Built on

A. Aguilar-Arevalo et al. (MiniBooNE Collaboration), Phys.Rev.Lett. 103
Original
1958
Earlier work this paper cites.
R. Cowsik and J. McClelland, Phys.Rev.Lett. 29
1972
Earlier work this paper cites.
G. Steigman, D. N. Schramm, and J. E. Gunn, Phys. Lett. B66
1977
Earlier work this paper cites.
L. M. Krauss and P. Romanelli, Astrophys. J. 358
1990
Earlier work this paper cites.
K. Enqvist, K. Kainulainen, and M. J. Thomson, Nucl. Phys. B373
1992
Earlier work this paper cites.
P. J. Kernan and L. M. Krauss, Phys. Rev. Lett. 72
1994
Earlier work this paper cites.
S. Dodelson and L. M. Widrow, Phys. Rev. Lett. 72
Original
1994
Earlier work this paper cites.
R. Foot and R. R. Volkas, Phys. Rev. Lett. 75
1995
Earlier work this paper cites.
R. Foot and R. R. Volkas, Phys. Rev. D55
1997
Earlier work this paper cites.
E. Ma, G. Rajasekaran, and I. Stancu, Phys.Rev. D61
2000
Earlier work this paper cites.
P. Di Bari, P. Lipari, and M. Lusignoli, Int.J.Mod.Phys. A15
2000
Earlier work this paper cites.
A. Aguilar et al. (LSND), Phys. Rev. D64
2001
Earlier work this paper cites.
K. Abazajian, G. M. Fuller, and M. Patel, Phys. Rev. D64
2001
Earlier work this paper cites.
G. Mangano et al. , Nucl. Phys. B729
2005
Earlier work this paper cites.
S. Palomares-Ruiz, S. Pascoli, and T. Schwetz, JHEP 0509
2005
Earlier work this paper cites.
M. Cirelli, G. Marandella, A. Strumia, and F. Vissani, Nucl. Phys. B708
2005
Earlier work this paper cites.
S. Dodelson, A. Melchiorri, and A. Slosar, Phys.Rev.Lett. 97
2006
Earlier work this paper cites.
K. Ichikawa, M. Kawasaki, K. Nakayama, M. Senami, and F. Takahashi, JCAP 0705
2007
Earlier work this paper cites.

Similar

D. Boyanovsky and C. M. Ho, JHEP 07
2007
Cited alongside, same era.
M. Maltoni and T. Schwetz, Phys.Rev. D76
Original
2007
Cited alongside, same era.
A. Melchiorri, O. Mena, S. Palomares-Ruiz, S. Pascoli, A. Slosar, et al. , JCAP 0901
Original
2009
Cited alongside, same era.
J. Abdurashitov et al. (SAGE Collaboration), Phys.Rev. C80
Original
2009
Cited alongside, same era.
L. M. Krauss, C. Lunardini, and C. Smith, (2010), arXiv:1009.4666 [hep-ph]
Original
2010
Cited alongside, same era.

Then

D. Hooper, F. S. Queiroz, and N. Y. Gnedin, Phys.Rev. D85
Original
2012
Later among the works it cites.
E. Aver, K. A. Olive, and E. D. Skillman, JCAP 1204
Original
2012
Later among the works it cites.
Z. Hou, C. Reichardt, K. Story, B. Follin, R. Keisler, et al. , (2012), arXiv:1212.6267 [astro-ph.CO]
Original
2012
Later among the works it cites.
G. Hinshaw, D. Larson, E. Komatsu, D. Spergel, C. Bennett, et al. , (2012), arXiv:1212.5226 [astro-ph.CO]
Original
2012
Later among the works it cites.
A. Aguilar-Arevalo et al. (MiniBooNE Collaboration), (2012), arXiv:1207.4809 [hep-ex]
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…

2013

Additional Light Sterile Neutrinos and Cosmology

Jacques, Thomas D., Krauss, Lawrence M., Lunardini, Cecilia

Understand

Tantalizing cosmological and terrestrial evidence suggests the number of light neutrinos may be greater than 3, motivating a careful re-examination of cosmological bounds on extra light species.

Big Bang Nucleosynthesis constrains the number of relativistic neutrino species present during nucleosynthesis, $N_{eff}^{BBN}$, while measurements of the CMB angular power spectrum constrain the effective energy density in relativistic neutrinos at the time of matter-radiation equality, $N_{eff}^{CMB}$.
There are a number of scenarios where new sterile neutrino species may have different contributions to $\Delta N_{eff}^{BBN}$ and $\Delta N_{eff}^{CMB}$, for masses that may be relevant to reconciling cosmological constraints with various terrestrial claims of neutrino oscillations.
We consider a scenario with two sterile neutrinos and explore whether partial thermalization of the sterile states can ease the tension between cosmological constraints on $N_{eff}^{BBN}$ and terrestrial data.

Built on

A. Aguilar-Arevalo et al. (MiniBooNE Collaboration), Phys.Rev.Lett. 103
Original
1958
Earlier work this paper cites.
R. Cowsik and J. McClelland, Phys.Rev.Lett. 29
1972
Earlier work this paper cites.
G. Steigman, D. N. Schramm, and J. E. Gunn, Phys. Lett. B66
1977
Earlier work this paper cites.
L. M. Krauss and P. Romanelli, Astrophys. J. 358
1990
Earlier work this paper cites.
K. Enqvist, K. Kainulainen, and M. J. Thomson, Nucl. Phys. B373
1992
Earlier work this paper cites.
P. J. Kernan and L. M. Krauss, Phys. Rev. Lett. 72
1994
Earlier work this paper cites.
S. Dodelson and L. M. Widrow, Phys. Rev. Lett. 72
Original
1994
Earlier work this paper cites.
R. Foot and R. R. Volkas, Phys. Rev. Lett. 75
1995
Earlier work this paper cites.
R. Foot and R. R. Volkas, Phys. Rev. D55
1997
Earlier work this paper cites.
E. Ma, G. Rajasekaran, and I. Stancu, Phys.Rev. D61
2000
Earlier work this paper cites.
P. Di Bari, P. Lipari, and M. Lusignoli, Int.J.Mod.Phys. A15
2000
Earlier work this paper cites.
A. Aguilar et al. (LSND), Phys. Rev. D64
2001
Earlier work this paper cites.
K. Abazajian, G. M. Fuller, and M. Patel, Phys. Rev. D64
2001
Earlier work this paper cites.
G. Mangano et al. , Nucl. Phys. B729
2005
Earlier work this paper cites.
S. Palomares-Ruiz, S. Pascoli, and T. Schwetz, JHEP 0509
2005
Earlier work this paper cites.
M. Cirelli, G. Marandella, A. Strumia, and F. Vissani, Nucl. Phys. B708
2005
Earlier work this paper cites.
S. Dodelson, A. Melchiorri, and A. Slosar, Phys.Rev.Lett. 97
2006
Earlier work this paper cites.
K. Ichikawa, M. Kawasaki, K. Nakayama, M. Senami, and F. Takahashi, JCAP 0705
2007
Earlier work this paper cites.