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PRODID:UW-Madison-Physics-Events
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UID:UW-Physics-Event-2294
DTSTART:20111108T220000Z
DURATION:PT1H0M0S
DTSTAMP:20260420T113918Z
LAST-MODIFIED:20111025T142103Z
LOCATION:Chamberlin 5280
SUMMARY:Massive gravitons and enhanced gravitational lensing\, Theory 
 Seminar (High Energy/Cosmology)\, Mark Wyman\, University of Chicago
DESCRIPTION:The mystery of dark energy suggests that there is new grav
 itational physics at low energies and on long length scales. On the ot
 her hand\, low mass degrees of freedom in gravity are strictly limited
  by observations within the solar system. A compelling way to resolve 
 this apparent contradiction is to add  a galilean-invariant scalar fie
 ld to gravity. Called galileons\, these scalars have strong self inter
 actions near overdensities\, like the solar system\, that suppress the
 ir effects on the motion of massive particles.  These non-linearities 
 are weak on cosmological scales\, permitting new physics to operate. E
 xtending galilean invariance to the coupling of galileons to stress-en
 ergy -- as was first done in the case of massive gravity -- can have a
  surprising phenomenological consequence: enhanced gravitational lensi
 ng.  Weak lensing observations will be able to detect or constrain out
  this effect\, which is not well described by existing model independe
 nt tests of GR.<br>
URL:https://www.physics.wisc.edu/events/?id=2294
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