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Probing for variation of neutrino mass with current observations

Nov, 2006

4 pages

Published in:

JCAP 07 (2007) 010

e-Print:

astro-ph/0611227 [astro-ph]

DOI:

10.1088/1475-7516/2007/07/010

View in:

ADS Abstract Service

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Abstract: (arXiv)

With the latest astronomical data including Cosmic Microwave Background (WMAP three year, CBI, ACBAR, VSA), Type Ia Supernova (gold sample), galaxy clustering (SDSS 3-D matter power, Lyman-

\alpha

forest and Baryon Acoustic Oscillating (BAO)), we make a global fitting to constrain the mass varying neutrinos. We find the parameter denoting time evolving of neutrino mass

\delta

is weakly constrained and the neutrino mass limit today can be relaxed at least by a factor of 2. Adding data of

0\nu2\beta

decay of Heidelberg-Moscow experiment to our analysis, we find

\delta

can be measured and mass varying neutrinos are favored at about 99.7% confidence level.

Note:

4 pages, 4 figures

neutrino: mass
mass: time dependence
cosmic background radiation
supernova
data analysis method
galaxy: cluster
baryon: oscillation
oscillation: acoustic
double-beta decay: (0neutrino)
dark matter

References(43)

Figures(0)

Neutrino oscillations as a probe of dark energy

- Phys.Rev.Lett. 93 (2004) 091801
•
e-Print:
- hep-ph/0401099
•
DOI:
- 10.1103/PhysRevLett.93.091801

Solar mass-varying neutrino oscillations

V. Barger
(
- Wisconsin U., Madison
)
,
Patrick Huber
(
- Wisconsin U., Madison
)
,
Danny Marfatia
(
- Kansas U.
)

- Phys.Rev.Lett. 95 (2005) 211802
•
e-Print:
- hep-ph/0502196
•
DOI:
- 10.1103/PhysRevLett.95.211802

Mass varying neutrinos in the sun

Marco Cirelli
(
- Yale U.
)
,
M.C. Gonzalez-Garcia
(
- SUNY, Stony Brook and
- Valencia U., IFIC
)
,
Carlos Pena-Garay
(
- Princeton, Inst. Advanced Study
)

- Nucl.Phys.B 719 (2005) 219-233
•
e-Print:
- hep-ph/0503028
•
DOI:
- 10.1016/j.nuclphysb.2005.04.034

Confronting mass-varying neutrinos with MiniBooNE

- Phys.Rev.D 73 (2006) 013005
•
e-Print:
- hep-ph/0509163
•
DOI:
- 10.1103/PhysRevD.73.013005

Detecting dark energy in long baseline neutrino oscillations

Pei-Hong Gu
(
- Beijing, Inst. High Energy Phys.
)
,
Xiao-Jun Bi
(
- Beijing, Inst. High Energy Phys.
)
,
Bo Feng
(
- Beijing Observ. and
- Tokyo U., RESCEU
)
,
Bing-Lin Young
(
- Iowa State U.
)
,
Xinmin Zhang
(
- Beijing, Inst. High Energy Phys.
)

- Chin.Phys.C 32 (2008) 530-535
•
e-Print:
- hep-ph/0512076
•
DOI:
- 10.1088/1674-1137/32/7/004

Testing mass varying neutrino with short gamma ray burst

- Phys.Rev.D 71 (2005) 113003
•
e-Print:
- hep-ph/0411228
•
DOI:
- 10.1103/PhysRevD.71.113003

Probing Neutrino Dark Energy with Extremely High-Energy Cosmic Neutrinos

Andreas Ringwald
(
- Desy
)
,
Lily Schrempp
(
- Desy
)

- JCAP 10 (2006) 012
•
e-Print:
- astro-ph/0606316
•
DOI:
- 10.1088/1475-7516/2006/10/012

Cosmological evolution of interacting dark energy models with mass varying neutrinos

- Phys.Rev.D 72 (2005) 123523
•
e-Print:
- hep-ph/0412002
•
DOI:
- 10.1103/PhysRevD.72.123523

Thermal leptogenesis in a model with mass varying neutrinos

- Phys.Rev.D 69 (2004) 113007
•
e-Print:
- hep-ph/0311022
•
DOI:
- 10.1103/PhysRevD.69.113007

Thermal leptogenesis with triplet Higgs boson and mass varying neutrinos

- Phys.Rev.D 70 (2004) 063511
•
e-Print:
- hep-ph/0405092
•
DOI:
- 10.1103/PhysRevD.70.063511

Supernova constraints on models of neutrino dark energy

- Phys.Rev.D 73 (2006) 103503
•
e-Print:
- astro-ph/0509272
•
DOI:
- 10.1103/PhysRevD.73.103503

Cosmology with massive neutrinos coupled to dark energy

A.W. Brookfield
(
- Sheffield U.
)
,
Carsten van de Bruck
(
- Sheffield U.
)
,
D.F. Mota
(
- Inst. Theor. Astrophys., Oslo and
- Oxford U.
)
,
D. Tocchini-Valentini
(
- Oxford U.
)

- Phys.Rev.Lett. 96 (2006) 061301
•
e-Print:
- astro-ph/0503349
•
DOI:
- 10.1103/PhysRevLett.96.061301

Cosmology of mass-varying neutrinos driven by quintessence: theory and observations

Anthony W. Brookfield
(
- Sheffield U.
)
,
C. van de Bruck
(
- Sheffield U.
)
,
D.F. Mota
(
- Inst. Theor. Astrophys., Oslo
)
,
D. Tocchini-Valentini
(
- Oxford U. and
- Johns Hopkins U.
)

- Phys.Rev.D 73 (2006) 083515,
- Phys.Rev.D 76 (2007) 049901 (erratum)
•
e-Print:
- astro-ph/0512367
•
DOI:
- 10.1103/PhysRevD.73.083515

Dark energy and neutrino mass limits from baryogenesis

- Phys.Rev.D 68 (2003) 087301
•
e-Print:
- hep-ph/0307148
•
DOI:
- 10.1103/PhysRevD.68.087301

Dark energy from mass varying neutrinos

- JCAP 10 (2004) 005
•
e-Print:
- astro-ph/0309800
•
DOI:
- 10.1088/1475-7516/2004/10/005

Neutrino models of dark energy

R.D. Peccei
(
- UCLA
)

- Phys.Rev.D 71 (2005) 023527
•
e-Print:
- hep-ph/0411137
•
DOI:
- 10.1103/PhysRevD.71.023527

Dark energy and its interactions with neutrinos

Xin-min Zhang
(
- Beijing, Inst. High Energy Phys.
)

- AIP Conf.Proc. 805 (2005) 1, 3-9
•
e-Print:
- hep-ph/0510072
•
DOI:
- 10.1063/1.2149667

Search for neutrinoless double beta decay with enriched Ge-76 in Gran Sasso 1990-2003

- Phys.Lett.B 586 (2004) 198-212
•
e-Print:
- hep-ph/0404088
•
DOI:
- 10.1016/j.physletb.2004.02.025

Observables sensitive to absolute neutrino masses: A Reappraisal after WMAP-3y and first MINOS results

G.L. Fogli
(
- Bari U. and
- INFN, Bari
)
,
E. Lisi
(
- Bari U. and
- INFN, Bari
)
,
A. Marrone
(
- Bari U. and
- INFN, Bari
)
,
A. Melchiorri
(
- Rome U. and
- INFN, Rome
)
,
A. Palazzo
(
- Bari U. and
- INFN, Bari and
- Oxford U.
)

et al.

- Phys.Rev.D 75 (2007) 053001
•
e-Print:
- hep-ph/0608060
•
DOI:
- 10.1103/PhysRevD.75.053001

Cosmological perturbation theory in the synchronous and conformal Newtonian gauges

Chung-Pei Ma
(
- Caltech
)
,
Edmund Bertschinger
(
- MIT, LNS
)

- Astrophys.J. 455 (1995) 7-25
•
e-Print:
- astro-ph/9506072
•
DOI:
- 10.1086/176550

Evolution of cosmological dark matter perturbations

Antony Lewis
(
- Cambridge U., DAMTP
)
,
Anthony Challinor
(
- Cambridge U.
)

- Phys.Rev.D 66 (2002) 023531
•
e-Print:
- astro-ph/0203507
•
DOI:
- 10.1103/PhysRevD.66.023531

Cosmological parameters from CMB and other data: A Monte Carlo approach

- Phys.Rev.D 66 (2002) 103511
•
e-Print:
- astro-ph/0205436
•
DOI:
- 10.1103/PhysRevD.66.103511

Wilkinson Microwave Anisotropy Probe (WMAP) three year results: implications for cosmology

WMAP

Collaboration

•

D.N. Spergel
(
- Princeton U., Astrophys. Sci. Dept. and
- Cerro-Tololo InterAmerican Obs.
)

et al.

- Astrophys.J.Suppl. 170 (2007) 377
•
e-Print:
- astro-ph/0603449
•
DOI:
- 10.1086/513700

Three year Wilkinson Microwave Anisotropy Probe (WMAP) observations: polarization analysis

WMAP

Collaboration

•

L. Page

et al.

- Astrophys.J.Suppl. 170 (2007) 335
•
e-Print:
- astro-ph/0603450
•
DOI:
- 10.1086/513699

Three-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: temperature analysis

WMAP

Collaboration

•

G. Hinshaw
(
- NASA, Goddard
)

et al.

- Astrophys.J.Suppl. 170 (2007) 288
•
e-Print:
- astro-ph/0603451
•
DOI:
- 10.1086/513698

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