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2013

Direct Detection with Dark Mediators

Curtin, David, Surujon, Ze'ev, Tsai, Yuhsin

Understand

We introduce dark mediator Dark matter (dmDM) where the dark and visible sectors are connected by at least one light mediator $\phi$ carrying the same dark charge that stabilizes DM.

$\phi$ is coupled to the Standard Model via an operator $\bar q q \phi \phi^*/\Lambda$, and to dark matter via a Yukawa coupling $y_\chi \overline{\chi^c}\chi \phi$.
Direct detection is realized as the $2\rightarrow3$ process $\chi N \rightarrow \bar \chi N \phi$ at tree-level for $m_\phi \lesssim 10 \ \mathrm{keV}$ and small Yukawa coupling, or alternatively as a loop-induced $2\rightarrow2$ process $\chi N \rightarrow \chi N$.
We explore the direct-detection consequences of this scenario and find that a heavy $\mathcal{O}(100 \ \mathrm{GeV})$ dmDM candidate fakes different $\mathcal{O}(10 \ \mathrm{GeV})$ standard WIMPs in different experiments.

Built on

M. W. Goodman and E. Witten, Phys. Rev. D 31
1985
Earlier work this paper cites.
E. W. Kolb and M. S. Turner, Front. Phys. 69
1990
Earlier work this paper cites.
R. J. Barlow, Nucl. Instrum. Meth. A 297
Original
1990
Earlier work this paper cites.
J. Engel, Phys. Lett. B 264
1991
Earlier work this paper cites.
E. D. Carlson, M. E. Machacek and L. J. Hall, Astrophys. J. 398
1992
Earlier work this paper cites.
J. D. Lewin and P. F. Smith, Astropart. Phys. 6
1996
Earlier work this paper cites.
D. N. Spergel and P. J. Steinhardt, Phys. Rev. Lett. 84
2000
Earlier work this paper cites.
D. Tucker-Smith and N. Weiner, Phys. Rev. D 64
2001
Earlier work this paper cites.
See, for example, G. Jungman, M. Kamionkowski and K. Griest, Phys. Rept. 267
2005
Earlier work this paper cites.
M. C. Smith, G. R. Ruchti, A. Helmi, R. F. G. Wyse, J. P. Fulbright, K. C. Freeman, J. F. Navarro and G. M. Seabroke et al
2007
Earlier work this paper cites.
G. G. Raffelt, Lect. Notes Phys. 741
2008
Earlier work this paper cites.
Y. Bai and P. J. Fox, JHEP 0911
Original
2009
Earlier work this paper cites.