Microlens of light rays near photon sphere

Naoki Tsukamoto

Microlens of light rays near photon sphere

Naoki Tsukamoto

Department of Physics

Research output: Contribution to conference › Paper › peer-review

Abstract

We have investigated the microlensing of the light rays which have passed Ellis wormhole throat. • The closest distance β between the source and Φ = π decides the maximum of apparent brightness of the light curve. • We would distinguish the light curves from the usual light curves of mass lenses. • Our method would be applied for passable wormholes with positive masses easily.

Original language	English
Pages	39-48
Number of pages	10
Publication status	Published - 2015
Event	25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015 - Kyoto, Japan Duration: 7 Dec 2015 → 11 Dec 2015

Conference

Conference	25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Country/Territory	Japan
City	Kyoto
Period	7/12/15 → 11/12/15

Cite this

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title = "Microlens of light rays near photon sphere",

abstract = "We have investigated the microlensing of the light rays which have passed Ellis wormhole throat. • The closest distance β between the source and Φ = π decides the maximum of apparent brightness of the light curve. • We would distinguish the light curves from the usual light curves of mass lenses. • Our method would be applied for passable wormholes with positive masses easily.",

author = "Naoki Tsukamoto",

note = "Publisher Copyright: {\textcopyright} Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015. All rights reserved.; 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015 ; Conference date: 07-12-2015 Through 11-12-2015",

year = "2015",

language = "English",

pages = "39--48",

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T1 - Microlens of light rays near photon sphere

AU - Tsukamoto, Naoki

PY - 2015

Y1 - 2015

N2 - We have investigated the microlensing of the light rays which have passed Ellis wormhole throat. • The closest distance β between the source and Φ = π decides the maximum of apparent brightness of the light curve. • We would distinguish the light curves from the usual light curves of mass lenses. • Our method would be applied for passable wormholes with positive masses easily.

AB - We have investigated the microlensing of the light rays which have passed Ellis wormhole throat. • The closest distance β between the source and Φ = π decides the maximum of apparent brightness of the light curve. • We would distinguish the light curves from the usual light curves of mass lenses. • Our method would be applied for passable wormholes with positive masses easily.

UR - https://www.scopus.com/pages/publications/85092231300

M3 - Paper

AN - SCOPUS:85092231300

SP - 39

EP - 48

T2 - 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015

Y2 - 7 December 2015 through 11 December 2015

ER -

Microlens of light rays near photon sphere

Abstract

Conference

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