Small dark energy without small parameters

Shlaer, Benjamin

dc.contributor.author	Shlaer, Benjamin	en
dc.date.accessioned	2018-10-08T20:52:25Z	en
dc.date.issued	2017	en
dc.identifier.citation	Arxiv (1706.09415v1) 28 Jun 2017, 5 pages.	en
dc.identifier.uri	http://hdl.handle.net/2292/39552	en
dc.description.abstract	We present a prototype model that resolves the cosmological constant problem using matter alone, i.e., without modifying gravity. Its generic cosmological solutions adjust an arbitrarily large, negative dark energy to a positive value parametrically suppressed by an initial field velocity. Inflationary initial conditions lead to a positive dark energy exponentially smaller in magnitude than any model parameter, or any scale in the initial conditions.	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.title	Small dark energy without small parameters	en
dc.type	Report	en
dc.rights.holder	Copyright: The author	en
pubs.author-url	http://arxiv.org/abs/1706.09415v1	en
dc.rights.accessrights	http://purl.org/eprint/accessRights/OpenAccess	en
pubs.subtype	Working Paper	en
pubs.elements-id	699488	en
pubs.org-id	Science	en
pubs.org-id	Physics	en
pubs.arxiv-id	1706.09415	en
pubs.number	1706.09415v1	en
pubs.record-created-at-source-date	2017-10-24	en