PPT-Cosmological structure formation with negative mass

Giovanni Manfredi Centre National de la Recherche Scientifique Institut de Physique et Chimie des Matériaux de Strasbourg Gabriel Chardin CNRS France Bruce Miller Texas Christian University USA. To understand the formation and evolution of largescale structures we have to introduce inhomogeneities As long as these perturbations remain relatively small we can treat them in perturbation theory In particular we can expand the Einstein equation Topic:. Formation of. gas giant planets. Lecture by: C.P. Dullemond. Two main theories. Gravitational instability of the gas disk. Core accretion scenario. Giant Planet Formation by. Gravitational Instability. Thorsten Naab . MPA, . Garching. . What regulates galaxy formation? . Leiden, April, 22. nd. How do massive galaxies get their gas and stars?. Gas accretion involves dissipation – energy can be radiated away . Leiden Observatory. Sensitive Barometers of Galaxy Formation. Simone . Weinmann. , . Romeel. Dave, . Kristian. . Finlator. , Jason . Tumlinson. , Rob Crain & others. Are Flat or Rising Star Formation Histories in . Galaxies. T.Naab. , P. Johansson, R. . Cen. , K. . Nagamine. , R. . Joung. . and J.P.O.. PPPL:, 19 Dec . 2012. ApJ.L.,. 658,710 . (2007) ApJ.,697, . 38 . (2009). ApJ.L.,699,L178 (. 2009. ). ApJ.,725,2312 . mode of . accretion. in . simulations. of . galaxy. . formation. G. Murante – INAF . OATo. P. Monaco – . Univ. . . Ts. M. Calabrese – SISSA . Ts. G. De Lucia - INAF . OATs. S. . Borgani. – . Chemistry. Ms. Pollock. 2013 - 2014. Introduction. Dalton’s atomic theory very good but not entirely correct. Atoms able to be broken into smaller particles. Electrons, Protons, and Neutrons. Electrons. below. ); this qualitative behavior is seen for all feedback models and mass ranges. details will depend on UV background. The Simulated Circumgalactic Medium at z∼2. . Molly . S. . Peeples . (CGE Fellow; UCLA). naturalness and . supersymmetry. Natsumi. Nagata. E-ken Summer school. September 04, 2012. Task. 発表は、. M. １にも分かる内容を混ぜつつ、新しい内容まで発表することが目標です。. The Last Epoch Cosmic Structure Formation Today we have a matter-dominated universe ruled by the force of gravity. Slight variations in density produces formation regions for stars and galaxies. 1 st with Marco Lombardi, . Joao Alves, . Jan Forbrich, . Gus Munch. Kevin Covey. & Carlos Roman . z = 1 - 10. Bouwens et al. 2010. z = 0.000. S. Guisard ESO. Pipe Nebula. in . simulations. of . galaxy. . formation. G. Murante – INAF . OATo. P. Monaco – . Univ. . . Ts. M. Calabrese – SISSA . Ts. G. De Lucia - INAF . OATs. S. . Borgani. – . Univ. . . Ts. K. . Zooming in on Star Formation. , Nafplio, June 14. , 2019. Galactic Scale Star Formation. What we know for sure now:. Feedback, and vertical pressure (. im. -)balance is crucial. The role of radial and vertical net mass transport is poorly understood. Pilechian. 99.12.18. R. eferral . to an endocrinology clinic for re-examination of . adrenal . masses . A 50-year-old woman . known . case . of . HTN . (for . 10 . years. ). , . who has had recurrent episodes of muscle weakness since that time, as it happened about once a month, lasted 24 hours and resolved spontaneously.