2014
DOI: 10.1103/physrevlett.113.123002
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Limits on a Gravitational Field Dependence of the Proton-Electron Mass Ratio fromH2in White Dwarf Stars

Abstract: Spectra of molecular hydrogen (H2) are employed to search for a possible proton-to-electron mass ratio (μ) dependence on gravity. The Lyman transitions of H2, observed with the Hubble Space Telescope towards white dwarf stars that underwent a gravitational collapse, are compared to accurate laboratory spectra taking into account the high temperature conditions (T∼13 000  K) of their photospheres. We derive sensitivity coefficients Ki which define how the individual H2 transitions shift due to μ dependence. The… Show more

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Cited by 29 publications
(33 citation statements)
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“…(2) doubles for condensed matter and given particulate electron's ( ) = 4.8828 10 , remaining as cognitively unclear as before". Variability of μ has been extensively investigated and majority findings would seem to support invariability, Ubachs et al (2015), Duff (2004), Varshalovich (1999), Bagdonaite et al (2014), Godun et al (2014), Kirakosyan (2015), Consiglio (2016), Gabrielse (2006), Berkenstein (1982), Berkenstein (2002).…”
Section: Planck Constant Hmentioning
confidence: 99%
“…(2) doubles for condensed matter and given particulate electron's ( ) = 4.8828 10 , remaining as cognitively unclear as before". Variability of μ has been extensively investigated and majority findings would seem to support invariability, Ubachs et al (2015), Duff (2004), Varshalovich (1999), Bagdonaite et al (2014), Godun et al (2014), Kirakosyan (2015), Consiglio (2016), Gabrielse (2006), Berkenstein (1982), Berkenstein (2002).…”
Section: Planck Constant Hmentioning
confidence: 99%
“…More recently direct observational constraints have been obtained, also at about the 50 ppm level of sensitivity, for both α and µ using white dwarf stars [127,128]. These come from spectroscopic observations of highly excited metal lines (FeV and NiV) and molecular hydrogen, respectively Two-dimensional likelihoods for each pair of couplings, marginalizing over the other, from a global analysis of the data in Table 6.…”
Section: Other Probesmentioning
confidence: 99%
“…In view of the high local temperatures higher vibrational states of H 2 are populated in the WD photospheres, in contrast to the cold environments probed in quasar absorption, where only H 2 (v = 0) is detected. In view of the Franck-Condon factors of H 2 the Lyman bands B-X(1, 3) and (1, 4) are the most strongly represented in the observed spectrum which covers the range 1310-1412 Å (Bagdonaite et al 2014a). At temperatures of T > 10 000 K rotational quantum states of up to J = 25 are effectively populated and a simulation of the spectra involves starting from the partition function including all states populated (Salumbides et al 2015):…”
Section: Detection Of H 2 In the Photosphere Of White Dwarfsmentioning
confidence: 97%
“…for GD-133 (at φ = 1.2 × 10 −4 ) (Bagdonaite et al 2014a). Thus far the objects GD-29-38 and GD-133 are the only white dwarf stars for which an H 2 absorption spectrum of sufficient SNR was obtained.…”
Section: Detection Of H 2 In the Photosphere Of White Dwarfsmentioning
confidence: 99%