PDF-You’ll be aware that all matter in the universe are made up of
Author : myesha-ticknor | Published Date : 2016-05-10
Antimatter atoms which in turn are made out of particles like protons neutrons and electrons However you might not have known that each of these particles has
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You’ll be aware that all matter in the universe are made up of: Transcript
Antimatter atoms which in turn are made out of particles like protons neutrons and electrons However you might not have known that each of these particles has a corr esponding antiparticle. Expanding Universe – consistent w/ a Big Bang?. Olber’s Paradox. Large Scale Structure and relation to Dark Matter. Evidence for the Big Bang. The Cosmic Microwave Background. The abundances of the elements. Sections 37.4 – 37.5. Reminders. Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test.. LAB B2-WNL: . Wave Nature of Light . due Friday @ 4pm.. Weekly Reflection #13 will be sent out after class today; due Tuesday evening after fall break.. Secs. 37.1-37.3. Reminders. Lab . D1-LFA: . Light from Atoms . due Friday @ 4 (this will be the last lab for the semester). In-class Quiz #6 Thursday, November 20???. Keep, reschedule, or delete . will address chapter 37 only. 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.. Cosmology and Inflationary Theory. Chad A. . Middleton. Mesa . State . College. Physics Seminar. February 18, 2010. Cosmology. is the scientific study of the large scale properties of the Universe as a whole.. :. Dark Matter & Dark Energy. WWK: Students will understand the theories of Dark Matter & Dark Energy and how they’re thought to affect the Universe. .. Dark Matter. Dark Matter . - . matter that influences the evolution of the universe . The Universe is commonly defined as the totality of existence, including planets, stars, galaxies, the contents of intergalactic space, the smallest subatomic particles, and all matter and energy. . Similar . Dark Energy and Dark Matter. Prof. Lawrence Wiencke. Department of Physics Engineering. Colorado School of Mines. Nov 9 2011. The Dark . Side. 95% of the. Universe Is Dark!. Energy budget of Universe. Prepared a presentation. Teacher of English. Anisova. Julia . Vladimirovna. The Big Bang. Most astronomers believe the Universe began in a Big Bang about 14 billion years ago. At that time, the entire Universe was inside a bubble that was thousands of times smaller than a pinhead. . Unit 1 – Area of Study 3. What do you know?. Outcome. : On . completion of this unit the student should be able explain the origins of atoms, the nature of subatomic particles and how energy can be produced by atoms. DARK MATTER &DARK ENERGY. We know about only normal matter which is only 5% of the composition of universe and the rest is . DARK MATTER & DARK ENERGY. DARK MATTER. The universe is the sum of all energy, matter, space and time.. But there. ’. s a difference between the universe we see (the observable universe) . and the universe as it really exists.. This gets complicated….. The time since the beginning of the universe is 1/H years or about 13.8 billion years.. The Big Bang started off immensely hot!. Radiation dominated the early universe.. Matter dominance occurs after radiation “cools” enough for matter to condense per the relationship E=mc. Dynamics. of. FRWL Universes. . Dynamics. FRW Universe. Friedmann-Robertson-Walker-Lemaitre Universe. . Cosmic Constituents:. Evolving Energy Density . . FRW Energy Equation. To infer the evolving energy density .
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