Fetching the paper…

Reading the bibliography…

2017

Confronting the DAMPE Excess with the Scotogenic Type-II Seesaw Model

Ding, Ran, Han, Zhi-Long, Feng, Lei et al.

Original
PDF
Post on X

Understand

The DArk Matter Particle Explorer (DAMPE) has observed a tentative peak at $E\sim1.4~\TeV$ in the cosmic-ray electron spectrum.

In this paper, we interpret this excess in the scotogenic type-II seesaw model.
This model extends the canonical type-II seesaw model with dark matter (DM) candidates and a loop-induced vacuum expectation value of the triplet scalars, $v_\Delta$, resulting in small neutrino masses naturally even for TeV scale triplet scalars.
Assuming a nearby DM subhalo, the DAMPE excess can be explained by DM annihilating into a pair of triplet scalars which subsequently decay to charged lepton final states.

Confronting the DAMPE Excess with the Scotogenic Type-II Seesaw Model · Around

Built on

A. Alloul, N. D. Christensen, C. Degrande, C. Duhr and B. Fuks, Comput. Phys. Commun. 185
Original
1921
Earlier work this paper cites.
A. Arhrib, R. Benbrik, M. Chabab, G. Moultaka, M. C. Peyranere, L. Rahili and J. Ramadan, Phys. Rev. D 84
Original
1925
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk and S. D. M. White, Astrophys. J. 462
1996
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk and S. D. M. White, Astrophys. J. 490
1997
Earlier work this paper cites.
A. W. Strong and I. V. Moskalenko, Astrophys. J. 509
1998
Earlier work this paper cites.
I. V. Moskalenko and A. W. Strong, Astrophys. J. 493
1998
Earlier work this paper cites.
P. Fileviez Perez, T. Han, G. y. Huang, T. Li and K. Wang, Phys. Rev. D 78
Original
2008
Earlier work this paper cites.
F. Aharonian et al
Original
2009
Earlier work this paper cites.
I. Gogoladze, N. Okada and Q. Shafi, Phys. Lett. B 679
Original
2009
Earlier work this paper cites.
A. G. Akeroyd, M. Aoki and H. Sugiyama, Phys. Rev. D 79
Original
2010
Earlier work this paper cites.
S. Kanemura and H. Sugiyama, Phys. Rev. D 86
Original
2012
Earlier work this paper cites.
A. Melfo, M. Nemevsek, F. Nesti, G. Senjanovic and Y. Zhang, Phys. Rev. D 85
Original
2012
Earlier work this paper cites.
M. Cirelli et al
Original
2012
Earlier work this paper cites.
Y. Bai and J. Berger, JHEP 1408
Original
2014
Earlier work this paper cites.

Similar

P. S. B. Dev, D. K. Ghosh, N. Okada and I. Saha, Phys. Rev. D 89
Original
2014
Cited alongside, same era.
C. H. Chen and T. Nomura, JHEP 1409
Original
2014
Cited alongside, same era.
J. Alwall et al
Original
2014
Cited alongside, same era.
M. Aguilar et al
2014
Cited alongside, same era.
C. H. Chen, C. W. Chiang and T. Nomura, Phys. Lett. B 747
Original
2015
Cited alongside, same era.
E. Ma, Phys. Rev. Lett. 115

Then

S. Y. Guo, Z. L. Han and Y. Liao, Phys. Rev. D 94
Original
2016
Later among the works it cites.
W. Wang and Z. L. Han, Phys. Rev. D 94
Original
2016
Later among the works it cites.
C. Patrignani et al
2016
Later among the works it cites.
P. A. R. Ade et al
Original
2016
Later among the works it cites.
I. Esteban, M. C. Gonzalez-Garcia, M. Maltoni, I. Martinez-Soler and T. Schwetz, JHEP 1701
Original
2017
Closest in time.
D. S. Akerib et al

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

2015

Cited alongside, same era.

C. Bonilla, J. W. F. Valle and J. C. Romao, Phys. Rev. D 91

2015

Cited alongside, same era.

W. Wang and Z. L. Han, Phys. Rev. D 92

2015

Cited alongside, same era.

Z. L. Han, R. Ding and Y. Liao, Phys. Rev. D 91

2015

Cited alongside, same era.

Z. L. Han, R. Ding and Y. Liao, Phys. Rev. D 92

2015

Cited alongside, same era.

M. Aaboud et al

2015

Cited alongside, same era.

G. B¨¦langer, F. Boudjema, A. Pukhov and A. Semenov, Comput. Phys. Commun. 192

2015

Cited alongside, same era.

2017

Closest in time.

E. Aprile et al

2017

Closest in time.

2017

Closest in time.

M. G. Aartsen et al

2017

Closest in time.

S. Abdollahi et al

2017

Closest in time.

A. Fowlie, Phys. Lett. B 780

2018

Closest in time.

Y. Z. Fan, W. C. Huang, M. Spinrath, Y. L. S. Tsai and Q. Yuan, Phys. Lett. B 781

2018

Closest in time.

T. Li, N. Okada and Q. Shafi, Phys. Lett. B 779

2018

Closest in time.