词条 | Mathisson–Papapetrou–Dixon equations |
释义 |
In physics, specifically general relativity, the Mathisson–Papapetrou–Dixon equations describe the motion of a massive spinning body moving in a gravitational field. Other equations with similar names and mathematical forms are the Mathisson-Papapetrou equations and Papapetrou-Dixon equations. All three sets of equations describe the same physics. They are named for M. Mathisson,[1] W. G. Dixon,[2] and A. Papapetrou.[3] Throughout, this article uses the natural units c = G = 1, and tensor index notation. Matthisson-Papapetrou–Dixon equationsThe Matthisson-Papapetrou-Dixon (MPD) equations for a mass spinning body are Here is the proper time along the trajectory, is the body's four-momentum the vector is the four-velocity of some reference point in the body, and the skew-symmetric tensor is the angular momentum of the body about this point. In the time-slice integrals we are asuming that the body is compact enough that we can use flat coordinates within the body where the energy-momentum tensor is non-zero. As they stand, there are only ten equations to determine thirteen quantities. These quantities are the six components of , the four components of and the three independent components of . The equations must therefore be supplimented by three additional constraints which serve to determine which point in the body has velocity . Matthison and Pirani originally chose to impose the condition which, although involving four components, contains only three constraints because is identically zero. This condition, however, leads to mysterious "helical motions" [4]. The Tulczyjew-Dixon condition is perhaps more physically reasonable as it selects the reference point to be the body's center of mass in the frame in which its momentum is . Accepting the Tulczyjew-Dixon condition , we can manipulate the second of the MPD equations into the form This is a form of Fermi-Walker transport of the spin tensor along the trajectory - but one preserving orthogonality to the momentum vector rather than to the tangent vector . Dixon calls this M-transport. See also
ReferencesNotes1. ^{{cite news |author=M. Mathisson|title=Neue Mechanik materieller Systeme |journal=Acta Physica Polonica |volume=6 |year=1937 |pages=163–209 |url=http://inspirehep.net/record/48323/citations}} 2. ^{{cite journal |title=Dynamics of Extended Bodies in General Relativity. I. Momentum and Angular Momentum |author=W. G. Dixon |url=http://rspa.royalsocietypublishing.org/content/314/1519/499.full.pdf+html |year=1970 |doi=10.1098/rspa.1970.0020 |journal=Proc. R. Soc. Lond. A |volume=314 |issue=1519 |bibcode=1970RSPSA.314..499D |pages=499–527}} 3. ^{{cite journal |author=A. Papapetrou |title=Spinning Test-Particles in General Relativity. I |url=http://rspa.royalsocietypublishing.org/content/209/1097/248.full.pdf+html |year=1951 |doi=10.1098/rspa.1951.0200 |journal=Proc. R. Soc. Lond. A |volume=209 |issue=1097 |bibcode=1951RSPSA.209..248P |pages=248–258}} 4. ^{{cite journal|title=Mathisson's helical motions demystified|journal=AIP Conf. Proc.|volume=1458 |pages=367–370 |author1=L. F. O. Costa |author2=J. Natário |author3=M. Zilhão |year=2012|arxiv=1206.7093|doi=10.1063/1.4734436|series=AIP Conference Proceedings }} Selected papers
|journal=Physics Letters A|year=2005|volume=343|issue=1–3|pages=1–7|title=Relativistic motion of spinning particles in a gravitational field|doi=10.1016/j.physleta.2005.05.072|arxiv=gr-qc/0504146|bibcode=2005PhLA..343....1C|hdl=10355/8357 }}
|author=M. Leclerc|year=2005|doi=10.1088/0264-9381/22/16/006|arxiv=gr-qc/0505021|volume=22|issue=16|journal=Classical and Quantum Gravity|pages=3203–3221|bibcode=2005CQGra..22.3203L}}
2 : Equations|General relativity |
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