Built on

P. Ullio and L. Bergström, Phys. Rev. D 57
1962
Earlier work this paper cites.
A. Zee, Phys. Lett. B 93
1980
Earlier work this paper cites.
H. Goldberg, Phys. Rev. Lett. 50
1983
Earlier work this paper cites.
L. Bergström and G. Hulth, Nucl. Phys. B 259
1986
Earlier work this paper cites.
L. Bergström, Phys. Lett. B225
1989
Earlier work this paper cites.
S. Aminneborg, L. Bergström and B. A. Lindholm, Phys. Rev. D 43
1991
Earlier work this paper cites.
L. Bergström and J. Kaplan, Astropart. Phys. 2
1994
Earlier work this paper cites.
L. Bergström and P. Ullio, Nucl. Phys. B 504
1997
Earlier work this paper cites.
Z. Bern, P. Gondolo and M. Perelstein, Phys. Lett. B 411
1997
Earlier work this paper cites.
L. Bergström and H. Snellman, Phys. Rev. D 37
1998
Earlier work this paper cites.
A. Djouadi, J. Kalinowski and M. Spira, Comput. Phys. Commun. 108
1998
Earlier work this paper cites.
E. Dudas, Y. Mambrini, S. Pokorski and A. Romagnoni, arXiv:1205.1520 [hep-ph]; J. M. Cline, arXiv:1205.2688 [hep-ph]; K. -Y. Choi and O. Seto, arXiv:1205.3276 [hep-ph]; B. Kyae and J. -C. Park, arXiv:1205.4151 [hep-ph]; H. M. Lee, M. Park and W. -I. Park, arXiv:1205.4675 [hep-ph]; B. S. Acharya, G. Kane, P. Kumar, R. Lu and B. Zheng, arXiv:1205.5789 [hep-ph]; M. R. Buckley and D. Hooper, arXiv:1205.6811 [hep-ph]; X. Chu, T. Hambye, T. Scarna and M. H. G. Tytgat, arXiv:1206.2279 [hep-ph]; D. Das, U. Ellwanger and P. Mitropoulos, arXiv:1206.2639 [hep-ph]; N. Weiner and I. Yavin, arXiv:1206.2910 [hep-ph]; J. H. Heo and C. S. Kim, arXiv:1207.1341 [astro-ph.HE]; I. Oda, arXiv:1207.1537 [hep-ph]; K. Cheung, Y. -L. S. Tsai, P. -Y. Tseng, T. -C. Yuan and A. Zee, arXiv:1207.4930 [hep-ph]; J. -C. Park and S. C. Park, arXiv:1207.4981 [hep-ph]; S. Tulin, H. -B. Yu and K. M. Zurek, arXiv:1208.0009 [hep-ph]; T. Li, J. A. Maxin, D. V. Nanopoulos and J. W. Walker, arXiv:1208.1999 [hep-ph]; J. M. Cline, A. R. Frey and G. D. Moore, arXiv:1208.2685 [hep-ph]; Y. Bai and J. Shelton, arXiv:1208.4100 [hep-ph]
Original
1999
Earlier work this paper cites.
A. Czarnecki and W. J. Marciano, Phys. Rev. D 64
2001
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2006
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2012

The 130 GeV Fingerprint of Right-Handed Neutrino Dark Matter

Bergström, Lars

Understand

Recently, an interesting indication for a dark matter signal in the form of a narrow line, or maybe two lines and/or an internal bremsstrahlung feature, has been found in data from the Fermi-LAT satellite detector.

As recent analyses have also shown that there is little sign of extra contributions to continuum photons, it is natural to investigate leptophilic interacting massive particle (LIMP) models.
We show that a model of radiatively generated neutrino masses may have the properties needed to explain the Fermi-LAT structure around 130 GeV.
This model was proposed some 10 years ago, and predicted a clearly observable $\gamma$-ray signal in the Fermi-LAT (then GLAST) detector.

Built on

P. Ullio and L. Bergström, Phys. Rev. D 57
1962
Earlier work this paper cites.
A. Zee, Phys. Lett. B 93
1980
Earlier work this paper cites.
H. Goldberg, Phys. Rev. Lett. 50
1983
Earlier work this paper cites.
L. Bergström and G. Hulth, Nucl. Phys. B 259
1986
Earlier work this paper cites.
L. Bergström, Phys. Lett. B225
1989
Earlier work this paper cites.
S. Aminneborg, L. Bergström and B. A. Lindholm, Phys. Rev. D 43
1991
Earlier work this paper cites.
L. Bergström and J. Kaplan, Astropart. Phys. 2
1994
Earlier work this paper cites.
L. Bergström and P. Ullio, Nucl. Phys. B 504
1997
Earlier work this paper cites.
Z. Bern, P. Gondolo and M. Perelstein, Phys. Lett. B 411
1997
Earlier work this paper cites.
L. Bergström and H. Snellman, Phys. Rev. D 37
1998
Earlier work this paper cites.
A. Djouadi, J. Kalinowski and M. Spira, Comput. Phys. Commun. 108
1998
Earlier work this paper cites.
E. Dudas, Y. Mambrini, S. Pokorski and A. Romagnoni, arXiv:1205.1520 [hep-ph]; J. M. Cline, arXiv:1205.2688 [hep-ph]; K. -Y. Choi and O. Seto, arXiv:1205.3276 [hep-ph]; B. Kyae and J. -C. Park, arXiv:1205.4151 [hep-ph]; H. M. Lee, M. Park and W. -I. Park, arXiv:1205.4675 [hep-ph]; B. S. Acharya, G. Kane, P. Kumar, R. Lu and B. Zheng, arXiv:1205.5789 [hep-ph]; M. R. Buckley and D. Hooper, arXiv:1205.6811 [hep-ph]; X. Chu, T. Hambye, T. Scarna and M. H. G. Tytgat, arXiv:1206.2279 [hep-ph]; D. Das, U. Ellwanger and P. Mitropoulos, arXiv:1206.2639 [hep-ph]; N. Weiner and I. Yavin, arXiv:1206.2910 [hep-ph]; J. H. Heo and C. S. Kim, arXiv:1207.1341 [astro-ph.HE]; I. Oda, arXiv:1207.1537 [hep-ph]; K. Cheung, Y. -L. S. Tsai, P. -Y. Tseng, T. -C. Yuan and A. Zee, arXiv:1207.4930 [hep-ph]; J. -C. Park and S. C. Park, arXiv:1207.4981 [hep-ph]; S. Tulin, H. -B. Yu and K. M. Zurek, arXiv:1208.0009 [hep-ph]; T. Li, J. A. Maxin, D. V. Nanopoulos and J. W. Walker, arXiv:1208.1999 [hep-ph]; J. M. Cline, A. R. Frey and G. D. Moore, arXiv:1208.2685 [hep-ph]; Y. Bai and J. Shelton, arXiv:1208.4100 [hep-ph]
Original
1999
Earlier work this paper cites.
A. Czarnecki and W. J. Marciano, Phys. Rev. D 64
2001
Earlier work this paper cites.

Similar

L. M. Krauss, S. Nasri and M. Trodden, Phys. Rev. D 67
2003
Cited alongside, same era.
E. A. Baltz and L. Bergström, Phys. Rev. D 67
2003
Cited alongside, same era.
K. Cheung and O. Seto, Phys. Rev. D 69
2004
Cited alongside, same era.
P. Gondolo, J. Edsjö, P. Ullio, L. Bergström, M. Schelke and E. A. Baltz, JCAP 0407
2004
Cited alongside, same era.
F. Boudjema, A. Semenov and D. Temes, Phys. Rev. D 72
2005
Cited alongside, same era.
J. Hisano, M. Nagai, M. M. Nojiri and M. Senami, AIP Conf. Proc. 805
2006
Cited alongside, same era.
G. W. Bennett et al
2006