gravitational waveforms from binary and three-body systems can be accidentally similar, hindering source identification.
  • A new chirp mass for triple systems is proposed to track the evolution of similar waveforms.
  • Higher-order multipole waveforms (lth multipoles) show potential for distinguishing between different source systems.

Conclusions:

  • The similarity of quadrupole waveforms necessitates alternative methods for source classification.
  • The proposed chirp mass offers a tool for analyzing triple system evolution.
  • Higher multipole moments are likely essential for accurately classifying gravitational wave sources, with a conjecture that l <= N for N particles.