https://arxiv.org/abs/1909.11090 close this message Donate to arXiv Please join the Simons Foundation and our generous member organizations in supporting arXiv during our giving campaign September 23-27. 100% of your contribution will fund improvements and new initiatives to benefit arXiv's global scientific community. DONATE [secure site, no need to create account] Skip to main content Cornell University We gratefully acknowledge support from the Simons Foundation and member institutions. arXiv.org > hep-ph > arXiv:1909.11090 [ ] Help | Advanced Search [All fields ] Search arXiv Cornell University Logo [ ] GO quick links * Login * Help Pages * About High Energy Physics - Phenomenology arXiv:1909.11090 (hep-ph) [Submitted on 24 Sep 2019] Title:What if Planet 9 is a Primordial Black Hole? Authors:Jakub Scholtz, James Unwin Download PDF Abstract: We highlight that the anomalous orbits of Trans-Neptunian Objects (TNOs) and an excess in microlensing events in the 5-year OGLE dataset can be simultaneously explained by a new population of astrophysical bodies with mass several times that of Earth ($M_\oplus$). We take these objects to be primordial black holes (PBHs) and point out the orbits of TNOs would be altered if one of these PBHs was captured by the Solar System, inline with the Planet 9 hypothesis. Capture of a free floating planet is a leading explanation for the origin of Planet 9 and we show that the probability of capturing a PBH instead is comparable. The observational constraints on a PBH in the outer Solar System significantly differ from the case of a new ninth planet. This scenario could be confirmed through annihilation signals from the dark matter microhalo around the PBH. Comments: 7 pages, 1 exact scale illustration of a 5 Earth mass black hole High Energy Physics - Phenomenology (hep-ph); Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO); Earth and Planetary Astrophysics (astro-ph.EP) Journal reference: Phys. Rev. Lett. 125, 051103 (2020) DOI: 10.1103/PhysRevLett.125.051103 Report number: IPPP/19/73 Cite as: arXiv:1909.11090 [hep-ph] (or arXiv:1909.11090v1 [hep-ph] for this version) Submission history From: James Unwin [view email] [v1] Tue, 24 Sep 2019 18:00:01 UTC (19 KB) Full-text links: Download: * PDF * Other formats (license) Current browse context: hep-ph < prev | next > new | recent | 1909 Change to browse by: astro-ph astro-ph.CO astro-ph.EP References & Citations * INSPIRE HEP * NASA ADS * Google Scholar * Semantic Scholar 3 blog links (what is this?) a export bibtex citation Loading... Bibtex formatted citation x [loading... ] Data provided by: Bookmark BibSonomy logo Mendeley logo Reddit logo ScienceWISE logo (*) Bibliographic Tools Bibliographic and Citation Tools [ ] Bibliographic Explorer Toggle Bibliographic Explorer (What is the Explorer?) [ ] Litmaps Toggle Litmaps (What is Litmaps?) ( ) Code & Data Code and Data Associated with this Article [ ] arXiv Links to Code Toggle arXiv Links to Code & Data (What is Links to Code & Data?) ( ) Related Papers Recommenders and Search Tools [ ] Connected Papers Toggle Connected Papers (What is Connected Papers?) [ ] Core recommender toggle CORE Recommender (What is CORE?) ( ) About arXivLabs arXivLabs: experimental projects with community collaborators arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs and how to get involved. Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?) * About * Help * Click here to contact arXiv Contact * Click here to subscribe Subscribe * Copyright * Privacy Policy * Web Accessibility Assistance * arXiv Operational Status Get status notifications via email or slack