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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Bibliographic Details
Published inChinese physics B Vol. 18; no. 12; pp. 5575 - 5582
Main Author 任军 贾孟文 袁常青
Format Journal Article
LanguageEnglish
Published IOP Publishing 01.12.2009
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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.
Bibliography:gravitational field, general relativity, neutrino interference phase, Kerr space-time, geodesic line
O572.321
11-5639/O4
O441
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ISSN:1674-1056
2058-3834
DOI:10.1088/1674-1056/18/12/073