TY  - CONF
AU  - Weltman, A.
TI  - Chameleon Fields Near and Far
IS  - DESY-PROC-2013-04
CY  - Hamburg
PB  - Verlag Deutsches Elektronen-Synchrotron
M1  - PUBDB-2018-02827
M1  - DESY-PROC-2013-04
SN  - 978-3-935702-83-6
T2  - DESY-PROC
SP  - 271-276
PY  - 2013
AB  - In this presentation we contemplate the problem of dark energy and advocate for a multi-faceted approach to studying its solution. Indeed it may be that, like the philosophers described above, we too cannot understand the nature of our beast by only touching one side of the problem. In particular we will study chameleon fields as a candidate for driving the observed acceleration of the universe and we will look how to test this theory through a varied approach as advocated here.
T2  - 9th Patras Workshop on Axions, WIMPs and WISPs
CY  - 24 Jun 2013 - 28 Jun 2013, Mainz (Germany)
Y2  - 24 Jun 2013 - 28 Jun 2013
M2  - Mainz, Germany
KW  - Hypothetisches Teilchen (gnd)
LB  - PUB:(DE-HGF)29 ; PUB:(DE-HGF)8 ; PUB:(DE-HGF)7
DO  - DOI:10.3204/DESY-PROC-2013-04/weltman_amanda
UR  - https://bib-pubdb1.desy.de/record/408374
ER  -