An Optimized Search for Dark Matter in the Galactic Halo with HAWC

J. Lundeen; J. P. Harding; A. U. Abeysekara; A. Albert; R. Alfaro; C. Alvarez; J. D. Álvarez; J. R. Angeles Camacho; J. C. Arteaga-Velázquez; K. P. Arunbabu; D. Avila Rojas; H. A. Ayala Solares; R. Babu; V. Baghmanyan; A. S. Barber; J. Becerra Gonzalez; E. Belmont-Moreno; S. Y. BenZvi; D. Berley; C. Brisbois; K. S. Caballero-Mora; T. Capistrán; A. Carramiñana; S. Casanova; O. Chaparro-Amaro; U. Cotti; J. Cotzomi; S. Coutiño de León; E. De la Fuente; C. de León; L. Diaz-Cruz; R. Diaz Hernandez; J. C. Díaz-Vélez; B. L. Dingus; M. Durocher; M. A. DuVernois; R. W. Ellsworth; K. Engel; C. Espinoza; K. L. Fan; K. Fang; M. Fernández Alonso; B. Fick; H. Fleischhack; J. L. Flores; N. I. Fraija; D. Garcia; J. A. García-González; J. L. García-Luna; G. García-Torales; F. Garfias; G. Giacinti; H. Goksu; M. M. González; J. A. Goodman; S. Hernandez; I. Herzog; J. Hinton; B. Hona; D. Huang; F. Hueyotl-Zahuantitla; C. M. Hui; B. Humensky; P. Hüntemeyer; A. Iriarte; A. Jardin-Blicq; H. Jhee; V. Joshi; D. Kieda; G. J. Kunde; S. Kunwar; A. Lara; J. Lee; W. H. Lee; D. Lennarz; H. León Vargas; J. Linnemann; A. L. Longinotti; R. López-Coto; G. Luis-Raya; J. Lundeen; K. Malone; V. Marandon; O. Martinez; I. Martinez-Castellanos; H. Martínez-Huerta; J. Martínez-Castro; J. A.J. Matthews; J. McEnery; P. Miranda-Romagnoli; J. A. Morales-Soto; E. Moreno; M. Mostafá; A. Nayerhoda; L. Nellen; M. Newbold; M. U. Nisa; R. Noriega-Papaqui; L. Olivera-Nieto; N. Omodei; A. Peisker; Y. Pérez Araujo; E. G. Pérez-Pérez; C. D. Rho; C. Rivière; D. Rosa-Gonzalez; E. Ruiz-Velasco; J. Ryan; H. Salazar; F. Salesa Greus; A. Sandoval; M. Schneider; H. Schoorlemmer; J. Serna-Franco; G. Sinnis; A. J. Smith; R. W. Springer; P. Surajbali; I. Taboada; M. Tanner; K. Tollefson; I. Torres; R. Torres-Escobedo; R. Turner; F. Ureña-Mena; L. Villaseñor; X. Wang; I. J. Watson; T. Weisgarber; F. Werner; E. Willox; J. Wood; G. B. Yodh; A. Zepeda; H. Zhou

An Optimized Search for Dark Matter in the Galactic Halo with HAWC

J. Lundeen, J. P. Harding, A. U. Abeysekara, A. Albert, R. Alfaro, C. Alvarez, J. D. Álvarez, J. R. Angeles Camacho, J. C. Arteaga-Velázquez, K. P. Arunbabu, D. Avila Rojas, H. A. Ayala Solares, R. Babu, V. Baghmanyan, A. S. Barber, J. Becerra Gonzalez, E. Belmont-Moreno, S. Y. BenZvi, D. Berley, C. BrisboisK. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, O. Chaparro-Amaro, U. Cotti, J. Cotzomi, S. Coutiño de León, E. De la Fuente, C. de León, L. Diaz-Cruz, R. Diaz Hernandez, J. C. Díaz-Vélez, B. L. Dingus, M. Durocher, M. A. DuVernois, R. W. Ellsworth, K. Engel, C. Espinoza, K. L. Fan, K. Fang, M. Fernández Alonso, B. Fick, H. Fleischhack, J. L. Flores, N. I. Fraija, D. Garcia, J. A. García-González, J. L. García-Luna, G. García-Torales, F. Garfias, G. Giacinti, H. Goksu, M. M. González, J. A. Goodman, S. Hernandez, I. Herzog, J. Hinton, B. Hona, D. Huang, F. Hueyotl-Zahuantitla, C. M. Hui, B. Humensky, P. Hüntemeyer, A. Iriarte, A. Jardin-Blicq, H. Jhee, V. Joshi, D. Kieda, G. J. Kunde, S. Kunwar, A. Lara, J. Lee, W. H. Lee, D. Lennarz, H. León Vargas, J. Linnemann, A. L. Longinotti, R. López-Coto, G. Luis-Raya, J. Lundeen, K. Malone, V. Marandon, O. Martinez, I. Martinez-Castellanos, H. Martínez-Huerta, J. Martínez-Castro, J. A.J. Matthews, J. McEnery, P. Miranda-Romagnoli, J. A. Morales-Soto, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, M. Newbold, M. U. Nisa, R. Noriega-Papaqui, L. Olivera-Nieto, N. Omodei, A. Peisker, Y. Pérez Araujo, E. G. Pérez-Pérez, C. D. Rho, C. Rivière, D. Rosa-Gonzalez, E. Ruiz-Velasco, J. Ryan, H. Salazar, F. Salesa Greus, A. Sandoval, M. Schneider, H. Schoorlemmer, J. Serna-Franco, G. Sinnis, A. J. Smith, R. W. Springer, P. Surajbali, I. Taboada, M. Tanner, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, L. Villaseñor, X. Wang, I. J. Watson, T. Weisgarber, F. Werner, E. Willox, J. Wood, G. B. Yodh, A. Zepeda, H. Zhou

Centro de Investigación en Computación (CIC)

Producción científica: Contribución a una revista › Artículo de la conferencia › revisión exhaustiva

1 Cita (Scopus)

Resumen

With a mass of approximately ∼10¹² solar masses, the Galactic Halo is the closest known large dark matter halo and a prime candidate for indirect dark matter detection. The High Altitude Water Cherenkov Observatory (HAWC) is a high energy (300 GeV to 100 TeV) gamma ray detector located in central Mexico. HAWC operates via the water Cherenkov technique and has both a wide field of view of ∼2 sr and a >95% duty cycle, making it ideal for analysis of highly extended sources. We made use of these properties of HAWC and a new background-estimation technique optimized for extended sources to probe a large region of the Galactic Halo for dark matter signals. With this approach and taking into account electroweak corrections to the gamma-ray spectra, we set improved constraints on dark matter annihilation and decay between masses of 10 and 100 TeV. Our constraints also take into account detector simulation systematics and are robust against uncertainties in the Galactic dark matter spatial profile.

Idioma original	Inglés
Número de artículo	531
Publicación	Proceedings of Science
Volumen	395
Estado	Publicada - 18 mar. 2022
Evento	37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Alemania Duración: 12 jul. 2021 → 23 jul. 2021

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Lundeen, J., Harding, J. P., Abeysekara, A. U., Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Angeles Camacho, J. R., Arteaga-Velázquez, J. C., Arunbabu, K. P., Avila Rojas, D., Ayala Solares, H. A., Babu, R., Baghmanyan, V., Barber, A. S., Becerra Gonzalez, J., Belmont-Moreno, E., BenZvi, S. Y., Berley, D., ... Zhou, H. (2022). An Optimized Search for Dark Matter in the Galactic Halo with HAWC. Proceedings of Science, 395, Artículo 531.

@article{8032e35258414d3282c213f349cef0d5,

title = "An Optimized Search for Dark Matter in the Galactic Halo with HAWC",

abstract = "With a mass of approximately ∼1012 solar masses, the Galactic Halo is the closest known large dark matter halo and a prime candidate for indirect dark matter detection. The High Altitude Water Cherenkov Observatory (HAWC) is a high energy (300 GeV to 100 TeV) gamma ray detector located in central Mexico. HAWC operates via the water Cherenkov technique and has both a wide field of view of ∼2 sr and a >95% duty cycle, making it ideal for analysis of highly extended sources. We made use of these properties of HAWC and a new background-estimation technique optimized for extended sources to probe a large region of the Galactic Halo for dark matter signals. With this approach and taking into account electroweak corrections to the gamma-ray spectra, we set improved constraints on dark matter annihilation and decay between masses of 10 and 100 TeV. Our constraints also take into account detector simulation systematics and are robust against uncertainties in the Galactic dark matter spatial profile.",

author = "J. Lundeen and Harding, {J. P.} and Abeysekara, {A. U.} and A. Albert and R. Alfaro and C. Alvarez and {\'A}lvarez, {J. D.} and {Angeles Camacho}, {J. R.} and Arteaga-Vel{\'a}zquez, {J. C.} and Arunbabu, {K. P.} and {Avila Rojas}, D. and {Ayala Solares}, {H. A.} and R. Babu and V. Baghmanyan and Barber, {A. S.} and {Becerra Gonzalez}, J. and E. Belmont-Moreno and BenZvi, {S. Y.} and D. Berley and C. Brisbois and Caballero-Mora, {K. S.} and T. Capistr{\'a}n and A. Carrami{\~n}ana and S. Casanova and O. Chaparro-Amaro and U. Cotti and J. Cotzomi and {Couti{\~n}o de Le{\'o}n}, S. and {De la Fuente}, E. and {de Le{\'o}n}, C. and L. Diaz-Cruz and {Diaz Hernandez}, R. and D{\'i}az-V{\'e}lez, {J. C.} and Dingus, {B. L.} and M. Durocher and DuVernois, {M. A.} and Ellsworth, {R. W.} and K. Engel and C. Espinoza and Fan, {K. L.} and K. Fang and {Fern{\'a}ndez Alonso}, M. and B. Fick and H. Fleischhack and Flores, {J. L.} and Fraija, {N. I.} and D. Garcia and Garc{\'i}a-Gonz{\'a}lez, {J. A.} and Garc{\'i}a-Luna, {J. L.} and G. Garc{\'i}a-Torales and F. Garfias and G. Giacinti and H. Goksu and Gonz{\'a}lez, {M. M.} and Goodman, {J. A.} and S. Hernandez and I. Herzog and J. Hinton and B. Hona and D. Huang and F. Hueyotl-Zahuantitla and Hui, {C. M.} and B. Humensky and P. H{\"u}ntemeyer and A. Iriarte and A. Jardin-Blicq and H. Jhee and V. Joshi and D. Kieda and Kunde, {G. J.} and S. Kunwar and A. Lara and J. Lee and Lee, {W. H.} and D. Lennarz and {Le{\'o}n Vargas}, H. and J. Linnemann and Longinotti, {A. L.} and R. L{\'o}pez-Coto and G. Luis-Raya and J. Lundeen and K. Malone and V. Marandon and O. Martinez and I. Martinez-Castellanos and H. Mart{\'i}nez-Huerta and J. Mart{\'i}nez-Castro and Matthews, {J. A.J.} and J. McEnery and P. Miranda-Romagnoli and Morales-Soto, {J. A.} and E. Moreno and M. Mostaf{\'a} and A. Nayerhoda and L. Nellen and M. Newbold and Nisa, {M. U.} and R. Noriega-Papaqui and L. Olivera-Nieto and N. Omodei and A. Peisker and {P{\'e}rez Araujo}, Y. and P{\'e}rez-P{\'e}rez, {E. G.} and Rho, {C. D.} and C. Rivi{\`e}re and D. Rosa-Gonzalez and E. Ruiz-Velasco and J. Ryan and H. Salazar and {Salesa Greus}, F. and A. Sandoval and M. Schneider and H. Schoorlemmer and J. Serna-Franco and G. Sinnis and Smith, {A. J.} and Springer, {R. W.} and P. Surajbali and I. Taboada and M. Tanner and K. Tollefson and I. Torres and R. Torres-Escobedo and R. Turner and F. Ure{\~n}a-Mena and L. Villase{\~n}or and X. Wang and Watson, {I. J.} and T. Weisgarber and F. Werner and E. Willox and J. Wood and Yodh, {G. B.} and A. Zepeda and H. Zhou",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).; 37th International Cosmic Ray Conference, ICRC 2021 ; Conference date: 12-07-2021 Through 23-07-2021",

year = "2022",

month = mar,

day = "18",

language = "Ingl{\'e}s",

volume = "395",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

Lundeen, J, Harding, JP, Abeysekara, AU, Albert, A, Alfaro, R, Alvarez, C, Álvarez, JD, Angeles Camacho, JR, Arteaga-Velázquez, JC, Arunbabu, KP, Avila Rojas, D, Ayala Solares, HA, Babu, R, Baghmanyan, V, Barber, AS, Becerra Gonzalez, J, Belmont-Moreno, E, BenZvi, SY, Berley, D, Brisbois, C, Caballero-Mora, KS, Capistrán, T, Carramiñana, A, Casanova, S, Chaparro-Amaro, O, Cotti, U, Cotzomi, J, Coutiño de León, S, De la Fuente, E, de León, C, Diaz-Cruz, L, Diaz Hernandez, R, Díaz-Vélez, JC, Dingus, BL, Durocher, M, DuVernois, MA, Ellsworth, RW, Engel, K, Espinoza, C, Fan, KL, Fang, K, Fernández Alonso, M, Fick, B, Fleischhack, H, Flores, JL, Fraija, NI, Garcia, D, García-González, JA, García-Luna, JL, García-Torales, G, Garfias, F, Giacinti, G, Goksu, H, González, MM, Goodman, JA, Hernandez, S, Herzog, I, Hinton, J, Hona, B, Huang, D, Hueyotl-Zahuantitla, F, Hui, CM, Humensky, B, Hüntemeyer, P, Iriarte, A, Jardin-Blicq, A, Jhee, H, Joshi, V, Kieda, D, Kunde, GJ, Kunwar, S, Lara, A, Lee, J, Lee, WH, Lennarz, D, León Vargas, H, Linnemann, J, Longinotti, AL, López-Coto, R, Luis-Raya, G, Lundeen, J, Malone, K, Marandon, V, Martinez, O, Martinez-Castellanos, I, Martínez-Huerta, H, Martínez-Castro, J, Matthews, JAJ, McEnery, J, Miranda-Romagnoli, P, Morales-Soto, JA, Moreno, E, Mostafá, M, Nayerhoda, A, Nellen, L, Newbold, M, Nisa, MU, Noriega-Papaqui, R, Olivera-Nieto, L, Omodei, N, Peisker, A, Pérez Araujo, Y, Pérez-Pérez, EG, Rho, CD, Rivière, C, Rosa-Gonzalez, D, Ruiz-Velasco, E, Ryan, J, Salazar, H, Salesa Greus, F, Sandoval, A, Schneider, M, Schoorlemmer, H, Serna-Franco, J, Sinnis, G, Smith, AJ, Springer, RW, Surajbali, P, Taboada, I, Tanner, M, Tollefson, K, Torres, I, Torres-Escobedo, R, Turner, R, Ureña-Mena, F, Villaseñor, L, Wang, X, Watson, IJ, Weisgarber, T, Werner, F, Willox, E, Wood, J, Yodh, GB, Zepeda, A & Zhou, H 2022, 'An Optimized Search for Dark Matter in the Galactic Halo with HAWC', Proceedings of Science, vol. 395, 531.

TY - JOUR

T1 - An Optimized Search for Dark Matter in the Galactic Halo with HAWC

AU - Lundeen, J.

AU - Harding, J. P.

AU - Abeysekara, A. U.

AU - Albert, A.

AU - Alfaro, R.

AU - Alvarez, C.

AU - Álvarez, J. D.

AU - Angeles Camacho, J. R.

AU - Arteaga-Velázquez, J. C.

AU - Arunbabu, K. P.

AU - Avila Rojas, D.

AU - Ayala Solares, H. A.

AU - Babu, R.

AU - Baghmanyan, V.

AU - Barber, A. S.

AU - Becerra Gonzalez, J.

AU - Belmont-Moreno, E.

AU - BenZvi, S. Y.

AU - Berley, D.

AU - Brisbois, C.

AU - Caballero-Mora, K. S.

AU - Capistrán, T.

AU - Carramiñana, A.

AU - Casanova, S.

AU - Chaparro-Amaro, O.

AU - Cotti, U.

AU - Cotzomi, J.

AU - Coutiño de León, S.

AU - De la Fuente, E.

AU - de León, C.

AU - Diaz-Cruz, L.

AU - Diaz Hernandez, R.

AU - Díaz-Vélez, J. C.

AU - Dingus, B. L.

AU - Durocher, M.

AU - DuVernois, M. A.

AU - Ellsworth, R. W.

AU - Engel, K.

AU - Espinoza, C.

AU - Fan, K. L.

AU - Fang, K.

AU - Fernández Alonso, M.

AU - Fick, B.

AU - Fleischhack, H.

AU - Flores, J. L.

AU - Fraija, N. I.

AU - Garcia, D.

AU - García-González, J. A.

AU - García-Luna, J. L.

AU - García-Torales, G.

AU - Garfias, F.

AU - Giacinti, G.

AU - Goksu, H.

AU - González, M. M.

AU - Goodman, J. A.

AU - Hernandez, S.

AU - Herzog, I.

AU - Hinton, J.

AU - Hona, B.

AU - Huang, D.

AU - Hueyotl-Zahuantitla, F.

AU - Hui, C. M.

AU - Humensky, B.

AU - Hüntemeyer, P.

AU - Iriarte, A.

AU - Jardin-Blicq, A.

AU - Jhee, H.

AU - Joshi, V.

AU - Kieda, D.

AU - Kunde, G. J.

AU - Kunwar, S.

AU - Lara, A.

AU - Lee, J.

AU - Lee, W. H.

AU - Lennarz, D.

AU - León Vargas, H.

AU - Linnemann, J.

AU - Longinotti, A. L.

AU - López-Coto, R.

AU - Luis-Raya, G.

AU - Lundeen, J.

AU - Malone, K.

AU - Marandon, V.

AU - Martinez, O.

AU - Martinez-Castellanos, I.

AU - Martínez-Huerta, H.

AU - Martínez-Castro, J.

AU - Matthews, J. A.J.

AU - McEnery, J.

AU - Miranda-Romagnoli, P.

AU - Morales-Soto, J. A.

AU - Moreno, E.

AU - Mostafá, M.

AU - Nayerhoda, A.

AU - Nellen, L.

AU - Newbold, M.

AU - Nisa, M. U.

AU - Noriega-Papaqui, R.

AU - Olivera-Nieto, L.

AU - Omodei, N.

AU - Peisker, A.

AU - Pérez Araujo, Y.

AU - Pérez-Pérez, E. G.

AU - Rho, C. D.

AU - Rivière, C.

AU - Rosa-Gonzalez, D.

AU - Ruiz-Velasco, E.

AU - Ryan, J.

AU - Salazar, H.

AU - Salesa Greus, F.

AU - Sandoval, A.

AU - Schneider, M.

AU - Schoorlemmer, H.

AU - Serna-Franco, J.

AU - Sinnis, G.

AU - Smith, A. J.

AU - Springer, R. W.

AU - Surajbali, P.

AU - Taboada, I.

AU - Tanner, M.

AU - Tollefson, K.

AU - Torres, I.

AU - Torres-Escobedo, R.

AU - Turner, R.

AU - Ureña-Mena, F.

AU - Villaseñor, L.

AU - Wang, X.

AU - Watson, I. J.

AU - Weisgarber, T.

AU - Werner, F.

AU - Willox, E.

AU - Wood, J.

AU - Yodh, G. B.

AU - Zepeda, A.

AU - Zhou, H.

N1 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).

PY - 2022/3/18

Y1 - 2022/3/18

N2 - With a mass of approximately ∼1012 solar masses, the Galactic Halo is the closest known large dark matter halo and a prime candidate for indirect dark matter detection. The High Altitude Water Cherenkov Observatory (HAWC) is a high energy (300 GeV to 100 TeV) gamma ray detector located in central Mexico. HAWC operates via the water Cherenkov technique and has both a wide field of view of ∼2 sr and a >95% duty cycle, making it ideal for analysis of highly extended sources. We made use of these properties of HAWC and a new background-estimation technique optimized for extended sources to probe a large region of the Galactic Halo for dark matter signals. With this approach and taking into account electroweak corrections to the gamma-ray spectra, we set improved constraints on dark matter annihilation and decay between masses of 10 and 100 TeV. Our constraints also take into account detector simulation systematics and are robust against uncertainties in the Galactic dark matter spatial profile.

AB - With a mass of approximately ∼1012 solar masses, the Galactic Halo is the closest known large dark matter halo and a prime candidate for indirect dark matter detection. The High Altitude Water Cherenkov Observatory (HAWC) is a high energy (300 GeV to 100 TeV) gamma ray detector located in central Mexico. HAWC operates via the water Cherenkov technique and has both a wide field of view of ∼2 sr and a >95% duty cycle, making it ideal for analysis of highly extended sources. We made use of these properties of HAWC and a new background-estimation technique optimized for extended sources to probe a large region of the Galactic Halo for dark matter signals. With this approach and taking into account electroweak corrections to the gamma-ray spectra, we set improved constraints on dark matter annihilation and decay between masses of 10 and 100 TeV. Our constraints also take into account detector simulation systematics and are robust against uncertainties in the Galactic dark matter spatial profile.

UR - http://www.scopus.com/inward/record.url?scp=85144611824&partnerID=8YFLogxK

M3 - Artículo de la conferencia

AN - SCOPUS:85144611824

SN - 1824-8039

VL - 395

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 531

T2 - 37th International Cosmic Ray Conference, ICRC 2021

Y2 - 12 July 2021 through 23 July 2021

ER -

An Optimized Search for Dark Matter in the Galactic Halo with HAWC

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