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Gravitational Microlensing in NUT Space

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arxiv astro-ph/0204282 v3 pith:IRQTJLFA submitted 2002-04-17 astro-ph gr-qc

Gravitational Microlensing in NUT Space

classification astro-ph gr-qc
keywords microlensinglightmagneticspacecurveseffecteventsgravitational
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the theoretical signature of magnetic masses on the light curve of gravitational microlensing effect in NUT space. The light curves for microlensing events in NUT space are presented and contrasted with those due to lensing produced by normal matter. In the next step, associating magnetic mass to massive astrophysical compact objects (MACHOs), we try to see its effect on the light curves of microlensing candidates observered by the MACHO group. Presence or absence of this feature in the observed microlensing events can shed light on the question of the existence of magnetic masses in the Universe.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Memory effect from the scattering of Taub-NUT black holes

    hep-th 2026-03 conditional novelty 7.0

    Soft theorems yield a gauge-invariant nutty soft factor and the associated memory tensor for Kerr-Taub-NUT scattering, with magnetic components and directional divergences absent in electromagnetism.