Fetching the paper…
Reading the bibliography…
Bosonic superweakly interacting massive particles (super-WIMPs) are a candidate for warm dark matter.
S. Fukuda et al
2003
Earlier work this paper cites.
R. Bernabei et al
2006
Earlier work this paper cites.
S. Nakamura et al
2007
Earlier work this paper cites.
M. Pospelov, A. Ritz, and M. Voloshin, Phys. Rev. D 78,
2008
Earlier work this paper cites.
C. E. Aalseth et al
2008
Earlier work this paper cites.
J. Redondo, M. Postma, J. Cosm. Astropart. Phys., 02,
2009
Cited alongside, same era.
Z. Ahmed et al
2009
Cited alongside, same era.
J. Beringer et al
2012
Cited alongside, same era.
K. Abe et al
2013
Cited alongside, same era.
K. Abe et al
2013
Cited alongside, same era.
This photoelectron yield is smaller than the value reported in Ref. [ 5 , 8 , 11 ] since we changed a correction on the charge observed in the electronics. This correction is within the uncertainty reported earlier, ± 1.2 \pm 1.2 p.e./keV
Cited in the paper.
Cited in the paper.
K. Abe et al
2013
Later among the works it cites.
E. Armengaud et al
2013
Later among the works it cites.
R. Horvat, D. Kekez, M. Krčmar, Z. Krečak, A. Ljubičić, Phys. Lett. B 721,
2013
Later among the works it cites.
K. Markovič and M. Viel, Publ. Astron. Soc. of Aust., 31
2014
Closest in time.
H. Uchida et al
2014
Closest in time.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…