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arXiv · 1811.11732

Searching for Dark Matter Sub-structure with HAWC

A. U. Abeysekara·A. Albert·R. Alfaro·C. Alvarez·R. Arceo·J. C. Arteaga-Velázquez·D. Avila Rojas·H. A. Ayala Solares·E. Belmont-Moreno·S. Y. BenZvi·C. Brisbois·K. S. Caballero-Mora·A. Carramiñana·S. Casanova·J. Cotzomi·S. Coutiño de León·C. De León·E. De la Fuente·S. Dichiara·B. L. Dingus·M. A. DuVernois·J. C. Díaz-Vélez·K. Engel·C. Espinoza·H. Fleischhack·N. Fraija·A. Galván-Gámez·J. A. García-González·M. M. González·J. A. Goodman·J. P. Harding·B. Hona·F. Hueyotl-Zahuantitla·P. Hüntemeyer·A. Iriarte·A. Lara·W. H. Lee·H. León Vargas·J. T. Linnemann·A. L. Longinotti·G. Luis-Raya·J. Lundeen·K. Malone·S. S. Marinelli·O. Martinez·I. Martinez-Castellanos·J. Martínez-Castro·J. A. Matthews·P. Miranda-Romagnoli·E. Moreno·M. Mostafá·A. Nayerhoda·L. Nellen·M. Newbold·M. U. Nisa·R. Noriega-Papaqui·E. G. Pérez-Pérez·Z. Ren·C. D. Rho·C. Rivière·D. Rosa-González·M. Rosenberg·H. Salazar·F. Salesa Greus·A. Sandoval·M. Schneider·G. Sinnis·A. J. Smith·R. W. Springer·K. Tollefson·I. Torres·G. Vianello·T. Weisgarber·J. Wood·T. Yapici·A. Zepeda·H. Zhou·J. D. Álvarez
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Abstract

Simulations of dark matter show a discrepancy between the expected number of Galactic dark matter sub-halos and how many have been optically observed. Some of these unseen satellites may exist as dark dwarf galaxies: sub-halos like dwarf galaxies with no luminous counterpart. Assuming WIMP dark matter, it may be possible to detect these unseen sub-halos from gamma-ray signals originating from dark matter annihilation. The High Altitude Water Cherenkov Observatory (HAWC) is a very high energy (500 GeV to 100 TeV) gamma ray detector with a wide field-of-view and near continuous duty cycle, making HAWC ideal for unbiased sky surveys. We perform such a search for gamma ray signals from dark dwarfs in the Milky Way halo. We perform a targeted search of HAWC gamma-ray sources which have no known association with lower-energy counterparts, based on an unbiased search of the entire sky. With no sources found to strongly prefer dark matter models, we calculate the ability of HAWC to observe dark dwarfs. We also compute the HAWC sensitivity to potential future detections for a given model of dark matter substructure.

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A. U. Abeysekara, A. Albert, R. Alfaro, C. Alvarez, R. Arceo, J. C. Arteaga-Velázquez, D. Avila Rojas, H. A. Ayala Solares, E. Belmont-Moreno, S. Y. BenZvi, C. Brisbois, K. S. Caballero-Mora, A. Carramiñana, S. Casanova, J. Cotzomi, S. Coutiño de León, C. De León, E. De la Fuente, S. Dichiara, B. L. Dingus, M. A. DuVernois, J. C. Díaz-Vélez, K. Engel, C. Espinoza, H. Fleischhack, N. Fraija, A. Galván-Gámez, J. A. García-González, M. M. González, J. A. Goodman, J. P. Harding, B. Hona, F. Hueyotl-Zahuantitla, P. Hüntemeyer, A. Iriarte, A. Lara, W. H. Lee, H. León Vargas, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, J. Lundeen, K. Malone, S. S. Marinelli, O. Martinez, I. Martinez-Castellanos, J. Martínez-Castro, J. A. Matthews, P. Miranda-Romagnoli, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, M. Newbold, M. U. Nisa, R. Noriega-Papaqui, E. G. Pérez-Pérez, Z. Ren, C. D. Rho, C. Rivière, D. Rosa-González, M. Rosenberg, H. Salazar, F. Salesa Greus, A. Sandoval, M. Schneider, G. Sinnis, A. J. Smith, R. W. Springer, K. Tollefson, I. Torres, G. Vianello, T. Weisgarber, J. Wood, T. Yapici, A. Zepeda, H. Zhou, J. D. Álvarez. 2019-06-20. Searching for Dark Matter Sub-structure with HAWC. https://doi.org/10.1088/1475-7516%2F2019%2F07%2F022

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