Testing the variability of the proton-to-electron mass ratio from observations of methanol in the dark cloud core L1498
arXiv:1709.03103 · doi:10.1093/mnras/stx2308
Abstract
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 detected and an extra line was tentatively detected at a lower confidence level in one of the positions. The observed centroid frequencies were then compared with their rest frame frequencies derived from least-squares fitting to a large data set. Systematic effects, as the underlying methanol hyperfine structure and the Doppler tracking of the telescope, were investigated and their effects were included in the total error budget. The comparison between the observations and the rest frame frequencies constrains potential mu variation at the level of Dmu/mu < 6 x 10^(-8), at a 3 sigma confidence level. For the dark cloud we determine a total CH3OH (A+E) beam averaged column density of 3-4 x 10^(12) cm(-2) (within roughly a factor of two), an E- to A-type methanol column density ratio of N(A-CH3OH)/N(E-CH3OH) = 1.00 +/- 0.15, a density of n(H2) = 3 x 10^5 cm^(-3) (again within a factor of two), and a kinetic temperature of Tkin = 6 +/- 1 K. In a kinetic model including the line intensities observed for the methanol lines, the n(H2) density is higher and the temperature is lower than that derived in previous studies based on different molecular species; the intensity of the 1_0 --> 1_-1 E line strength is not well reproduced.
10 pages, 6 figures, accepted for publication in MNRAS
References in corpus (7)
- Environmental Dependence of Masses and Coupling Constants
- On the internal structure of starless cores. II. A molecular survey of L1498 and L1517B
- Strong Limit on a Variable Proton-to-Electron Mass Ratio from Molecules in the Distant Universe
- Enhanced sensitivity to time-variation of m_p/m_e in the inversion spectrum of ammonia
- The UVES Large Program for testing fundamental physics - III. Constraints on the fine-structure constant from 3 telescopes
- Constraints on changes in the proton-electron mass ratio using methanol lines
- Limits on a Gravitational Field Dependence of the Proton--Electron Mass Ratio from H in White Dwarf Stars
Cited by in corpus (7)
- Vibronic branching ratios for nearly-closed rapid photon cycling of SrOH
- A study of submillimeter methanol absorption toward PKS1830-211: Excitation, invariance of the proton-electron mass ratio, and systematics
- Testing the weak equivalence principle by differential measurements of fundamental constants in the Magellanic Clouds
- Constraints on the electron-to-proton mass ratio variation at the epoch of reionization
- Methanol isotopologues as a probe for spatial and temporal variations of the electron-to-proton mass ratio
- Probing the electron-to-proton mass ratio gradient in the Milky Way with class I methanol masers
- Optically Derived Radio-Frequency Benchmark in Methanol: A Sub-kHz Reference for Astrophysical Tests of Fundamental Physics