First HAWC observations of the Sun constrain steady TeV gamma-ray emission

Steady gamma-ray emission up to at least 200 GeV has been detected from the solar disk in the Fermi-LAT data, with the brightest, hardest emission occurring during solar minimum. The likely cause is hadronic cosmic rays undergoing collisions in the Sun’s atmosphere after being redirected from ingoin...

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Main Authors: Albert, A., Alfaro, R., Alvarez, C., Arceo, R., Arteaga-Velázquez, J. C., Avila Rojas, D., Ayala Solares, H. A., Belmont-Moreno, E., BenZvi, S. Y., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotzomi, J., Coutiño de León, S., De León, C., De la Fuente, E., Dichiara, S., Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Engel, K., Enríquez-Rivera, O., Espinoza, C., Fleischhack, H., Fraija, N., García-González, J. A., Garfias, F., González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hona, B., Hueyotl-Zahuantitla, F., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., León Vargas, H., Luis-Raya, G., Lundeen, J., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nayerhoda, A., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Salesa Greus, F., Sandoval, A., Schneider, M., Schoorlemmer, H., Seglar Arroyo, M., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Zepeda, A., Zhou, H., Álvarez, J. D., Beacom, J. F., Linden, T., Ng, K. C. Y., Peter, A. H. G., Zhou, B., Leane, Rebecca K
Other Authors: Massachusetts Institute of Technology. Laboratory for Nuclear Science
Format: Article
Language:English
Published: American Physical Society 2019
Online Access:http://hdl.handle.net/1721.1/120071
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author Albert, A.
Alfaro, R.
Alvarez, C.
Arceo, R.
Arteaga-Velázquez, J. C.
Avila Rojas, D.
Ayala Solares, H. A.
Belmont-Moreno, E.
BenZvi, S. Y.
Brisbois, C.
Caballero-Mora, K. S.
Capistrán, T.
Carramiñana, A.
Casanova, S.
Castillo, M.
Cotzomi, J.
Coutiño de León, S.
De León, C.
De la Fuente, E.
Dichiara, S.
Dingus, B. L.
DuVernois, M. A.
Díaz-Vélez, J. C.
Engel, K.
Enríquez-Rivera, O.
Espinoza, C.
Fleischhack, H.
Fraija, N.
García-González, J. A.
Garfias, F.
González, M. M.
Goodman, J. A.
Hampel-Arias, Z.
Harding, J. P.
Hernandez, S.
Hona, B.
Hueyotl-Zahuantitla, F.
Hüntemeyer, P.
Iriarte, A.
Jardin-Blicq, A.
Joshi, V.
Kaufmann, S.
León Vargas, H.
Luis-Raya, G.
Lundeen, J.
López-Coto, R.
Malone, K.
Marinelli, S. S.
Martinez, O.
Martinez-Castellanos, I.
Martínez-Castro, J.
Miranda-Romagnoli, P.
Moreno, E.
Mostafá, M.
Nayerhoda, A.
Nellen, L.
Newbold, M.
Nisa, M. U.
Noriega-Papaqui, R.
Pretz, J.
Pérez-Pérez, E. G.
Ren, Z.
Rho, C. D.
Rivière, C.
Rosa-González, D.
Rosenberg, M.
Ruiz-Velasco, E.
Salazar, H.
Salesa Greus, F.
Sandoval, A.
Schneider, M.
Schoorlemmer, H.
Seglar Arroyo, M.
Sinnis, G.
Smith, A. J.
Springer, R. W.
Surajbali, P.
Taboada, I.
Tibolla, O.
Tollefson, K.
Torres, I.
Villaseñor, L.
Weisgarber, T.
Westerhoff, S.
Wisher, I. G.
Wood, J.
Yapici, T.
Zepeda, A.
Zhou, H.
Álvarez, J. D.
Beacom, J. F.
Linden, T.
Ng, K. C. Y.
Peter, A. H. G.
Zhou, B.
Leane, Rebecca K
author2 Massachusetts Institute of Technology. Laboratory for Nuclear Science
author_facet Massachusetts Institute of Technology. Laboratory for Nuclear Science
Albert, A.
Alfaro, R.
Alvarez, C.
Arceo, R.
Arteaga-Velázquez, J. C.
Avila Rojas, D.
Ayala Solares, H. A.
Belmont-Moreno, E.
BenZvi, S. Y.
Brisbois, C.
Caballero-Mora, K. S.
Capistrán, T.
Carramiñana, A.
Casanova, S.
Castillo, M.
Cotzomi, J.
Coutiño de León, S.
De León, C.
De la Fuente, E.
Dichiara, S.
Dingus, B. L.
DuVernois, M. A.
Díaz-Vélez, J. C.
Engel, K.
Enríquez-Rivera, O.
Espinoza, C.
Fleischhack, H.
Fraija, N.
García-González, J. A.
Garfias, F.
González, M. M.
Goodman, J. A.
Hampel-Arias, Z.
Harding, J. P.
Hernandez, S.
Hona, B.
Hueyotl-Zahuantitla, F.
Hüntemeyer, P.
Iriarte, A.
Jardin-Blicq, A.
Joshi, V.
Kaufmann, S.
León Vargas, H.
Luis-Raya, G.
Lundeen, J.
López-Coto, R.
Malone, K.
Marinelli, S. S.
Martinez, O.
Martinez-Castellanos, I.
Martínez-Castro, J.
Miranda-Romagnoli, P.
Moreno, E.
Mostafá, M.
Nayerhoda, A.
Nellen, L.
Newbold, M.
Nisa, M. U.
Noriega-Papaqui, R.
Pretz, J.
Pérez-Pérez, E. G.
Ren, Z.
Rho, C. D.
Rivière, C.
Rosa-González, D.
Rosenberg, M.
Ruiz-Velasco, E.
Salazar, H.
Salesa Greus, F.
Sandoval, A.
Schneider, M.
Schoorlemmer, H.
Seglar Arroyo, M.
Sinnis, G.
Smith, A. J.
Springer, R. W.
Surajbali, P.
Taboada, I.
Tibolla, O.
Tollefson, K.
Torres, I.
Villaseñor, L.
Weisgarber, T.
Westerhoff, S.
Wisher, I. G.
Wood, J.
Yapici, T.
Zepeda, A.
Zhou, H.
Álvarez, J. D.
Beacom, J. F.
Linden, T.
Ng, K. C. Y.
Peter, A. H. G.
Zhou, B.
Leane, Rebecca K
author_sort Albert, A.
collection MIT
description Steady gamma-ray emission up to at least 200 GeV has been detected from the solar disk in the Fermi-LAT data, with the brightest, hardest emission occurring during solar minimum. The likely cause is hadronic cosmic rays undergoing collisions in the Sun’s atmosphere after being redirected from ingoing to outgoing in magnetic fields, though the exact mechanism is not understood. An important new test of the gamma-ray production mechanism will follow from observations at higher energies. Only the High Altitude Water Cherenkov (HAWC) Observatory has the required sensitivity to effectively probe the Sun in the TeV range. Using 3 years of HAWC data from November 2014 to December 2017, just prior to the solar minimum, we search for 1–100 TeV gamma rays from the solar disk. No evidence of a signal is observed, and we set strong upper limits on the flux at a few 10[superscript -12]  TeV[superscript -1] cm[superscript -2] s[superscript -1] at 1 TeV. Our limit, which is the most constraining result on TeV gamma rays from the Sun, is ∼10% of the theoretical maximum flux (based on a model where all incoming cosmic rays produce outgoing photons), which in turn is comparable to the Fermi-LAT data near 100 GeV. The prospects for a first TeV detection of the Sun by HAWC are especially high during the solar minimum, which began in early 2018.
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spelling mit-1721.1/1200712022-09-30T12:50:13Z First HAWC observations of the Sun constrain steady TeV gamma-ray emission Albert, A. Alfaro, R. Alvarez, C. Arceo, R. Arteaga-Velázquez, J. C. Avila Rojas, D. Ayala Solares, H. A. Belmont-Moreno, E. BenZvi, S. Y. Brisbois, C. Caballero-Mora, K. S. Capistrán, T. Carramiñana, A. Casanova, S. Castillo, M. Cotzomi, J. Coutiño de León, S. De León, C. De la Fuente, E. Dichiara, S. Dingus, B. L. DuVernois, M. A. Díaz-Vélez, J. C. Engel, K. Enríquez-Rivera, O. Espinoza, C. Fleischhack, H. Fraija, N. García-González, J. A. Garfias, F. González, M. M. Goodman, J. A. Hampel-Arias, Z. Harding, J. P. Hernandez, S. Hona, B. Hueyotl-Zahuantitla, F. Hüntemeyer, P. Iriarte, A. Jardin-Blicq, A. Joshi, V. Kaufmann, S. León Vargas, H. Luis-Raya, G. Lundeen, J. López-Coto, R. Malone, K. Marinelli, S. S. Martinez, O. Martinez-Castellanos, I. Martínez-Castro, J. Miranda-Romagnoli, P. Moreno, E. Mostafá, M. Nayerhoda, A. Nellen, L. Newbold, M. Nisa, M. U. Noriega-Papaqui, R. Pretz, J. Pérez-Pérez, E. G. Ren, Z. Rho, C. D. Rivière, C. Rosa-González, D. Rosenberg, M. Ruiz-Velasco, E. Salazar, H. Salesa Greus, F. Sandoval, A. Schneider, M. Schoorlemmer, H. Seglar Arroyo, M. Sinnis, G. Smith, A. J. Springer, R. W. Surajbali, P. Taboada, I. Tibolla, O. Tollefson, K. Torres, I. Villaseñor, L. Weisgarber, T. Westerhoff, S. Wisher, I. G. Wood, J. Yapici, T. Zepeda, A. Zhou, H. Álvarez, J. D. Beacom, J. F. Linden, T. Ng, K. C. Y. Peter, A. H. G. Zhou, B. Leane, Rebecca K Massachusetts Institute of Technology. Laboratory for Nuclear Science Leane, Rebecca K Steady gamma-ray emission up to at least 200 GeV has been detected from the solar disk in the Fermi-LAT data, with the brightest, hardest emission occurring during solar minimum. The likely cause is hadronic cosmic rays undergoing collisions in the Sun’s atmosphere after being redirected from ingoing to outgoing in magnetic fields, though the exact mechanism is not understood. An important new test of the gamma-ray production mechanism will follow from observations at higher energies. Only the High Altitude Water Cherenkov (HAWC) Observatory has the required sensitivity to effectively probe the Sun in the TeV range. Using 3 years of HAWC data from November 2014 to December 2017, just prior to the solar minimum, we search for 1–100 TeV gamma rays from the solar disk. No evidence of a signal is observed, and we set strong upper limits on the flux at a few 10[superscript -12]  TeV[superscript -1] cm[superscript -2] s[superscript -1] at 1 TeV. Our limit, which is the most constraining result on TeV gamma rays from the Sun, is ∼10% of the theoretical maximum flux (based on a model where all incoming cosmic rays produce outgoing photons), which in turn is comparable to the Fermi-LAT data near 100 GeV. The prospects for a first TeV detection of the Sun by HAWC are especially high during the solar minimum, which began in early 2018. United States. Department of Energy. High Energy Physics Division (Grant DE-SC00012567) United States. Department of Energy. High Energy Physics Division (Grant DE-SC0013999) 2019-01-15T19:01:09Z 2019-01-15T19:01:09Z 2018-12 2018-12-17T18:00:19Z Article http://purl.org/eprint/type/JournalArticle 2470-0010 2470-0029 http://hdl.handle.net/1721.1/120071 Albert, A., et al. “First HAWC Observations of the Sun Constrain Steady TeV Gamma-Ray Emission.” Physical Review D, vol. 98, no. 12, Dec. 2018. © 2018 American Physical Society en http://dx.doi.org/10.1103/PhysRevD.98.123011 Physical Review D Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. American Physical Society application/pdf American Physical Society American Physical Society
spellingShingle Albert, A.
Alfaro, R.
Alvarez, C.
Arceo, R.
Arteaga-Velázquez, J. C.
Avila Rojas, D.
Ayala Solares, H. A.
Belmont-Moreno, E.
BenZvi, S. Y.
Brisbois, C.
Caballero-Mora, K. S.
Capistrán, T.
Carramiñana, A.
Casanova, S.
Castillo, M.
Cotzomi, J.
Coutiño de León, S.
De León, C.
De la Fuente, E.
Dichiara, S.
Dingus, B. L.
DuVernois, M. A.
Díaz-Vélez, J. C.
Engel, K.
Enríquez-Rivera, O.
Espinoza, C.
Fleischhack, H.
Fraija, N.
García-González, J. A.
Garfias, F.
González, M. M.
Goodman, J. A.
Hampel-Arias, Z.
Harding, J. P.
Hernandez, S.
Hona, B.
Hueyotl-Zahuantitla, F.
Hüntemeyer, P.
Iriarte, A.
Jardin-Blicq, A.
Joshi, V.
Kaufmann, S.
León Vargas, H.
Luis-Raya, G.
Lundeen, J.
López-Coto, R.
Malone, K.
Marinelli, S. S.
Martinez, O.
Martinez-Castellanos, I.
Martínez-Castro, J.
Miranda-Romagnoli, P.
Moreno, E.
Mostafá, M.
Nayerhoda, A.
Nellen, L.
Newbold, M.
Nisa, M. U.
Noriega-Papaqui, R.
Pretz, J.
Pérez-Pérez, E. G.
Ren, Z.
Rho, C. D.
Rivière, C.
Rosa-González, D.
Rosenberg, M.
Ruiz-Velasco, E.
Salazar, H.
Salesa Greus, F.
Sandoval, A.
Schneider, M.
Schoorlemmer, H.
Seglar Arroyo, M.
Sinnis, G.
Smith, A. J.
Springer, R. W.
Surajbali, P.
Taboada, I.
Tibolla, O.
Tollefson, K.
Torres, I.
Villaseñor, L.
Weisgarber, T.
Westerhoff, S.
Wisher, I. G.
Wood, J.
Yapici, T.
Zepeda, A.
Zhou, H.
Álvarez, J. D.
Beacom, J. F.
Linden, T.
Ng, K. C. Y.
Peter, A. H. G.
Zhou, B.
Leane, Rebecca K
First HAWC observations of the Sun constrain steady TeV gamma-ray emission
title First HAWC observations of the Sun constrain steady TeV gamma-ray emission
title_full First HAWC observations of the Sun constrain steady TeV gamma-ray emission
title_fullStr First HAWC observations of the Sun constrain steady TeV gamma-ray emission
title_full_unstemmed First HAWC observations of the Sun constrain steady TeV gamma-ray emission
title_short First HAWC observations of the Sun constrain steady TeV gamma-ray emission
title_sort first hawc observations of the sun constrain steady tev gamma ray emission
url http://hdl.handle.net/1721.1/120071
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