New constraint on cosmological variation of the proton-to-electron mass ratio from Q0528-250

J.A. King; M.T. Murphy; W.M.G. Ubachs; J.K. Webb

doi:10.1111/j.1365-2966.2011.19460.x

New constraint on cosmological variation of the proton-to-electron mass ratio from Q0528-250

J.A. King, M.T. Murphy, W.M.G. Ubachs, J.K. Webb

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Abstract

Molecular hydrogen transitions in quasar spectra can be used to constrain variation in the proton-to-electron mass ratio, μ≡m

Original language	English
Pages (from-to)	3010-3024
Number of pages	15
Journal	Monthly Notices of the Royal Astronomical Society
Volume	417
DOIs	https://doi.org/10.1111/j.1365-2966.2011.19460.x
Publication status	Published - 2011

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@article{8314e12ea6ec4238a914430abd88faae,

title = "New constraint on cosmological variation of the proton-to-electron mass ratio from Q0528-250",

abstract = "Molecular hydrogen transitions in quasar spectra can be used to constrain variation in the proton-to-electron mass ratio, μ≡m",

author = "J.A. King and M.T. Murphy and W.M.G. Ubachs and J.K. Webb",

year = "2011",

doi = "10.1111/j.1365-2966.2011.19460.x",

language = "English",

volume = "417",

pages = "3010--3024",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

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T1 - New constraint on cosmological variation of the proton-to-electron mass ratio from Q0528-250

AU - King, J.A.

AU - Murphy, M.T.

AU - Ubachs, W.M.G.

AU - Webb, J.K.

PY - 2011

Y1 - 2011

N2 - Molecular hydrogen transitions in quasar spectra can be used to constrain variation in the proton-to-electron mass ratio, μ≡m

AB - Molecular hydrogen transitions in quasar spectra can be used to constrain variation in the proton-to-electron mass ratio, μ≡m

U2 - 10.1111/j.1365-2966.2011.19460.x

DO - 10.1111/j.1365-2966.2011.19460.x

M3 - Article

VL - 417

SP - 3010

EP - 3024

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

ER -

New constraint on cosmological variation of the proton-to-electron mass ratio from Q0528-250

Abstract

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