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Neutron Physics at the Precision Frontier Susan Gardner Fermi National Accelerator Laboratory Batavia, IL 60510 USA Department of Physics and Astronomy∗ University of Kentucky…
Dark photon manifestation in the tripletlike QED processes γ + `i → `+j `−j + `i i 6= j i = e µ j = e µ τ G I Gakh∗ National Science Centre Kharkov Institute of…
1 The electron is a photon around Dark Matter Adrian Ferent I discovered a new Gravitation theory which breaks the wall of Planck scale! Abstract My Nobel Prize - Discoveries…
Spectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy 172 2017 109–114 Contents lists available at ScienceDirect Spectrochimica Acta Part A: Molecular and…
Image: Navarro et al. The Physics of Fine Tuning June, 2017 Rocky Kolb University of Chicago Dark Matter Shapes the Universe Dark Matter: 25% Dark Energy: 70% Stars: 0.8%…
Decaying vs Annihilating Dark Matter in Light of a Tentative Gamma-Ray Line Mathias Garny DESY Hamburg, Germany TUM, 05.07.12 based on arXiv:1206.7056 with Wilfried Buchmüller…
De Viveiros - Brown University April 2009 v07 FCT - Universidade de Coimbra - Café com Física Luiz de Viveiros Brown University – Physics Department Searching for Dark…
Slide 1 Testing the Equivalence Principle for Dark Matter Using Tidal Streams Michael Kesden, CITA Collaborator: Marc Kamionkowski, Caltech COSMO ‘06 Tahoe City, CA Thursday,…
Solvay Inst Brussels 5 April 2019 Chris Kouvaris Dark Stars Dark Matter and Black Holes Why Dark Matter Self-Interactions Problems with Collisionless Cold Dark Matter •…
From the Motion Picture “The Dark Knight” A DARK KNIGHT Original Score by Hans Zimmer and James Newton Howard Arranged by Connor Griffin & & B ? ? ? ÷ 4 4 4…
A Study of In-Situ Multilayer Tape Casting Ba3Ca1.18 Nb1.82O9-δ Membrane for Proton Conducting Solid Oxide Fuel CellNb1.82O9-δ Membrane for Proton Conducting
Dark Matter Dark Matter Cryogenic Detectors Direct Dark Matter Search Dark Matter Matter in the Universe - Composition ‘ν too light‘ = most of the Dark Matter is cold…
Jennifer Gaskins GRAPPA, University of Amsterdam Indirect dark matter searches: recent results and excitement Dark matter vs MOND Crete May 22, 2015J. Gaskins How to detect…
Star formation Star Formation in the Early Universe: Population III stars Redshift Age of the Universe and Lookback time The ΛCDM Model WMAP ● Flat Universe ● H0 = 73kmsMpc…
WIMP Dark Matter Searches with Liquid Xenon and Liquid Argon Detectors Elena Aprile Columbia University TeVPA08 Beijing, September 27, 2008 Principle of Direct Detection…
vikhlinin-chandra10.keyA.VIKHLININ Detailed properties: Chandra & XMM Cluster physics: Chandra & simulations • Direct observational constraints on ICM physics
WIMP Dark Matter Searches with Liquid Xenon and Liquid Argon Detectors Elena Aprile Columbia University TeVPA08 Beijing, September 27, 2008 Principle of Direct Detection…
Hadronic matrix elements for Dark Matter and other searches Laurent Lellouch CPT Marseille CNRS Aix-Marseille U. Budapest-Marseille-Wuppertal collaboration BMWc Phys.Rev.Lett.…
Stau Pair Production At The ILC Tohoku University – Senior Presentation Tran Vuong Tung e+ e - Z*γ τ τ+ –1– Outline Introduction of the International Linear Collider…
L’UNIVERSO OSCURO Aldai 27 novembre 2018 Le certezze dell’ Ottocento • Spazio e Tempo Universale e assoluto • Materia ed Energia distinti componenti dell’ Universo…