Limits on primordial black hole evaporation from H.E.S.S. observations
- Tavernier, T.
- Glicenstein, J. F.
- Brun, F.
- Marandon, V.
- Abdalla, H.
- Aharonian, F.
- Ait-Benkhali, F.
- Anguener, O.
- Arcaro, C.
- Armand, C.
- Armstrong, T.
- Ashkar, H.
- Backes, M.
- Baghmanyan, V.
- Barbosa Martins, V.
- Barnacka, Anna
- Barnard, M.
- Batzofin, R.
- Becherini, Y.
- Berge, D.
- Bernloehr, K.
- Bi, B.
- Böttcher, M.
- Boisson, C.
- Bolmont, J.
- Bony (de), M.
- Breuhaus, M.
- Brose, R.
- Bulik, T.
- Bylund, T.
- Cangemi, F.
- Caroff, S.
- Casanova, S.
- Catalano, J.
- Chambery, P.
- Chand, T. B.
- Chen, A.
- Cotter, G.
- Curlo, M.
- Dalgleish, H.
- Damascene Mbarubucyeye, J.
- Davids, I. D.
- Davies, J.
- Devin, J.
- Djannati-Ataï, A.
- Dmytriiev, A.
- Donath, A.
- Doroshenko, V.
- Dreyer, L.
- Du Plessis, L.
- Duffy, C.
- Egberts, K.
- Einecke, S.
- Ernenwein, J. P.
- Fegan, S.
- Feijen, K.
- Fiasson, A.
- Fichet de Clairfontaine, G.
- Fontaine, G.
- Frans, L.
- Fuessling, M.
- Funk, S.
- Gabici, S.
- Gallant, Y.
- Giavitto, G.
- Giunti, L.
- Glawion, D.
- Grondin, M. H.
- Hattingh, S.
- Haupt, M.
- Hermann, G.
- Hinton, J.
- Hofmann, W.
- Hoischen, C.
- Holch, T.
- Holler, M.
- Horns, D.
- Huang, Z.
- Huber, D.
- Hörbe, M.
- Jamrozy, Marek
- Jankowsky, F.
- Joshi, V.
- Jung, I.
- Kasai, E.
- Katarzynski, K.
- Katz, U.
- Khangulyan, D.
- Khelifi, B.
- Klepser, S.
- Kluzniak, W.
- Komin, N.
- Konno, R.
- Kosack, K.
- Kostunin, D.
- Kreter, M.
- Kukec Mezek, G.
- Kundu, A.
- Lamanna, G.
- Le Stum, S.
- Lemiere, A.
- Lemoine-Goumard, M.
- Lenain, J. P.
- Leuschner, F.
- Levy, C.
- Lohse, T.
- Luashvili, A.
- Lypova, I.
- Mackey, J.
- Majumdar, J.
- Malyshev, D.
- Marchegiani, P.
- Marcowith, A.
- Mares, A.
- Marti'i-Devesa, G.
- Marx, R.
- Maurin, G.
- Meintjes, P.
- Meyer, M.
- Mitchell, A.
- Moderski, R.
- Mohrmann, L.
- Montanari, A.
- Moore, C.
- Morris, P.
- Moulin, E.
- Muller, J.
- Murach, T.
- Nakashima, K.
- Naurois (de), M.
- Nayerhoda, A.
- Davids, H.
- Niemiec, J.
- Noel, Angel
- O'Brien, P.
- Oberholzer, L. L.
- Ohm, S.
- Olivera-Nieto, L.
- Ona-Wilhelmi (de), E.
- Ostrowski, Michał
- Panny, S.
- Panter, M.
- Parsons, D.
- Peron, G.
- Pita, S.
- Poireau, V.
- Prokhorov, D.
- Prokoph, H.
- Puehlhofer, G.
- Punch, M.
- Quirrenbach, A.
- Reichherzer, P.
- Reimer, A.
- Reimer, O.
- Remy, Q.
- Renaud, M.
- Reville, B.
- Rieger, F.
- Romoli, C.
- Rowell, G.
- Rudak, B.
- Rueda Ricarte, H.
- Ruiz Velasco, E.
- Sahakian, V.
- Sailer, S.
- Salzmann, H.
- Sanchez, D.
- Santangelo, A.
- Sasaki, M.
- Schaefer, J.
- Schutte, H.
- Schwanke, U.
- Schüssler, F.
- Senniappan, M.
- Seyffert, A.
- Shapopi, J. N. S.
- Shiningayamwe, K.
- Simoni, R.
- Sinha, A.
- Sol, H.
- Spackman, H.
- Specovius, A.
- Spencer, S. T.
- Spir-Jacob, M.
- Stawarz, Łukasz
- Steenkamp, R.
- Stegmann, C.
- Steinmassl, S.
- Steppa, C.
- Sun, L.
- Takahashi, T.
- Tanaka, T.
- Taylor, A.
- Terrier, R.
- Thiersen, H.
- Thorpe-Morgan, C.
- Tluczykont, M.
- Tomankova, L.
- Tsirou, M.
- Tsuji, N.
- Tuffs, R.
- Uchiyama, Y.
- van der Walt, J.
- van Eldik, C.
- van Rensburg, C.
- van Soelen, B.
- Vasileiadis, G.
- Veh, J.
- Venter, C.
- Vincent, P.
- Vink, J.
- Völk, H. J.
- Wagner, S.
- Watson, J. J.
- Werner, F.
- White, R.
- Wierzcholska, Alicja
- Wong, Y. W.
- Yassin, H.
- Yusafzai, A.
- Zacharias, M.
- Zanin, R.
- Zargaryan, D.
- Zdziarski, A.
- Zech, A.
- Zhu, S.
- Zmija, A.
- Zouari, S.
- Żywucka, N.
Publication date
January 2022
DOI Publisher
Sissa Medialab Journal
1824-8039 Language
EnglishAbstract
Primordial Black Holes are expected to be formed in the early Universe by the gravitational collapse of overdense regions, among other mechanisms. They are also expected to loose their mass over time by the Hawking radiation process. As the rates of this radiation increase with temperature, the PBH evaporation should result in a violent explosion. The current upper limits on explosion rates are on the order of 10$^{4}$ − 10$^{5}$pc$^{-3}$yr$^{-1}$. In this contribution we'll present the results of a search for TeV γ-ray burst within timescale of few seconds, using nearly 5000 hours of H.E.S.S. data. The search algorithm and statistical estimation strategy will be presented as well as cosmological implications of this measurement
.png%3Fwidth%3D300&w=3840&q=75)
Add to ORKG