% IMPORTANT: The following is UTF-8 encoded.  This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.

@INPROCEEDINGS{Mantry:315513,
      author       = {Mantry, Sonny and Pitschmann, Mario and Ramsey-Musolf,
                      Michael J.},
      title        = {{D}ifferences between {A}xions and {G}eneric {L}ight
                      {S}calars in {L}aboratory {E}xperiments},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2016-05920},
      isbn         = {978-3-935702-59-1},
      series       = {DESY-PROC},
      pages        = {102-107},
      year         = {2014},
      comment      = {Mantry, Sonny "Differences between Axions and Generic Light
                      Scalars in Laboratory Experiments" in Proceedings, 10th
                      Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014)
                      / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag
                      Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 :
                      10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29
                      - 2014-07-04, Geneva},
      booktitle     = {Mantry, Sonny "Differences between
                       Axions and Generic Light Scalars in
                       Laboratory Experiments" in Proceedings,
                       10th Patras Workshop on Axions, WIMPs
                       and WISPs (AXION-WIMP 2014) /
                       Tsesmelis, Emmanuel, Maroudas, Marios
                       (eds.), Verlag Deutsches
                       Elektronen-Synchrotron : 2014 ;
                       AXION-WIMP 2014 : 10th Patras Workshop
                       on Axions, WIMPs and WISPs, 2014-06-29
                       - 2014-07-04, Geneva},
      abstract     = {It is well-known that electric dipole moment (EDM)
                      constraints provide the most stringent bounds on
                      axion-mediated macroscopic spin-dependent (SD) and time
                      reversal and parity violating (TVPV) forces. These bounds
                      are several orders of magnitude stronger than those arising
                      from direct searches in fifth-force experiments and
                      combining astrophysical bounds on stellar energy loss with
                      $E\"otv\"os$ tests of the weak equivalence principle (WEP).
                      This is a consequence of the specific properties of the
                      axion, invoked to solve the Strong CP problem. However, the
                      situation is quite different for generic light scalars that
                      are unrelated to the strong CP problem. In this case, bounds
                      from fifth-force experiments and astrophysical processes are
                      far more stringent than the EDM bounds, for the mass range
                      explored in direct searches.},
      month         = {Jun},
      date          = {2014-06-29},
      organization  = {10th Patras Workshop on Axions, WIMPs
                       and WISPs, Geneva (Switzerland), 29 Jun
                       2014 - 4 Jul 2014},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2014-03/mantry_sonny},
      url          = {https://bib-pubdb1.desy.de/record/315513},
}