'Sterile neutrino' presentation slideshows

Neutrinos and the stars

Neutrinos and the stars. Supernova Neutrinos. Georg Raffelt, MPI for Physics Lectures at the Topical Seminar Neutrino Physics & Astrophysics 17 - 21 Sept 2008, Beijing, China. Sanduleak - 69 202. Supernova 1987A 23 February 1987. Tarantula Nebula. Large Magellanic Cloud Distance 50 kpc

905 views • 72 slides

A. Yu. Smirnov

Sterile neutrinos:. searches & implications. A. Yu. Smirnov. International Centre for Theoretical Physics, Trieste, Italy. Planck 2011, May29, Lisbon. Sterile neutrino. n s. Light. No weak interactions: - singlets of the SM symmetry group. RH - components of neutrinos.

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3+1 sterile neutrino @NuFact

569 views • 44 slides

3+1 sterile neutrino @NuFact

448 views • 44 slides

Neutrino Oscillation

Neutrino Oscillation. Hitoshi Murayama (Berkeley) PRC-US Meeting @ IHEP June 12, 2006. Outline. Past: Why Neutrinos? Present: Era of Revolution Future Conclusion. Past. Why Neutrinos?. Interest in Neutrino Mass. So much activity on neutrino mass already. Why am I interested in this?

742 views • 43 slides

Constraints on Neutrino Physics from Cosmology

375 views • 37 slides

Asking for Directions in Ireland... Continuing the Hunt for the Sterile Neutrino

454 views • 36 slides

MATTEO VIEL

NEUTRINOS FROM THE LYMAN- a FOREST: MYTH or REALITY ?. Trieste. MATTEO VIEL. OUTLINE. - What is the Lyman- a forest ? Is it a cosmological probe ? - Constraints on sterile neutrinos - Constraints on active neutrinos.

450 views • 32 slides

Visible and Invisible Universe: A short commentary

Visible and Invisible Universe: A short commentary. Carlo Rubbia CERN Geneva, Switzerland and INFN/LNGS, Assergi, Italy.

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Light Sterile Neutrinos: The Evidence Jonathan Link Center for Neutrino Physics Virginia Tech

Light Sterile Neutrinos: The Evidence Jonathan Link Center for Neutrino Physics Virginia Tech HQL 2012 6/12/12. Sterile Neutrinos. A sterile neutrino is a lepton with no ordinary electroweak interaction except those induced by mixing. Phys.Rept. 427, 257 (2006). Active neutrinos:

413 views • 30 slides

Reactor Antineutrino Anomaly

Reactor Antineutrino Anomaly. E.A. McCutchan , A.A. Sonzogni , T.D. Johnson National Nuclear Data Center. Anti-neutrinos from reactors. Daya Bay. Detection through inverse ? decay on proton. Principal Contributors. 235 U, 238 U, 239 Pu, 241 Pu.

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Does current data imply a Baroque neutrino sector?

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Light Sterile Neutrinos: The Evidence Jonathan Link Virginia Tech

Light Sterile Neutrinos: The Evidence Jonathan Link Virginia Tech Workshop on Neutrinos at the SNS Oak Ridge National Lab 5/2/12. Outline. Sterile Neutrinos in Theory and Phenomenology Evidence from Particle Physics Evidence from Cosmology Proposed Future Experiments.

400 views • 25 slides

The Detection of an Unexplained Emission Line at 3.56 keV

The Detection of an Unexplained Emission Line at 3.56 keV. Esra Bulbul Harvard-Smithsonian Center for Astrophysics. Maxim Markevitch (NASA/GSFC), Adam Foster ( CfA ), Randall Smith ( CfA ), Mike Loewenstein ( NASA/GSFC) , and Scott Randall ( CfA ).

351 views • 25 slides

The n MSM

The n MSM. Takehiko Asaka (Tohoku University). -- Neutrino Masses and Dark matter --. TA, S.Blanchet, M.Shaposhnikov [hep-ph/0503065] TA, M.Shaposhnikov [hep-ph/0505013]. Neutrino oscillations. The MSM contradicts with n oscillation experiments!!

369 views • 24 slides

Reactor antineutrino physics with DANSS experiment Igor Alekseev*

ITEP, Moscow. Reactor antineutrino physics with DANSS experiment Igor Alekseev* for the DANSS collaboration: ITEP(Moscow) + JINR(Dubna) *ITEP ( Alikhanov Institute for Theoretical and Experimental Physics ).

251 views • 24 slides

Suzaku search for evidence of sterile neutrinos in the X-ray spectra of dwarf spheroidal galaxies

Suzaku search for evidence of sterile neutrinos in the X-ray spectra of dwarf spheroidal galaxies. Michael Loewenstein, Alexander Kusenko (UCLA), Peter Biermann (MPIfr, UAla). Meet the Sterile Neutrino.

376 views • 22 slides

The first stars formation in warm dark matter model

The first stars formation in warm dark matter model. Liang Gao National Observatories, China. Outline . Why is WDM still interesting? 1 st stars WDM. Why warm dark matter?. Small scale power spectrum of Universe is poorly constrained, so why not?

294 views • 17 slides

Facility for exquisite precisions

Facility for exquisite precisions. K. Long and E. Wildner. Daya Bay & Reno results: CPV discovery conceivable; emphasizes control of systematics critical Scientific priorities: MH; CPV; Precision measurement; Gamma=100, Beta beam plus SPL/ Frejus super-beam:

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Abstract

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