Built on

J. Dormand and P. Prince, “A family of embedded Runge-Kutta formulae,” J. Comp. Appl. Math
1980
Earlier work this paper cites.
B. Holdom, “Two U(1)’s and Epsilon Charge Shifts,” Phys. Lett
1986
Earlier work this paper cites.
J. Miralda-Escudé, “A Test of the Collisional Dark Matter Hypothesis from Cluster Lensing,” Astrophys. J
2002
Earlier work this paper cites.
D. Javorsek, D. Elmore, E. Fischbach, D. Granger, T. Miller, D. Oliver, and V. Teplitz, “Search for anomalously heavy nuclei in gold and iron,” Phys. Rev. D
2002
Earlier work this paper cites.
K. Sigurdson, M. Doran, A. Kurylov, R. R. Caldwell, and M. Kamionkowski, “Dark-matter electric and magnetic dipole moments,” Phys.Rev
2004
Earlier work this paper cites.
International Union of Crystallography, 1st ed., 2006
P. J. Brown, A. G. Fox, E. N. Maslen, M. A. O’Keefe, and B. T. M. Willis, International Tables for Crystallography · 2006
Earlier work this paper cites.
D. Feldman, Z. Liu, and P. Nath, “The Stueckelberg Z-prime Extension with Kinetic Mixing and Milli-Charged Dark Matter From the Hidden Sector,” Phys.Rev
2007
Earlier work this paper cites.
M. Y. Khlopov, A. G. Mayorov, and E. Y. Soldatov, “The dark atoms of dark matter,” Prespacetime. J
Original
2010
Earlier work this paper cites.

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2014

Dark antiatoms can explain DAMA

Wallemacq, Quentin, Cudell, Jean-René

Understand

We show that the existence of a sub-dominant form of dark matter, made of dark antiatoms of mass and size of the order of 1 TeV and 30 fm respectively, can explain the results of direct detection experiments, with a positive signal in DAMA/NaI and DAMA/LIBRA and no signal in other experiments.

The signal comes from the binding of the dark antiatoms to thallium, a dopant in DAMA, and is not present for the constituent atoms of other experiments.
The dark antiatoms are made of two particles oppositely charged under a dark U(1) symmetry and can bind to terrestrial atoms because of a kinetic mixing between the photon and the massless dark photon, such that the dark particles acquire an electric millicharge of the order of 0.0005e.
This millicharge enables them to bind to high-Z atoms via radiative capture, after they thermalize in terrestrial matter through elastic collisions.

Built on

J. Dormand and P. Prince, “A family of embedded Runge-Kutta formulae,” J. Comp. Appl. Math
1980
Earlier work this paper cites.
B. Holdom, “Two U(1)’s and Epsilon Charge Shifts,” Phys. Lett
1986
Earlier work this paper cites.
J. Miralda-Escudé, “A Test of the Collisional Dark Matter Hypothesis from Cluster Lensing,” Astrophys. J
2002
Earlier work this paper cites.
D. Javorsek, D. Elmore, E. Fischbach, D. Granger, T. Miller, D. Oliver, and V. Teplitz, “Search for anomalously heavy nuclei in gold and iron,” Phys. Rev. D
2002
Earlier work this paper cites.
K. Sigurdson, M. Doran, A. Kurylov, R. R. Caldwell, and M. Kamionkowski, “Dark-matter electric and magnetic dipole moments,” Phys.Rev
2004
Earlier work this paper cites.
International Union of Crystallography, 1st ed., 2006
P. J. Brown, A. G. Fox, E. N. Maslen, M. A. O’Keefe, and B. T. M. Willis, International Tables for Crystallography · 2006
Earlier work this paper cites.
D. Feldman, Z. Liu, and P. Nath, “The Stueckelberg Z-prime Extension with Kinetic Mixing and Milli-Charged Dark Matter From the Hidden Sector,” Phys.Rev
2007
Earlier work this paper cites.
M. Y. Khlopov, A. G. Mayorov, and E. Y. Soldatov, “The dark atoms of dark matter,” Prespacetime. J
Original
2010
Earlier work this paper cites.