Neutrino oscillation interference phase in Kerr space-time
The mass neutrino interference phases along the null trajectory and the geodesic line in Kerr space-time are studied on the plane θ = π/2. Because of the rotation object in Kerr space-time, a particle travelling along the radial geodesic must have a dragging effect produced by the angular momentum o...
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Published in | Chinese physics B Vol. 18; no. 12; pp. 5575 - 5582 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
IOP Publishing
01.12.2009
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Subjects | |
Online Access | Get full text |
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Summary: | The mass neutrino interference phases along the null trajectory and the geodesic line in Kerr space-time are studied on the plane θ = π/2. Because of the rotation object in Kerr space-time, a particle travelling along the radial geodesic must have a dragging effect produced by the angular momentum of the central object. We give the correction of the phase due to the rotation of the space-time. We find that the type-I interference phase along the geodesic remains the double of that along the null on the condition that the rotating quantity parameter a^2 is preserved and the higher order terms are negligible (e.g. a^4). In addition, we calculate the proper oscillation length in Kerr space-time. All of our results can return to those in Schwarzschild space-time as the rotating parameter a approaches zero. |
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Bibliography: | gravitational field, general relativity, neutrino interference phase, Kerr space-time, geodesic line O572.321 11-5639/O4 O441 ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 ObjectType-Article-1 ObjectType-Feature-2 |
ISSN: | 1674-1056 2058-3834 |
DOI: | 10.1088/1674-1056/18/12/073 |