Infimum Microlensing Amplification of the Maximum Number of Images ofn‐Point Lens Systems
Author(s) -
Sun Hong Rhie
Publication year - 1997
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/304336
Subject(s) - caustic (mathematics) , gravitational microlensing , physics , infimum and supremum , lens (geology) , binary number , point (geometry) , plane (geometry) , astrophysics , point source , optics , mathematical analysis , geometry , stars , mathematics , arithmetic , mathematical physics
The total amplification of a source inside a caustic curve of a binary lens is no less than 3. Here we show that the infimum amplification, 3, is satisfied by a family of binary lenses where the source position is at the midpoint of the lens positions, independent of the mass ratio that parameterizes the family. We present a new proof of an underlying constraint that the total amplification of the two positive images is larger than that of the three negative images by 1 inside a caustic. We show that a similar constraint holds for an arbitrary class of n-point lens systems for sources in the "maximal domains." We introduce the notions that a source plane consists of "graded caustic domains" and that the "maximal domain" is the area of the source plane where a source star produces the maximum number of images, n2 + 1. We show that the infimum amplification of a three-point lens is 7 and that the amplification is larger than n2 + 1 - n for n ≥ 4.
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