dc.contributor.author |
Shandera, S |
en |
dc.contributor.author |
Adshead, P |
en |
dc.contributor.author |
Amin, M |
en |
dc.contributor.author |
Dimastrogiovanni, E |
en |
dc.contributor.author |
Dvorkin, C |
en |
dc.contributor.author |
Easther, Richard |
en |
dc.contributor.author |
Fasiello, M |
en |
dc.contributor.author |
Flauger, R |
en |
dc.contributor.author |
Jr, JTG |
en |
dc.contributor.author |
Hanany, S |
en |
dc.contributor.author |
Knox, L |
en |
dc.contributor.author |
Lim, E |
en |
dc.contributor.author |
McAllister, L |
en |
dc.contributor.author |
Meyers, J |
en |
dc.contributor.author |
Peloso, M |
en |
dc.contributor.author |
Rocha, G |
en |
dc.contributor.author |
Shiraishi, M |
en |
dc.contributor.author |
Sorbo, L |
en |
dc.contributor.author |
Watson, S |
en |
dc.date.accessioned |
2019-09-12T22:20:37Z |
en |
dc.date.issued |
2019-03-12 |
en |
dc.identifier.citation |
Arxiv (1903.04700v1). 12 Mar 2019. 15 pages |
en |
dc.identifier.uri |
http://hdl.handle.net/2292/47671 |
en |
dc.description.abstract |
The next generation of instruments designed to measure the polarization of the cosmic microwave background (CMB) will provide a historic opportunity to open the gravitational wave window to the primordial Universe. Through high sensitivity searches for primordial gravitational waves, and tighter limits on the energy released in processes like phase transitions, the CMB polarization data of the next decade has the potential to transform our understanding of the laws of physics underlying the formation of the Universe. |
en |
dc.relation.ispartof |
Arxiv |
en |
dc.rights |
Items in ResearchSpace are protected by copyright, with all rights reserved, unless otherwise indicated. Previously published items are made available in accordance with the copyright policy of the publisher. |
en |
dc.rights.uri |
https://researchspace.auckland.ac.nz/docs/uoa-docs/rights.htm |
en |
dc.rights.uri |
https://arxiv.org/licenses/nonexclusive-distrib/1.0/license.html |
en |
dc.subject |
astro-ph.CO |
en |
dc.subject |
astro-ph.CO |
en |
dc.subject |
gr-qc |
en |
dc.subject |
hep-th |
en |
dc.title |
Probing the origin of our Universe through cosmic microwave background constraints on gravitational waves |
en |
dc.type |
Report |
en |
dc.rights.holder |
Copyright: The authors |
en |
pubs.author-url |
http://arxiv.org/abs/1903.04700v1 |
en |
pubs.commissioning-body |
National Academies of Science, Engineering and Medicine |
en |
dc.rights.accessrights |
http://purl.org/eprint/accessRights/OpenAccess |
en |
pubs.subtype |
Commissioned Report |
en |
pubs.elements-id |
766316 |
en |
pubs.org-id |
Science |
en |
pubs.org-id |
Physics |
en |
pubs.arxiv-id |
1903.04700 |
en |
pubs.number |
1903.04700v1 |
en |
pubs.record-created-at-source-date |
2019-09-23 |
en |