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Loop corrections to the primordial perturbations Yuko Urakawa (Waseda university) Kei-ichi Maeda (Waseda university) Motivation [Inflation model] Minimally coupled…
rio1.pptUros Seljak, UC Berkeley Rio de Janeiro, August 2014 Outline • Primordial nongaussianity • Introduction and basic physics • CMB temperature power spectrum
PowerPoint PresentationAntony Lewis http://cosmologist.info/ Outline ⇒ ∼ ∫ (, Ω)Ω is statistically isotropic and non-Gaussian Note: statistical anisotropy
Physics of Massive Neutrinos Concha Gonzalez-Garcia PHYSICS OF MASSIVE NEUTRINOS Concha Gonzalez-Garcia ICREA-University of Barcelona YITP-Stony Brook Nufact07 Summer Institute…
PINGU and the Neutrino Mass Hierarchy Ken Clark, Penn State University Neutrinos at the Forefront - Lyon, Oct 2012 Ken Clark - PSU Lyon, Oct 2012 Neutrino Oscillations •…
André de Gouvêa Northwestern The Brave ν World André de Gouvêa Northwestern University University of Mississippi – Colloquium March 18, 2014 March 18, 2014 Brave…
Detection of Ultra-high energy neutrinos The ‘First Light’ of the high energy neutrino astronomy Shigeru Yoshida Department of Physics Chiba University radiation enveloping…
Down-Going UHE Neutrinos In The Pierre Auger Observatory + Neutrino Follow-Up Of GW Michael Schimp on behalf of the Pierre Auger Collaboration October 11 2016 UHE EeV ν…
The sixth Astrophysical Multimessenger Observatory NetworkAMON Workshop May 22, 2019 Detection of supernova neutrinos at Super-Kamiokande 1 M. Nakahata Kamioka Observatory,…
New supernova neutrino spectrum Gleb Sinev LArSoft Coordination Meeting April 12, 2016 2016412 New supernova neutrino spectrum 2 New SNν energy spectrum ● Original spectrum…
Zero Threshold Reactions for Detecting Cosmic Relic Neutrinos R. S. Raghavan Virginia Tech XII Neutrino Telescopes Venice March 9 2007 Be Beginnings: Important influences:…
Why neutrino astronomy? Astrophysical Accelerators Neutrinos allow for observation of ‘hidden regions’ of cosmic accelerators (BH, pulsars, initial epochs of SN explosions).…
Neutrino Overview by a non-expert § Long Range Plan HEPAP 102: Neutrinos listed 3rd after ILC and LHC § Long Range Plan NSAC 402: Recommendation #3 – NUSEL: ββ-decay…
Still Hunting for Primordial Non-Gaussianity: Current Status and Future Prospects Eiichiro Komatsu The University of Texas at Austin Cosmic Microwave Radiation Aspen, January…
NuPRISM 10 m 14m 6 m 10m ν beam Spans many off-‐axis angles to measure many Eν spectra 4% bias in θ23 Improved θ23 Error NuPRISM 10 m 14m 6 m 10m…
sivellink.dk Neutrino Theory and Phenomenology: Lecture I NBIA PhD School: Neutrinos Underground in the Heavens Copenhagen, DK, 2016 Eligio Lisi INFN, Bari, Italy [email protected]…
Results and Prospectives of Reactor Neutrino Experiments Liangjian Wen The 12th particle physics phenomenology workshop PPP12 16-19 May, NCTU, Hsinchu, Taiwan Outline •…
Experimental Approaches to Sterile Neutrinos Using Low Energy Neutrinos Jonathan Link Center for Neutrino Physics Virginia Tech NOW 2012 9/14/12 The LENS-Sterile Proposal…
André de Gouvêa Northwestern 3. Sterile Neutrinos: Theory André de Gouvêa Northwestern University The Allure of Ultrasensitive Experiments V. Neutrinos January 14…
Imrich KRIŠTOF, M.Sc. [email protected] -1- 26.8.2019, Brno “Charm νC and Beauty νB flavour of neutrinos and very probably “colours“ of neutrino resonances and their…