Built on

P. Padovani, F. Oikonomou, M. Petropoulou, P. Giommi, and E. Resconi, Mon. Not. R. Astron. Soc.: Letters 484
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L. Maraschi, G. Ghisellini, and A. Celotti, Astrophys. J. 397
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2021

Direct Detection Constraints on Blazar-Boosted Dark Matter

Wang, Jin-Wei, Granelli, Alessandro, Ullio, Piero

Understand

We explore the possibility that relativistic protons in the extremely powerful jets of blazars may boost via elastic collisions the dark matter particles in the surroundings of the source to high energies.

We concentrate on two sample blazars, TXS 0506+056 - towards which IceCube recently reported evidence for a high-energy neutrino flux - and BL Lacertae, a representative nearby blazar.
We find that the dark matter flux at Earth induced by these sources may be sizable, larger than the flux associated with the analogous process of dark matter boosted by galactic cosmic rays, and relevant to access direct detection for dark matter particle masses lighter than 1 GeV.
From the null detection of a signal by XENON1T, MiniBooNE, and Borexino, we derive limits on dark matter-nucleus spin-independent and spin-dependent cross sections which, depending on the modelization of the source, improve on other currently available bounds for light dark matter candidates of 1 up to 5 orders of magnitude.

Built on

P. Padovani, F. Oikonomou, M. Petropoulou, P. Giommi, and E. Resconi, Mon. Not. R. Astron. Soc.: Letters 484
Original
1901
Earlier work this paper cites.
R. Xue, R.-Y. Liu, M. Petropoulou, F. Oikonomou, Z.-R. Wang, K. Wang, and X.-Y. Wang, Astrophys. J. 886
Original
1908
Earlier work this paper cites.
M. Petropoulou, K. Murase, M. Santander, S. Buson, A. Tohuvavohu, T. Kawamuro, G. Vasilopoulos, H. Negoro, Y. Ueda, M. H. Siegel, A. Keivani, N. Kawai, A. Mastichiadis and S. Dimitrakoudis, Astrophys. J. 891
Original
1911
Earlier work this paper cites.
N. S. Kardashev, Sov. Astron. 6
1962
Earlier work this paper cites.
J. B. Oke and J. E. Gunn, Astrophys. J. 189
1974
Earlier work this paper cites.
G. D. Starkman, A. Gould, R. Esmailzadeh, and S. Dimopoulos, Phys. Rev. D 41
1990
Earlier work this paper cites.
L. Maraschi, G. Ghisellini, and A. Celotti, Astrophys. J. 397
1992
Earlier work this paper cites.
K. Mannheim, Astron. Astrophys. 269
1993
Earlier work this paper cites.
C. M. Urry and P. Padovani, Publ. Astron. Soc. Pac. 107
1995
Earlier work this paper cites.
S. D. Bloom and A. P. Marscher, Astrophys. J. 461
1996
Earlier work this paper cites.
E. D. Bloom and J. D. Wells, Phys. Rev. D 57
1998
Earlier work this paper cites.
P. Gondolo and J. Silk, Phys. Rev. Lett. 83
1999
Earlier work this paper cites.
A. Mücke and R. Protheroe, Astropart. Phys. 15
2001
Earlier work this paper cites.
P. Ullio, H. S. Zhao, and M. Kamionkowski, Phys. Rev. D 64
2001
Earlier work this paper cites.
G. Alimonti et al. (Borexino Collaboration), Astropart. Phys. 16
2002
Earlier work this paper cites.
J. F. Beacom, W. M. Farr, and P. Vogel, Phys. Rev. D 66
2002
Earlier work this paper cites.
I. Angeli, At. Data Nucl. Data Tables 87
2004
Earlier work this paper cites.
G. Bertone, D. Hooper, and J. Silk, Phys. Rep. 405
2005
Earlier work this paper cites.
G. D. Mack, J. F. Beacom, and G. Bertone, Phys. Rev. D 76
Original
2007
Earlier work this paper cites.
A. Celotti and G. Ghisellini, Mon. Not. R. Astron. Soc. 385
Original
2008
Earlier work this paper cites.