PPT-Microlensing Theory and Observables

Yossi Shvartzvald NPP Fellow JPL Microlensing Geometry       Microlensing Geometry           Microlensing Geometry           Microlensing Geometry. NON-COMMUTATIVE GEOMETRY. P.A. . Marchetti. Universita. ’ . di. . Padova. SISSA 2011. P.A. M., R. . Rubele. , Int. Jour. . Theor. . Phys. 46 (2007) 49. Underlying idea. To a physical system it is intrinsically and not “a priori” associated a “logic” of the propositions concerning its properties. Technical Track Session VI. This material constitutes supporting material for the "Impact Evaluation in Practice" book. This additional material is made freely but please acknowledge its use as follows: . David . Bennett. University of Notre Dame. WFIRST. Unique Science from Space-based Survey. Exoplanet Survey Question #1: How do planetary systems form and evolve?. complementary to . Kepler. Exoplanet sensitivity down to sub-Earth masses at 0.5 AU - ∞. of . the Standard . Model after . the discovery of an SM-like scalar boson. Andreas Hoecker (CERN). Solvay . workshop . “. Facing . the Scalar . Sector. ”, . May . 29. -. 31, . 2013 . Introduction. for Measurements of. . G. eneralized . P. arton . D. istributions. e. +. @ . JLab. Generalized . parton. distributions. Polarized positron production. Polarization transfer physics. . PEPPo. Figure of Merit . David . Bennett. University of Notre Dame. WFIRST. WFIRST Microlensing Figure of Merit. Primary FOM1 - # of planets detected for a particular mass and separation range. Cannot be calculated analytically – must be simulated. Antony Lewis. http://cosmologist.info/. Lewis . arXiv:1204.5018. see also . Creminelli. . et al . astro-ph. /0405428, . arXiv:1109.1822, . Bartolo. et al arXiv:1109.2043. Lewis . arXiv:1107.5431. Lewis. Irakli Garishvili. G. roup members: Ron . Soltz. , Betty . Abelev. , Andy Glenn. 29. th. Winter Workshop in. Nuclear Dynamics. Motivation . A. chieved a very good qualitative understanding of the full picture of heavy ion collisions at RHIC and LHC. in Globular Clusters. Margarita . Safonova. . Ancient Greeks knew that light travels in a straight line... Or you wouldn’t be able to cross the road!. Gravitational . Lensing. —. Astronomical Mirages. J.T. . Hoeksema, J. . Schou. , S. . Couvidat. , R.S. Bogart, R.I. Bush, T.L. Duvall, Jr., Y. Liu, A.A. Norton, and P.H. Scherrer. The . Helioseismic. and Magnetic Imager (HMI) acquires sequences of polarized . The Ohio State University. (with the WFIRST SDTs and on behalf of the WFIRST . μSIT. ). Completing the Census of . Exoplanetary. Systems . with WFIRST.. 21. st. International . Microlnesing. Conference. C249: Planetary Astrophysics. September 6, 2017. What does a microlensing event look like?. Gaudi 2012. What are caustics?. Gaudi 2012. s = instantaneous projected separation of star & planet (in Einstein radii). J.T. . Hoeksema, J. . Schou. , S. . Couvidat. , R.S. Bogart, R.I. Bush, T.L. Duvall, Jr., Y. Liu, A.A. Norton, and P.H. Scherrer. The . Helioseismic. and Magnetic Imager (HMI) acquires sequences of polarized . David A. Kosower. Institut. de Physique . Th. é. orique. , CEA–. Saclay. work with. Ben . Maybee. and . Donal. O’Connell (Edinburgh). [arXiv:1811.10950];. by. Ben . Maybee. , . Donal. O’Connell, and Justin Vines [1906.09260].