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相关论文: Limits on the space-time variations of fundamental…

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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…

星系天体物理 · 物理学 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…

宇宙学与河外天体物理 · 物理学 2009-11-05 Paolo Molaro , Sergei A. Levshakov , MiKhail G. Kozlov

(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…

天体物理学 · 物理学 2008-08-06 S. A. Levshakov , P. Molaro , M. G. Kozlov

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…

宇宙学与河外天体物理 · 物理学 2009-11-20 S. A. Levshakov , I. I. Agafonova , P. Molaro , D. Reimers

(Abridged) In our previous work we found a statistically significant offset Delta V = 27 m/s between the radial velocities of the HC3N(2-1) and NH3(1,1) transitions observed in molecular cores from the Milky Way. This may indicate that the…

宇宙学与河外天体物理 · 物理学 2015-06-11 S. A. Levshakov , A. V. Lapinov , C. Henkel , P. Molaro , D. Reimers , M. G. Kozlov , I. I. Agafonova

(Abridged) A procedure is suggested to explore the value of F = alpha^2/mu, where mu = m_e/m_p is the electron-to-proton mass ratio, and alpha is the fine-structure constant. The fundamental physical constants, which are measured in…

宇宙学与河外天体物理 · 物理学 2015-05-18 S. A. Levshakov , P. Molaro , D. Reimers

Using the 32-m Medicina, 45-m Nobeyama, and 100-m Effelsberg telescopes we found a statistically significant velocity offset Delta V = 27 +/- 3 m/s (1sigma) between the inversion transition in NH3(1,1) and low-J rotational transitions in…

宇宙学与河外天体物理 · 物理学 2016-02-03 S. A. Levshakov , P. Molaro , M. G. Kozlov , A. V. Lapinov , C. Henkel , D. Reimers , T. Sakai , I. I. Agafonova

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…

天体物理学 · 物理学 2014-10-13 S. A. Levshakov , M. Dessauges-Zavadsky , S. D'Odorico , P. Molaro

Many modern theories predict that the fundamental constants depend on time, position, or the local density of matter. We develop a spectroscopic method for pulsed beams of cold molecules, and use it to measure the frequencies of microwave…

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…

天体物理学 · 物理学 2009-08-18 Michael T. Murphy , Victor V. Flambaum , Sebastien Muller , Christian Henkel

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 </=…

宇宙学与河外天体物理 · 物理学 2015-06-15 Rodger I. Thompson

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) Many-multiplet (MM) method applied to three inhomogeneous samples of Keck/HIRES quasar absorption spectra gives a shift in the value of the fine-structure constant of Delta alpha/alpha = (-5.4+/-1.2) 10^{-6} in the redshift range…

天体物理学 · 物理学 2017-08-23 Sergei A. Levshakov

The variation of the dimensionless fundamental physical constant mu = m_p/m_e (the proton to electron mass ratio) can be constrained via observation of Lyman and Werner lines of molecular hydrogen in the spectra of damped Lyman alpha…

宇宙学与河外天体物理 · 物理学 2015-06-04 Martin Wendt , Paolo Molaro

Precision comparisons of different atomic frequency standards over a period of a few years can be used for a sensitive search for temporal variations of fundamental constants. We present recent frequency measurements of the 688 THz…

原子物理 · 物理学 2008-11-25 E. Peik , B. Lipphardt , H. Schnatz , Chr. Tamm , S. Weyers , R. Wynands

This article summarizes the latest results on the proton-to-electron mass ratio $\mu$ derived from H$_2$ observations at high redshift in the light of possible variations of fundamental physical constants. The focus lies on UVES…

宇宙学与河外天体物理 · 物理学 2015-06-17 Martin Wendt

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…

宇宙学与河外天体物理 · 物理学 2013-12-11 Julija Bagdonaite , Mario Daprà , Paul Jansen , Hendrick L. Bethlem , Wim Ubachs , Sébastien Muller , Christian Henkel , Karl M. Menten

Far infrared fine-structure transitions of CI and CII and rotational transitions of CO are used to probe hypothetical variations of the electron-to-proton mass ratio mu = m_e/m_p at the epoch of reionization (z > 6). A constraint on Delta…

宇宙学与河外天体物理 · 物理学 2020-09-09 S. A. Levshakov , M. G. Kozlov , I. I. Agafonova

Aims. We constrain a hypothetical variation in the fundamental physical constants over the course of cosmic time. Methods. We use unique observations of the CO(7-6) rotational line and the [CI] 3P_2 - 3P_1 fine-structure line towards a…

宇宙学与河外天体物理 · 物理学 2013-06-12 S. A. Levshakov , F. Combes , F. Boone , I. I. Agafonova , D. Reimers , M. G. Kozlov

We present a strong constraint on variation of the proton-to-electron mass ratio, mu, over cosmological time scales using molecular hydrogen transitions in optical quasar spectra. Using high quality spectra of quasars Q0405-443, Q0347-383…

天体物理学 · 物理学 2010-05-12 Julian A. King , John K. Webb , Michael T. Murphy , Robert F. Carswell
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