Planet nine, dark matter and MOND

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7156

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.contributor.author	Arun, K	-
dc.contributor.author	Kiren, O. V	-
dc.date.accessioned	2020-11-17T14:26:01Z	-
dc.date.available	2020-11-17T14:26:01Z	-
dc.date.issued	2016-07	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 361, No. 7, 230	en_US
dc.identifier.issn	1572-946X	-
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/7156	-
dc.description	Restricted Access © Springer The original publication is available at springerlink.com http://dx.doi.org/10.1007/s10509-016-2815-z	en_US
dc.description.abstract	Here we propose the possibility that the recently postulated Neptune-sized planet with an orbital period of 15,000 years could be a gravitationally condensed dark matter (DM) object. The observed mass of Planet Nine fits with the theoretical mass predicted for such DM objects formed by 60 GeV DM particles, which is the currently favoured DM particles. This object could also provide us with a testing ground for modification of Newtonian dynamics.	en_US
dc.language.iso	en	en_US
dc.publisher	Springer	en_US
dc.subject	Planet Nine	en_US
dc.subject	Dark matter	en_US
dc.subject	MOND	en_US
dc.title	Planet nine, dark matter and MOND	en_US
dc.type	Article	en_US
Appears in Collections:	IIAP Publications

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