'Neutrino masses' presentation slideshows

Matter, Energy, Space and Time: Particle Physics in the 21st Century

Matter, Energy, Space and Time: Particle Physics in the 21st Century. Jonathan Bagger May 8, 2003. A Century of Physics. The 20th century witnessed the triumph physics From the discovery of the electron and the nucleus To the development of relativity and quantum mechanics

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Neutrino Masses and the Quest for Unification

Neutrino Masses and the Quest for Unification. K.S. Babu Oklahoma State University. Physics Seminar Wichita State University, Wichita, KS November 6, 2013. Cosmic Gall Neutrinos, they are very small. They have no charge and have no mass And do not interact at all.

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Masato Yamanaka (Saitama University)

Universal Extra Dimension models with right-handed neutrinos. Masato Yamanaka (Saitama University). collaborators. Shigeki Matsumoto Joe Sato Masato Senami. Phys.Lett.B647:466-471 and. Phys.Rev.D76:043528,2007. Introduction. What is dark matter ?.

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Seesaw 25

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MASSIVE NEUTRINOS AND COSMOLOGY

MASSIVE NEUTRINOS AND COSMOLOGY. ?. Sergio Pastor (IFIC). CuTAPP 2005, Ringberg Castle. Outline. Neutrinos as DM. Effect of neutrino mass on cosmological observables. Current bounds and future sensitivities. Neutrinos decoupled at T~MeV, keeping a

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452 views • 31 slides

Neutrinoless double beta decay and Lepton Flavor Violation

Neutrinoless double beta decay and Lepton Flavor Violation. Or, in other words, how the study of LFV can help us to decide what mechanism is responsible for the 0 nbb decay if it is ever observed. Petr Vogel, Caltech Erice, 9/20/2005. Based on

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Common problem against B and L genesis and its possible resolution M. Yoshimura

Common problem against B and L genesis and its possible resolution M. Yoshimura. Introduction 3 conditions for B asymmetry generation Sources of B non-conservation at finite T GUT, electroweak ?? Scenario of original B-genesis ?? Thermal L-genesis and general remarks

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Neutrinos at LHC Results from CMS

Neutrinos at LHC Results from CMS. Andrea Gozzelino (University of Padova and INFN LNL) on behalf of CMS Collaboration. Outlines. Neutrinos parameters Seesaw mechanism LHC performance CMS physics objects Type I fermionic isospin singlets Type II scalar triplets

367 views • 27 slides

Neutrino Physics

Neutrino Physics. José Bernabéu IFIC-University of Valencia December 2007. Neutrino Physics. History and Interest First evidence of neutrino masses Origin of masses? - Experiment - Beyond Standard Model Dimension 5: Majorana ’s Grand Unification Scale: See-saw Leptogenesis

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NEUTRINOLESS DOUBLE BETA DECAY ANGULAR CORRELATION AND NEW PHYSICS

NEUTRINOLESS DOUBLE BETA DECAY ANGULAR CORRELATION AND NEW PHYSICS. Dmitry Zhuridov Particles and Fields Journal club Department of Physics National Tsing Hua University. The talk is based mostly on the paper: Probing new physics in the neutrinoless double beta decay

411 views • 26 slides

Large Theta(13) From Minimal SO(10) Unification

Large Theta(13) From Minimal SO(10) Unification. K.S. Babu Oklahoma State University. ICHEP 2012 Melbourne , July 4-11, 2012. Outline. Recent Results on Theta(13). Daya Bay. RENO. Global Fit to Neutrino Oscillations. Forero, Tortola, Valle, 2012.

334 views • 25 slides

NEUTRINO MASSES, LEPTOGENESIS, DARK MATTER, etc.

NEUTRINO MASSES, LEPTOGENESIS, DARK MATTER, etc. Dmitry Zhuridov ( NTHU, Hsinchu) The Chung-Yuan Christian University HEP Seminar Chungli, November 10, 2009. In collaboration with: Chao-Qiang Geng (NTHU) Chuan-Hung Chen (NCKU & NCTS). Outline. Brief introduction and motivation.

338 views • 25 slides

Calculation of absolute neutrino masses in the seesaw extension

Calculation of absolute neutrino masses in the seesaw extension. D . J ur ?iukonis , T. Gajdosik and A. Juodagalvis. Vilnius University , Institute of Theoretical Physics and Astronomy. Content. Seesaw mechanism One-loop corrections Case n R = 1 Case n R = 2 Conclusions.

487 views • 24 slides

Double Beta Decay What if we see it?

Double Beta Decay What if we see it?. Steve Elliott. Outline. Physics/Technical Goals Experimental Uncertainties NEMO/SuperNEMO Sean Sutton had to cancel. Sasha Barabash is here for discussion. KKDC Claim. 50 meV Or ~ 10 27 yr. Atmospheric Scale. Inverted. Solar Scale. Normal.

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TexPoint fonts used in EMF.

TexPoint fonts used in EMF. Read the TexPoint manual before you delete this box.: A A A A A A A A. Dark Matter Shining Light - Gravitino Dark Matter and R-parity Violation. Are R. Raklev University of Cambridge In collaboration with Magda Lola (Patras) and Per Osland (Bergen).

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ICFA Seminar Matrix Summary October 6, 2011

ICFA Seminar Matrix Summary October 6, 2011. Hugh Montgomery Jefferson Lab. The Frontier Convention. Energy Frontier Intensity Frontier Cosmic Frontier Note that when funding agencies put us in boxes, we object. Even when we choose the boxes ourselves the boundaries are not perfect.

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New aspects of leptogenesis

Cosmo 08 August 25-29, 2008, Madison, Wisconsin, USA. New aspects of leptogenesis. Steve Blanchet. August 28, 2008. Outline. Modern view of leptogenesis See-saw mechanism and cancellation New aspects Usual lower bound in the hierarchical limit can be relaxed Effect of the Higgs asymmetry

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Particle Physics Cosmology

Neutrino Mass Measurements. Particle Physics Cosmology. What is the neutrino mass scale?. Hamish Robertson, ESPP12, Kracow , Sept. 11, 2012 . Y.Y.Y. Wong. Y.Y.Y. Wong. Neutrino mass from Beta Spectra. With flavor mixing :. mixing. neutrino masses. from oscillations.

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Beyond Vanilla

Beyond Vanilla. CMB+LSS will measure the standard cosmological parameters ( W m h 2 , W b h 2 , n , A S , h ) to percent level in the next few years. But there's lots more to do, e.g., Dark Energy: cosmological constant or not? If not, what? Dark Matter, deviations from CDM

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