PPT-Did LIGO detect dark matter?

Simeon Bird JHU I Cholis J Munoz Y AliHaimoud M Kamionkowski E Kovetz A Raccanelli A Riess PRL 116 201301 arXiv 160300464 LIGO detected Gravitational Waves LIGO Detection Two merging 30 solar mass BHs. 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.. and Large-Scale Structure. 1. Cora Dvorkin. IAS (Princeton) Harvard (Hubble fellow) . COSMO 2014. August 2014, Chicago. Outline. Dark Matter overview.. Effect of . WIMP Dark Matter . Paul McMillan. Surveys For All, 1st February 2016 . Why do we care?. On the biggest scales, the ΛCDM model works. Why do we care?. On the scale of individual galaxies, agreement is less obvious.. Things are more complicated, we have to consider the baryons. Detecting Einstein’s Elusive Waves. Opening a New Window to the Universe. An Indo-US joint mega-project concept proposal. . IndIGO. Consortium. (. Ind. ian . I. nitiative in . G. ravitational-wave . Cody . Carr. , Minh Nguyen. December 9. th. , 2014.. Agenda. Motivations (Cosmic & Atomic scales). Dark Matter categories. The Dark Matter Zoo. Neutrinos. Neutralinos. Kaluza. -Klein particles. Summary. John . Moffat. Perimeter Institute. Miami 2015 Conference. Fort Lauderdale, December 16, 2015. 2015-12-21. 1. 2. 2015-12-21. 3. https://angel.co/mog. 2015-12-21. Introduction. Observations of the dynamics of galaxies as well as the dynamics. https://www.ligo.caltech.edu/system/video_items/files/4/EinsteinsMessengerLIGO.mp4?1436490806. 2017 Nobel Prize in Physics. : Rainer Weiss - Barry C. . Barish. -Kip S. . Thorne. "for . decisive contributions to the LIGO detector and the observation of gravitational waves". 1 A Brief History of LIGO One hundred years ago, using his recently general relativity theory, Albert Einstein predicted the existence of gravitational waves and described their properties. To Einstei LIGO is an acronym for Laser Interferometer Gravitational-wave Observatory. The word 1ABriefHistoryofLIGOOnehundredyearsagousinghisrecentlygeneralrelativitytheoryAlbertEinsteinpredictedtheexistenceofgravitationalwavesanddescribedtheirpropertiesToEinsteinthesewavesseemedtooweakevertobe Cosmic Opportunities. . –. 45. th. SLAC Summer Institute. Jonathan . Feng. , UC Irvine. 16 August 2017. INTRODUCTION. We’ve learned a lot about the Universe. Dark . Matter: 23% . ± 4. %. Dark . Perimeter Explorations 01. CERN HST2019 . Uniform Circular Motion. Predict. Observe. Explain. How are . mass. and . speed. connected in circular motion?. mass. speed. Uniform Circular Motion. Objective: . Niayesh Afshordi. Western University. Friday, April 13, 2012. “Friday . the 13th. . is a date considered to be bad luck in. . Western. . superstition. .” . -Wikipedia. . Outline. Introduction: Cold Dark Matter (CDM) . Jonah Kanner. , Branson Stephens. , . Michele . Vallisneri. , Alan Weinstein, Roy . Williams. 8/11/14. LOSC. 1. LIGO-. G1400509v4. Why LOSC? . Access data with ease. No need to login to LDAS cluster.