Asset Details
MbrlCatalogueTitleDetail
Do you wish to reserve the book?
Constraints on the electron-to-proton mass ratio variation at the epoch of reionization
by
Levshakov, S A
, Kozlov, M G
, Agafonova, I I
in
Dark energy
/ Dark matter
/ Ionization
/ Protons
/ Red shift
2020
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
You are currently in the queue to collect this book. You will be notified once it is your turn to collect the book.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
Oops! Something went wrong.
While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
Constraints on the electron-to-proton mass ratio variation at the epoch of reionization
by
Levshakov, S A
, Kozlov, M G
, Agafonova, I I
in
Dark energy
/ Dark matter
/ Ionization
/ Protons
/ Red shift
2020
Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
Constraints on the electron-to-proton mass ratio variation at the epoch of reionization
Paper
Constraints on the electron-to-proton mass ratio variation at the epoch of reionization
2020
Request Book From Autostore
and Choose the Collection Method
Overview
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 mu/mu = (mu_obs - mu_lab)/mu_lab = (0.7 +/- 1.2)x10^-5 (1sigma) obtained at = 6.31 is the most stringent up-to-date limit on the variation of mu at such high redshift. For all available estimates of Delta mu/mu ranging between z = 0 and z = 1100, - the epoch of recombination, - a regression curve Delta mu/mu = k_mu (1+z)^p, with k_mu = (1.6 +/- 0.3) x10^-8 and p = 2.00 +/- 0.03, is deduced. If confirmed, this would imply a dynamical nature of dark matter/dark energy.
Publisher
Cornell University Library, arXiv.org
Subject
This website uses cookies to ensure you get the best experience on our website.