{ "id": "2104.00014", "version": "v1", "published": "2021-03-31T18:00:03.000Z", "updated": "2021-03-31T18:00:03.000Z", "title": "Evidence of TeV Halos Around Millisecond Pulsars", "authors": [ "Dan Hooper", "Tim Linden" ], "comment": "8 pages, 5 figures", "categories": [ "astro-ph.HE", "astro-ph.GA", "hep-ph" ], "abstract": "Using data from the HAWC gamma-ray Telescope, we have studied a sample of 37 millisecond pulsars (MSPs), selected for their spindown power and proximity. From among these MSP, we have identified four which favor the presence of very high-energy gamma-ray emission at a level of $(2\\Delta \\ln \\mathcal{L})^{1/2} \\ge 2.5$. Adopting a correlation between the spindown power and gamma-ray luminosity of each pulsar, we performed a stacked likelihood analysis of these 37 MSPs, finding that the data supports the conclusion that these sources emit very high-energy gamma-rays at a level of $(2\\Delta \\ln \\mathcal{L})^{1/2} = 4.24$. Among sets of randomly selected sky locations within HAWC's field-of-view, less than 1\\% of such realizations yielded such high statistical significance. Our analysis suggests that MSPs produce very high-energy gamma-ray emission with a similar efficiency to that observed from the Geminga TeV-halo, $\\eta_{\\rm MSP} = (0.39-1.08) \\times \\eta_{\\rm Geminga}$. This conclusion poses a significant challenge for pulsar interpretations of the Galactic Center gamma-ray excess, as it suggests that any population of MSPs potentially capable of producing the GeV excess would also produce TeV-scale emission in excess of that observed by HESS from this region. Future observations by CTA will be able to substantially clarify this situation.", "revisions": [ { "version": "v1", "updated": "2021-03-31T18:00:03.000Z" } ], "analyses": { "keywords": [ "millisecond pulsars", "tev halos", "high-energy gamma-ray emission", "galactic center gamma-ray excess", "spindown power" ], "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable" } } }