'Baryonic matter' presentation slideshows

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(It really does) Matter and its Phases

(It really does) Matter and its Phases

(It really does) Matter and its Phases. Dr. Anti-Matter Hazlett MHS. Inertia. To understand matter – you need to understand the concept of inertia This is the force(s) that keep something in rest The idea is based on energy This energy is divided into Kinetic and Potential

By bess
(152 views)

Low- frequency radio maps for the REXCESS cluster sample

Low- frequency radio maps for the REXCESS cluster sample

Low- frequency radio maps for the REXCESS cluster sample . S.R. Heidenreich, University of Southampton In collaboration with J.H. Croston, University of Southampton;

By luann
(54 views)

Masayasu Harada (Nagoya Univ.)

Masayasu Harada (Nagoya Univ.)

Effects of vector – axial-vector mixing to dilepton spectrum in hot and/or dense matter . Masayasu Harada (Nagoya Univ.). @KEK 理論センター 研究会 「 原子核・ハドロン物理 」 (August 11, 2009). based on M.H. and C.Sasaki , arXiv:0902.3608

By dermot
(109 views)

Dark Universe or twisted Universe? Einstein- Cartan theory.

Dark Universe or twisted Universe? Einstein- Cartan theory.

Dark Universe or twisted Universe? Einstein- Cartan theory. Thomas Schucker : CPT Marseille France Andre Tilquin : CPPM Marseille France THCA Tsinghua China \. arXiv:1104.0160. arXiv:1109.4568. Preliminary. References.

By heath
(404 views)

Symmetry energy   in the era of advanced gravitational wave detectors

Symmetry energy   in the era of advanced gravitational wave detectors

Heavy Ion Meeting 20313-05 , Asan Science Hall, Korea University, May 24 2013. Symmetry energy   in the era of advanced gravitational wave detectors. Hyun Kyu Lee Hanyang University. 0. Introduction. Temperature frontier. Density frontier. High baryon number density .

By lynn
(98 views)

D.S. Hajdukovic GBAR Collaboration Meeting 18 th April 2012

D.S. Hajdukovic GBAR Collaboration Meeting 18 th April 2012

Quantum vacuum and the gravitational repulsion between matter and antimatter: a key for the understanding of the Universe?. D.S. Hajdukovic GBAR Collaboration Meeting 18 th April 2012. Our best physics The Standard Model of Particles and Fields + General Relativity

By mahsa
(153 views)

Kati Nikolics

Kati Nikolics

The DARK MATTER Mystery. Kati Nikolics. Contents. Evidence for the existence of DM Properties Possible Candidates - Theoretical Models Requirements for experimental detection Trying to find the cosmic needle in a haystack: DEAP. …dark traces in the Universe…. F. Zwicky 1933:

By mircea
(128 views)

Wide-field Weak Lensing Mass Reconstructions of Merging Galaxy Clusters

Wide-field Weak Lensing Mass Reconstructions of Merging Galaxy Clusters

Introduction. Abell 1758. Wide-field Weak Lensing Mass Reconstructions of Merging Galaxy Clusters. Brett Ragozzine, Douglas Clowe Ohio University, Department of Physics & Astronomy, Athens, OH 45701.

By enid
(142 views)

Public Star Party

Public Star Party

Public Star Party. Organized by Institute for Astronomy, University of Hawaii. Contact person: Prof. Jim Heasley. When? Tonight between 8:30 and 10 pm Where? Kapiolani Park, Honolulu How to get there? Intersection Paki Avenue with Noela Street What about the weather? Check 956-6195.

By solada
(78 views)

The Compressed Baryonic Matter Experiment at FAIR

The Compressed Baryonic Matter Experiment at FAIR

The Compressed Baryonic Matter Experiment at FAIR. Peter Senger, GSI Bergen, April 3, 2005. Outline:  Physics case  Detector requirements  Feasibility studies  Detector R&D  Outlook. The future Facility for Antiproton an Ion Research (FAIR).

By deo
(161 views)

Welcome to Stars, Galaxies, and the Universe Fall 2010

Welcome to Stars, Galaxies, and the Universe Fall 2010

Welcome to Stars, Galaxies, and the Universe Fall 2010. Initial pleasantries, who I am, who you are This should be the most interesting course you take in college. Welcome to Stars, Galaxies, and the Universe Fall 2010. Initial pleasantries, who I am, who you are

By jenis
(77 views)

GALAXY FORMATION AND EVOLUTION - 2

GALAXY FORMATION AND EVOLUTION - 2

GALAXY FORMATION AND EVOLUTION - 2. DISCOVER Magazine’s 2007 Scientist of the Year. David Charbonneau, of the Harvard-Smithsonian Canter for Astrophysics (CfA), for his studies of alien worlds, in search of Earth-like planets, and the possibility that they may be hosting life.

By brynne-vang
(197 views)

The Compressed Baryonic Matter Experiment at FAIR

The Compressed Baryonic Matter Experiment at FAIR

The Compressed Baryonic Matter Experiment at FAIR. Peter Senger Seoul, April 21, 2005. Outline:  Physics case  Feasibility studies and Detector R&D  Outlook. The future Facility for Antiproton an Ion Research (FAIR). Primary beams: 10 12 /s 238 U 28+ 1-2 AGeV

By pfolse
(0 views)

More buzz words, etc.  Structure evolution and types of WIMPS

More buzz words, etc. Structure evolution and types of WIMPS

More buzz words, etc. Structure evolution and types of WIMPS Bottom-up <=> Cold Dark Matter (CDM) Top-Down <=> Hot Dark Matter (HDM) “Cold” = “slow” = less then 1/10 speed of light “Hot” = “fast” = 0.99 or closer to speed of light

By elizabethcsmith
(0 views)


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