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Cosmological constraints on
sterile neutrino mass
in gravity
Hayato Motohashi
本橋 隼人 (RESCEU, The University of Tokyo)
1 2012.11.12-16 RESCEU symposium and JGRG22, Univ. of Tokyo
Alexei A. Starobinsky (Landau Inst.)
Jun’ichi Yokoyama (RESCEU)
in collaboration with
Two regimes of accelerated expansion
2
Reheating
gravity
can describe the accelerated expansion.
Primordial inflation
Late-time acceleration
3
Starobinsky, JETP Lett. 86, 157 (2007)
[arXiv:0706.2041]
Starobinsky, Phys.Lett. B91 (1980) 99
Appleby, Battye, Starobinsky, JCAP 1006, 005 (2010) [arXiv:0909.1737]
H.M., Nishizawa, PRD 86 (2012) 093514 [arXiv:1204.1472]
cf. model for both accelerated expansion
4
Local scale
Solar system test
Horizon scale
Expansion history
Testing modified gravity
Intermediate scale
Large scale structure
Time variation of EoS parameter
5
- 0.92 - 0.23
- 0.94 - 0.22
- 0.96 - 0.21
H.M., Starobinsky, Yokoyama
PTP 123 (2010) 887 [arXiv:1002.1141]
Komatsu et al.,
APJ Suppl. 192, 18 (2011)
[arXiv:1001.4538]
Growth index
Rapetti et al., arXiv: 1205.4679 6
H.M., Starobinsky, Yokoyama
PTP 123 (2010) 887 [arXiv:1002.1141]
Additional transfer function in gravity
gravity enhances matter power spectrum.
cancel
Massive neutrino suppresses matter power spectrum.
7
Constraint on from BBN
8
[331] Izotov, Thuan, Astrophys.J. 710, L67 (2010) [arXiv:1001.4440]
[332] Mangano,Serpico, Phys.Lett. B701, 296 (2011) [arXiv:1103.1261]
[333] Nollett, Holder [arXiv:1112.2683]
[122] Hamann et al, JCAP 1109, 034 (2011) [arXiv:1108.4136]
Abazajian et al [arXiv:1204.5379]
Constraints on and in ΛCDM
CMB
9
(95% CL)
(68% CL)
LSS
ΛCDM + Komatsu et al.,
APJ Suppl. 192, 18 (2011)
[arXiv:1001.4538]
Reid et al,
Mon.Not.Roy.Astron.Soc. 404
(2010) 60 [arXiv:0907.1659]
Constraints on and in ΛCDM
10
Riemer-Sorensen et al
[arXiv:1210.2131]
ΛCDM cosmology
sub-eV
sterile neutrino
Sterile neutrino mass 1 eV
ΛCDM model
11
Mention et al.,
PRD 83, 073006 (2011)
[arXiv:1101.2755]
Giunti, Laveder,
Phys.Rev. C83 (2011) 065504
[arXiv:1006.3244]
Antonello et al,
[arXiv:1209.0122]
Neutrino oscillation
MCMC analysis: ΛCDM vs gravity
12
H.M., Starobinsky and Yokoyama, arXiv:1203.6828
3 massless and 1 massive neutrino with mass = 1 eV
WMAP7, SDSS DR 7
Better fit : 10.7 (Δ AIC = 8.7)
GR : , :
ΛCDM
MCMC analysis: ΛCDM vs gravity
13
H.M., Starobinsky and Yokoyama, arXiv:1203.6828
3 massless and 1 massive neutrino with mass = 1 eV
WMAP7, SDSS DR 7
Better fit : 10.7 (Δ AIC = 8.7)
GR : , :
ΛCDM
WMAP
ΛCDM
SDSS
14
Summary
14
Cosmology based on ΛCDM model
Sterile neutrino mass 1 eV
Neutrino oscillation experiments
Sterile neutrino mass 1 eV
gravity can resolve the tension.