Built on

S. Baum, N. R. Shah and K. Freese, JHEP 04
Original
1901
Earlier work this paper cites.
J. Cao, Y. He, Y. Pan, Y. Yue, H. Zhou and P. Zhu, Impact of leptonic unitarity and dark matter direct detection experiments on the NMSSM with inverse seesaw mechanism , JHEP 2012
Original
1903
Earlier work this paper cites.
W. Abdallah, A. Chatterjee and A. Datta, Revisiting singlino dark matter of the natural Z 3 Z_{3} -symmetric NMSSM in the light of LHC , JHEP 1909
Original
1907
Earlier work this paper cites.
G. Aad et al
Original
1908
Earlier work this paper cites.
J. Cao, L. Meng, Y. Yue, H. Zhou and P. Zhu, Suppressing the scattering of wimp dark matter and nucleons in supersymmetric theories , Phys. Rev. D 101
Original
1910
Earlier work this paper cites.
G. Aad et al
Original
1911
Earlier work this paper cites.
G. Aad et al
Original
1912
Earlier work this paper cites.
H. Jeffreys (1961). The Theory of Probability (3rd ed.). Oxford. p. 432
1961
Earlier work this paper cites.
K. Griest, M. Kamionkowski and M. S. Turner, Supersymmetric Dark Matter Above the W Mass Phys. Rev. D 41
1990
Earlier work this paper cites.
K. Griest and D. Seckel, Three exceptions in the calculation of relic abundances , Physical Review D 43
1991
Earlier work this paper cites.
M. Drees and M. Nojiri, Neutralino - nucleon scattering revisited , Phys. Rev. D 48
1993
Earlier work this paper cites.
M. Drees and M. M. Nojiri, New contributions to coherent neutralino - nucleus scattering , Phys. Rev. D 47
1993
Earlier work this paper cites.
G. Jungman, M. Kamionkowski and K. Griest, Supersymmetric dark matter , Physics Reports 333
1995
Earlier work this paper cites.
G. Aad et al
Original
2002
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov and A. Semenov, MicrOMEGAs: A Program for calculating the relic density in the MSSM , Comput. Phys. Commun. 149
2002
Earlier work this paper cites.
W. Porod, SPheno, a program for calculating supersymmetric spectra, SUSY particle decays and SUSY particle production at e+ e- colliders , Comput. Phys. Commun. 153
2003
Earlier work this paper cites.
G. Bertone, D. Hooper and J. Silk, Particle dark matter: Evidence, candidates and constraints , Phys. Rept. 405
2004
Earlier work this paper cites.
D. J. Miller, R. Nevzorov and P. M. Zerwas, The higgs sector of the next-to-minimal supersymmetric standard model , Nuclear Physics B 681
Original
2004
Earlier work this paper cites.
W. G. Hollik, C. Li, G. Moortgat-Pick and S. Paasch, Phenomenology of a Supersymmetric Model Inspired by Inflation , arXiv:2004.14852 [hep-ph]
Original
2004
Earlier work this paper cites.
M. Guchait and A. Roy, Phys. Rev. D 102
Original
2005
Earlier work this paper cites.
G. Belanger, F. Boudjema, C. Hugonie, A. Pukhov and A. Semenov, Relic density of dark matter in the NMSSM , JCAP 09
2005
Earlier work this paper cites.
P. Gregory, Bayesian Logical Data Analysis for the Physical Sciences. Cambridge University Press, 2005
2005
Earlier work this paper cites.
T. Sjostrand, S. Mrenna and P. Z. Skands, PYTHIA 6.4 Physics and Manual , JHEP 0605
2006
Earlier work this paper cites.
Q. Wang et al
Original
2007
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov and A. Semenov, MicrOMEGAs 2.0: A Program to calculate the relic density of dark matter in a generic model , Comput. Phys. Commun. 176
2007
Earlier work this paper cites.
M. Pospelov, A. Ritz and M. B. Voloshin, Secluded WIMP Dark Matter , Phys. Lett. B 662
Original
2008
Earlier work this paper cites.

Similar

F. Feroz, B. C. Allanach, M. Hobson, S. S. AbdusSalam, R. Trotta and A. M. Weber, Bayesian Selection of sign(mu) within mSUGRA in Global Fits Including WMAP5 Results , JHEP 0810
Original
2008
Cited alongside, same era.
G. Bélanger, F. Boudjema, A. Pukhov and A. Semenov, Dark matter direct detection rate in a generic model with micromegas2.2 , Computer Physics Communications 180
2009
Cited alongside, same era.
F. Feroz, M. P. Hobson and M. Bridges, MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics , Mon. Not. Roy. Astron. Soc. 398
Original
2009
Cited alongside, same era.
U. Ellwanger, C. Hugonie and A. M. Teixeira, The Next-to-Minimal Supersymmetric Standard Model , Phys. Rept. 496
Original
2010
Cited alongside, same era.
G. Belanger, F. Boudjema, A. Pukhov and A. Semenov, micromegas : a tool for dark matter studies , 2010, arXiv:1005.4133 [hep-ph]

Then

M. J. Baker et al
Original
2015
Later among the works it cites.
M. Ackermann et al
Original
2015
Later among the works it cites.
P. Bechtle, S. Heinemeyer, O. Stal, T. Stefaniak and G. Weiglein, Applying Exclusion Likelihoods from LHC Searches to Extended Higgs Sectors , Eur. Phys. J. C 75
Original
2015
Later among the works it cites.
F. Staub, Exploring new models in all detail with sarah , Advances in High Energy Physics (2015) , arXiv:1503.04200 [hep-ph]
Original
2015
Later among the works it cites.
J. S. Kim, D. Schmeier, J. Tattersall and K. Rolbiecki, A framework to create customised LHC analyses within CheckMATE , Comput. Phys. Commun. 196
Original

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2021

Singlino-dominated dark matter in general NMSSM

Cao, Junjie, Li, Demin, Lian, Jingwei et al.

Understand

The general Next-to-Minimal Supersymmetric Standard Model (NMSSM) describes the singlino-dominated dark-matter (DM) property by four independent parameters: singlet-doublet Higgs coupling coefficient $\lambda$, Higgsino mass $\mu_{tot}$, DM mass $m_{\tilde{\chi}_1^0}$, and singlet Higgs self-coupling coefficient $\kappa$.

The first three parameters strongly influence the DM-nucleon scattering rate, while $\kappa$ usually affects the scattering only slightly.
This characteristic implies that singlet-dominated particles may form a secluded DM sector.
Under such a theoretical structure, the DM achieves the correct abundance by annihilating into a pair of singlet-dominated Higgs bosons by adjusting $\kappa$'s value.