%0 Generic %1 citeulike:13495342 %A Klöckner, H. R. %A Obreschkow, D. %A Martins, C. %A Raccanelli, A. %A Champion, D. %A Roy, A. %A Lobanov, A. %A Wagner, J. %A Keller, R. %D 2015 %K imported %T Real time cosmology - A direct measure of the expansion rate of the Universe %U http://arxiv.org/abs/1501.03822 %X In recent years cosmology has undergone a revolution, with precise measurements of the microwave background radiation, large galaxy redshift surveys, and the discovery of the recent accelerated expansion of the Universe using observations of distant supernovae. In this light, the SKA enables us to do an ultimate test in cosmology by measuring the expansion rate of the Universe in real time. This can be done by a rather simple experiment of observing the neutral hydrogen (HI) signal of galaxies at two different epochs. The signal will encounter a change in frequency imprinted as the Universe expands over time and thus monitoring the drift in frequencies will provide a real time measure of the cosmic acceleration. Over a period of 12 years one would expected a frequency shift of the order of 0.1 Hz assuming a standard Lambda-CDM cosmology. Based on the sensitivity estimates of the SKA and the number counts of the expected HI galaxies, it is shown that the number counts are sufficiently high to compensate for the observational uncertainties of the measurements and hence allow a statistical detection of the frequency shift. abstract abridged

@misc{citeulike:13495342, abstract = {{In recent years cosmology has undergone a revolution, with precise measurements of the microwave background radiation, large galaxy redshift surveys, and the discovery of the recent accelerated expansion of the Universe using observations of distant supernovae. In this light, the SKA enables us to do an ultimate test in cosmology by measuring the expansion rate of the Universe in real time. This can be done by a rather simple experiment of observing the neutral hydrogen (HI) signal of galaxies at two different epochs. The signal will encounter a change in frequency imprinted as the Universe expands over time and thus monitoring the drift in frequencies will provide a real time measure of the cosmic acceleration. Over a period of 12 years one would expected a frequency shift of the order of 0.1 Hz assuming a standard Lambda-CDM cosmology. Based on the sensitivity estimates of the SKA and the number counts of the expected HI galaxies, it is shown that the number counts are sufficiently high to compensate for the observational uncertainties of the measurements and hence allow a statistical detection of the frequency shift. [abstract abridged]}}, added-at = {2019-03-25T08:20:55.000+0100}, archiveprefix = {arXiv}, author = {Kl\"{o}ckner, H. R. and Obreschkow, D. and Martins, C. and Raccanelli, A. and Champion, D. and Roy, A. and Lobanov, A. and Wagner, J. and Keller, R.}, biburl = {https://www.bibsonomy.org/bibtex/204b0edb69d0a04e6fb8326a6e7c15e9a/ericblackman}, citeulike-article-id = {13495342}, citeulike-linkout-0 = {http://arxiv.org/abs/1501.03822}, citeulike-linkout-1 = {http://arxiv.org/pdf/1501.03822}, day = 15, eprint = {1501.03822}, interhash = {636296920c6d58261e7ce7b42abe9c4b}, intrahash = {04b0edb69d0a04e6fb8326a6e7c15e9a}, keywords = {imported}, month = jan, posted-at = {2015-01-19 04:34:47}, priority = {2}, timestamp = {2019-03-25T08:20:55.000+0100}, title = {{Real time cosmology - A direct measure of the expansion rate of the Universe}}, url = {http://arxiv.org/abs/1501.03822}, year = 2015 }