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Related papers: Indication of the electron-to-proton mass ratio va…

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Differential measurements of the fundamental constant mu = m_e/m_p (the electron-to-proton mass ratio) for two sources near the Galactic Center - the Sgr B2(N) and B2(M) molecular clouds - suggest that mu is lower in these clouds than its…

Astrophysics of Galaxies · Physics 2025-11-04 J. S. Vorotyntseva , S. A. Levshakov , C. Henkel

In this paper, we show that methanol (CH3OH) torsional-rotational transitions, which have increased sensitivity to small variations of mu - the electron-to-proton mass ratio, are shifted relative to less sensitive transitions in the…

Astrophysics of Galaxies · Physics 2026-03-09 J. S. Vorotyntseva , S. A. Levshakov

We report on the using of torsion-rotational transitions in the CH3OH and (13)CH3OH molecules to evaluate possible variations of the physical constant mu=m_e/m_p - the electron-to-proton mass ratio - from spectral observations of emission…

Astrophysics of Galaxies · Physics 2024-05-09 J. S. Vorotyntseva , S. A. Levshakov

We present results on numerical calculations of the sensitivity coefficients, Qmu, of microwave molecular transitions in (13C)H3OH and CH3(18O)H to the hypothetical variation in the fundamental physical constant mu - the electron-to-proton…

Astrophysics of Galaxies · Physics 2023-11-17 J. S. Vorotyntseva , M. G. Kozlov , S. A. Levshakov

The dependence of the proton-to-electron mass ratio, mu, on the local matter density was investigated using methanol emission in the dense dark cloud core L1498. Towards two different positions in L1498, five methanol transitions were…

Cosmology and Nongalactic Astrophysics · Physics 2017-10-18 M. Daprà , C. Henkel , S. A. Levshakov , K. M. Menten , S. Muller , H. L. Bethlem , S. Leurini , A. V. Lapinov , W. Ubachs

A limit on a possible cosmological variation of the proton-to-electron mass ratio $\mu$ is derived from methanol (CH$_3$OH) absorption lines in the benchmark PKS1830$-$211 lensing galaxy at redshift $z = 0.89$ observed with the Effelsberg…

Cosmology and Nongalactic Astrophysics · Physics 2013-12-11 Julija Bagdonaite , Mario Daprà , Paul Jansen , Hendrick L. Bethlem , Wim Ubachs , Sébastien Muller , Christian Henkel , Karl M. Menten

New PKS1830-211 radio frequency observations of methanol at a redshift of 0.88582 have established the most stringent limits on changes in the proton to electron mass ratio mu to date. The observations place the limit of (delta mu)/mu </=…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Rodger I. Thompson

We estimate limits on non-universal coupling of hypothetical hidden fields to standard matter by evaluating the fractional changes in the electron-to-proton mass ratio, mu = m_e/m_p, based on observations of ClassI methanol masers…

Astrophysics of Galaxies · Physics 2022-01-19 S. A. Levshakov , I. I. Agafonova , C. Henkel , Kee-Tae Kim , M. G. Kozlov , B. Lankhaar , W. Yang

The possible cosmological variation of the proton-to-electron mass ratio was estimated by measuring the H_2 wavelengths in the high-resolution spectrum of the quasar Q~0347-382. Our analysis yielded an estimate for the possible deviation of…

Astrophysics · Physics 2009-11-07 A. Ivanchik , P. Petitjean , E. Rodriguez , D. Varshalovich

We report on new tests that improve our previous (2009-2010) estimates of the electron-to-proton mass ratio variation, mu = m_e/m_p. Subsequent observations (2011-2013) at the Effelsberg 100-m telescope of a sample of eight molecular cores…

Cosmology and Nongalactic Astrophysics · Physics 2013-10-02 S. A. Levshakov , C. Henkel , D. Reimers , P. Molaro

Aims. To validate the Einstein equivalence principle (local position invariance) by limiting the fractional changes in the electron-to-proton mass ratio, mu = m_e/m_p, measured in Galactic plane objects. Methods. High resolution spectral…

Astrophysics of Galaxies · Physics 2015-06-17 S. A. Levshakov , D. Reimers , C. Henkel , B. Winkel , A. Mignano , M. Centurion , P. Molaro

The ammonia method to probe variations of the electron-to-proton mass ratio, Delta_mu/mu, is applied for the first time to dense prestellar molecular clouds in the Milky Way. Carefully selected sample of 21 NH_3/CCS pairs observed in the…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-05 Paolo Molaro , Sergei A. Levshakov , MiKhail G. Kozlov

We report Karl G. Jansky Very Large Array (VLA) absorption spectroscopy in four methanol (CH$_3$OH) lines in the $z = 0.88582$ gravitational lens towards PKS1830-211. Three of the four lines have very different sensitivity coefficients…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-23 N. Kanekar , W. Ubachs , K. M. Menten , J. Bagdonaite , A. Brunthaler , C. Henkel , S. Muller , H. L. Bethlem , M. Dapra

The Standard Model of particle physics assumes that the so-called fundamental constants are universal and unchanging. Absorption lines arising in molecular clouds along quasar sightlines offer a precise test for variations in the…

Astrophysics · Physics 2009-08-18 Michael T. Murphy , Victor V. Flambaum , Sebastien Muller , Christian Henkel

(Abridged) Radio-astronomical observations of molecular cores in lines of NH3 (J,K)=(1,1), CCS J_N=2_1-1_0, HC3N J=5-4, and N2H+ J=1-0 are used to measure the relative radial velocity offsets, Delta V, between the NH3 (1,1) and other…

Astrophysics · Physics 2008-08-06 S. A. Levshakov , P. Molaro , M. G. Kozlov

Exotic cosmologies predict variability of the fundamental physical constants over the cosmic time. Using the VLT/UVES high resolution spectra of the quasar Q0347-3819 and unblended electronic - vibrational - rotational lines of the H2…

Astrophysics · Physics 2014-10-13 S. A. Levshakov , M. Dessauges-Zavadsky , S. D'Odorico , P. Molaro

A new limit on the possible cosmological variation of the proton-to-electron mass ratio \mu=m_p/m_e is estimated by measuring wavelengths of H_2 lines of Lyman and Werner bands from two absorption systems at z_abs = 2.5947 and 3.0249 in the…

Astrophysics · Physics 2009-11-13 A. Ivanchik , P. Petitjean , D. Varshalovich , B. Aracil , R. Srianand , H. Chand , C. Ledoux , P. Boisse

In an effort to resolve the discrepancy between two measurements of the fundamental constant mu, the proton to electron mass ratio, at early times in the universe we reanalyze the same data used in the earlier studies. Our analysis of the…

(Abridged) The ammonia method, which has been proposed to explore the electron-to-proton mass ratio, mu = m_e/m_p, is applied to nearby dark clouds in the Milky Way. This ratio, which is measured in different physical environments of high…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 S. A. Levshakov , P. Molaro , A. V. Lapinov , D. Reimers , C. Henkel , T. Sakai

Spatial and temporal variations in the electron-to-proton mass ratio, mu, and in the fine-structure constant, alpha, are predicted in non-Standard models aimed to explain the nature of dark energy. Among them the so-called chameleon-like…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-20 S. A. Levshakov , I. I. Agafonova , P. Molaro , D. Reimers
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