PPT-Cosmological Information

Ue Li Pen Tingting Lu Olivier Dore Cosmological Errors How do we know errors on measurement and theory For Gaussian field Pk is 2PCF its error Fisher is 4PCF and the error on Fisher is 8PCF. 郭宗寛 . (. Zong-Kuan. . Guo. ). ITP. , . CAS. 3rd . Joint Retreat on Cosmology and LHC . Physics. November 2, 2012. Based on . collaboration . with . D.J. . . Schwarz. Phys. . Rev. D 80 (2009) 063523 [arXiv:0907.0427. 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 . Lecture 4: The extragalactic distance scale. Prof.. . Dr.. M. Baes (. UGent. ). Prof.. . Dr.. C. . Waelkens. (KUL). Academic year 2015-2016. The expanding Universe. One of the most important cosmological discoveries: . God: What We’re Not Talking About. God: What We Are Talking About. The arguments for & against the existence of a supernatural . Force.. Being.. I. ntelligence.. Designer.. Cause.. Logical and/or physical necessity.. This . powerpoint. will show you the basics of dark matter and dark energy . Their place in the universe . By Jordan . Ilori. . DARK MATTER. Dark matter is a type of matter hypothesized in astronomy and cosmology to account for a large part of the mass that appears to be missing from the universe. Dark matter cannot be seen directly with telescopes; evidently it neither emits nor absorbs light or other electromagnetic radiation at any significant level. Instead, the existence and properties of dark matter are inferred from its gravitational effects on visible matter, radiation, and the large-scale structure of the universe. According to the Planck mission team, and based on the standard model of cosmology, the total mass–energy of the known universe contains 4.9% ordinary matter, 26.8% dark matter and 68.3% dark energy. Thus, dark matter is estimated to constitute 84.5% of the total matter in the universe and 26.8% of the total content of the universe.. PHIL/RS 335. Going back to the beginning.. The cosmological argument has its origin in Ancient Greek Philosophy.. We see versions of the argument in the work of both Plato and Aristotle.. There, of course, the argument was not aimed at proving the existence of a theistic divinity, but at explaining the origin of the world.. 
       sion as a superdense state in the beginning ofthe Universe, for now they couldclaim that the biblical account ofcreation is right, and Bishop Usher was mis-tak Thomas Krühler (DARK). Thanks to J. . Fynbo. , D. . Malesani. , J. . Hjorth. ,. J. Greiner, D. A. . Kann. , D. . Perley. , N. . Tanvir. , . S. . Klose. and many others. Very High Energy Phenomena in the . History and Present Status. . Motivated by . the book. :. Breakthrough Beyond the Edge of the World. Valery . Rubakov. Alexei . Starobinsky. Andrei . Linde. Vyacheslav. . Mukhanov. Vladimir . Lukash. What is the Cosmological argument?. Cosmological: Referring to the origin and structure of the universe.. The cosmological argument tries to prove that there is a perfect and well ordered universe, and a world in which we live (cosmos), rather than nothingness, because God brought the cosmos into existence. Theists argue that the universe is perfect because it was created by God and is not the result of random chance (the big bang theory).. Astronomy 123. Cosmology. Cosmology is the empirical study of the organization, structure and evolution of the Universe. At any given time we always think our Cosmology is correct: . Ancient: Earth is at center of Universe. a. nd . Synchrotron . Emission. Dongsu. . Ryu. (CNU), . Magnetism Team . in Korea. Magnetic fields in the intergalactic space. c. lusters of. galaxies:. B ~ a few . m. G. filaments of. galaxies:. Alexander . Polnarev. QMUL, School of Physics and Astronomy, London, UK. Tarusa. , 10 September 2015. Talk Overview:. Introduction: . Free electrons + Anisotropy = Polarization. The History of Polarization in Cosmology: . Clare Burrage . University of Nottingham. What is dark energy . and how do we find it?. Clare Burrage. University of Nottingham. Outline:. Accelerated expansion and the cosmological constant. Dark energy, scalar fields, and fifth forces.