Fetching the paper…
Reading the bibliography…
Recently, the DAMA/LIBRA experiment has convincingly confirmed the DAMA/NaI annual modulation signal, experimentally demonstrating the existence of non-baryonic dark matter in the halo of our galaxy.
R. H, Helm, Phys. Rev. 104, 1466 (1956)
1956
Earlier work this paper cites.
R. Foot, H. Lew and R. R. Volkas, Phys. Lett. B272, 67 (1991). The idea of a mirror sector was discussed, prior to the advent of the standard model, in: T. D. Lee and C. N. Yang, Phys. Rev. 104, 256 (1956); I. Kobzarev, L. Okun and I. Pomeranchuk, Sov. J. Nucl. Phys. 3, 837 (1966). The idea that the mirror particles might be the dark matter was first discussed in: S. I. Blinnikov and M. Yu. Khlopov, Sov. J. Nucl. Phys. 36, 472 (1982); Sov. Astron. 27, 371 (1983)
1983
Earlier work this paper cites.
B. Holdom, Phys. Lett. B166, 196 (1986)
1986
Earlier work this paper cites.
E. D. Carlson and S. L. Glashow, Phys. Lett. B193, 168 (1987)
1987
Earlier work this paper cites.
A. K. Drukier, K. Freese and D. N. Spergel, Phys. Rev. D33, 3495 (1986); K. Freese, J. A. Frieman and A. Gould, Phys. Rev. D37, 3388 (1988)
1988
Earlier work this paper cites.
R. Foot and X-G. He, Phys. Lett. B267, 509 (1991)
1991
Earlier work this paper cites.
R. Foot, H. Lew and R. R. Volkas, Mod. Phys. Lett. A7, 2567 (1992); R. Foot, Mod. Phys. Lett. A9, 169 (1994) [hep-ph/9402241]; R. Foot and R. R. Volkas, Phys. Rev. D52, 6595 (1995) [hep-ph/9505359]
1995
Earlier work this paper cites.
E. W. Kolb, D. Seckel and M. S. Turner, Nature 314, 415 (1985); H. Hodges, Phys. Rev. D47, 456 (1993); Z. G. Berezhiani, A. D. Dolgov and R. N. Mohapatra, Phys. Lett. B375, 26 (1996) [hep-ph/9511221]
1996
Earlier work this paper cites.
J. D. Lewin and P. F. Smith, Astropart. Phys. 6, 87 (1996)
1996
Earlier work this paper cites.
C. S. Kochanek, Astrophys. J. 457, 228 (1996)
1996
Earlier work this paper cites.
See e.g. Z. Silagadze, Phys. Atom. Nucl. 60, 272 (1997) [hep-ph/9503481]
1997
Earlier work this paper cites.
Z. Berezhiani, D. Comelli and F. L. Villante, Phys. Lett. B503, 362 (2001) [hep-ph/0008105]
2001
Earlier work this paper cites.
L. Bento and Z. Berezhiani, Phys. Rev. Lett. 87, 231304 (2001) [hep-ph/0107281]; hep-ph/0111116
2001
Earlier work this paper cites.
R. Foot, A. Yu. Ignatiev and R. R. Volkas, Phys. Lett. B503, 355 (2001) [astro-ph/0011156]
2001
Cited alongside, same era.
G. Angloher it et al. (CRESST Collaboration), Astroparticle Phys. 18, 43 (2002)
2002
Cited alongside, same era.
A. Yu. Ignatiev and R. R. Volkas, Phys. Rev. D68, 023518 (2003) [hep-ph/0304260]
2003
Cited alongside, same era.
R. Foot and S. Mitra, Astropart. Phys. 19, 739 (2003) [astro-ph/0211067]; Phys. Lett. B558, 9 (2003) [hep-ph/0303005]; Phys. Lett. A315, 178 (2003) [cond-mat/0306561]
2003
Cited alongside, same era.
R. Bernabei et al. (DAMA Collaboration), Phys. Lett. B480, 23 (2000); Riv. Nuovo Cimento. 26, 1 (2003) [astro-ph/0307403]; Int. J. Mod. Phys. D13, 2127 (2004) and references there-in
2004
Cited alongside, same era.
Z. Berezhiani, P. Ciarcelluti, D. Comelli and F. L. Villante, Int. J. Mod. Phys. D14, 107 (2005) [astro-ph/0312605]; P. Ciarcelluti, Int. J. Mod. Phys. D14, 187 (2005) [astro-ph/0409630]; Int. J. Mod. Phys. D14, 223 (2005) [astro-ph/0409633]
2005
Later among the works it cites.
R. Foot and Z. K. Silagadze, Int. J. Mod. Phys. D14, 143 (2005) [astro-ph/0404515]
2005
Later among the works it cites.
D. S. Akerib et al
2006
Later among the works it cites.
R. Bernabei et al
2006
Later among the works it cites.
R. Foot, Phys. Rev. D74, 023514 (2006) [arXiv: astro-ph/0510705]
2006
Later among the works it cites.
Z. Berezhiani, P. Ciarcelluti, S. Cassisi and A. Pietrinferni, astropart. Phys. 24, 495 (2006) [astro-ph/0507153]
2006
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
R. Foot, Phys. Rev. D69, 036001 (2004) [hep-ph/0308254]
2004
Cited alongside, same era.
R. Foot, Mod. Phys. Lett. A19, 1841 (2004) [astro-ph/0405362]
2004
Cited alongside, same era.
R. Foot, Int. J. Mod. Phys. D13, 2161 (2004) [astro-ph/0407623]
2004
Cited alongside, same era.
R. Foot and R. R. Volkas, Phys. Rev. D68, 021304 (2003) [hep-ph/0304261]; Phys. Rev. D69, 123510 (2004) [hep-ph/0402267]
2004
Cited alongside, same era.
R. Foot and R. R. Volkas, Phys. Rev. D70, 123508 (2004) [astro-ph/0407522]
2004
Cited alongside, same era.
R. Foot, Int. J. Mod. Phys. A19 3807 (2004) [astro-ph/0309330]
2004
Cited alongside, same era.
S. L. Glashow, Phys. Lett. B167, 35 (1986); R. Foot and S. N. Gninenko, Phys. Lett. B480, 171 (2000) [hep-ph/0003278]. Although the current best limit on ϵ \epsilon from laboratory experiments is [ 30 ] ϵ < 5 × 10 − 7 \epsilon<5\times 10^{-7} , forthcoming orthopositronium experiments [A. Badertscher et al
2004
Cited alongside, same era.
Later among the works it cites.
R. Bernabei et al
2007
Later among the works it cites.
S. Calchi Novati, II Nuovo Cimento 122B, 557 (2007) [arXiv:0711.4474]
2007
Later among the works it cites.
R. Bernabei et al. (DAMA Collaboration), arXiv:0804.2741 (2008)
2008
Closest in time.
Z. Ahmed et al
2008
Closest in time.
2008
Closest in time.
2008
Closest in time.
R. Bernabei et al
2008
Closest in time.