Axions PowerPoint PPT Presentations

Gauged Axions Claudio Coriano Physics Department University of Salento, INFN Lecce

Cluster Lensing, and Axions Search

Upon entering the horizon. CDM density perturbations evolve linearly ... linear regime inside the horizon on all scales of. observational interest. ...

Search for high-energy axions with the CERN Axion Solar Telescope ... Use the 95% CL allowed counts at each energy and convolve with. Detector efficiency (e) ...

'Snooker' (Billiards) Quantitative Analysis. Final Remarks. Agenda ... Double check pool table physics. Oscillations depend on length of lever arm (decay const. ...

The Giant Dipole Resonance group is searching for the axions through their decay into electronpositr

B. Morgan1, N.J.C. Spooner1, S.M. Paling1, T.B. Lawson1, J.C. Davies1, K. Zioutas2, D.H.H. Hoffmann3, J. Jacoby4. Introduction: Axions in Extra Dimensions

Padova and Torino) CRC Louvain-la-Neuve. GB University of Birmingham ... Neutrino oscillations ( CERN - Gran Sasso) OPERA - Solar axions ( CERN, RBI ) CAST ...

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Ramage,GGR. KK state. For some compactifications LKP stable ... Cryptons,... Indirect detection. Direct detection possible. CMSSM. Ramage, GGR. SO(10) ...

... guess the correct theory. More likely, success will come from looking at classes of theories (Supersymmetric? ... One can construct field theory models for this. ...

UC Davis High Energy Seminar Ultrasensitive Searches for the Axion Karl van Bibber, LLNL January 23,

Search for new physics from the CERN Axion Solar Telescope (CAST) ... Thermocouple. placement. Ultra-low bckg Pb. Incoming gammas (from magnet bore) Pb shielding ...

Nuevas Observaciones

CAST: Axion helioscope experimental setting. La Thuile, March 2005. Berta Beltr n. 10 ... (Tokyo Helioscope sensitivity) CAST TPC Subtracted spectrum ...

Research will thus become a collective process and the evaluation of the methods ... Behavioral designers. Model builders and rapid prototypers. User-testers ...

... Full Width Half Maximum ROOT Conclusion Labview program successful Useful tool Collects & stores data Visual during data collection Future Find optimal voltage ...

LAB OF TOMORROW project: A constructivist approach in science teaching through emerging technologies IST-2000-25076 S.A.Sotiriou, Ellinogermaniki Agogi

Consider a photon beam in vacuo with k along the z-axis. ... 'Sic stantibus rebus'.... INDEPENDENT CHECKS of PVLAS claim look COMPELLING. ...

It is accepted now that dark matter is observed(SN1,WMAP). There are several particle physics ... compared to X-ray images(red) Gravitational lensing ...

Searching for some extra neutral interactions at the Large ... Valence quark sector. Gluon sector. The structure of the anomalous amplitude. Z photon photon ...

Searches for Dark Matter the Quest

Searches for Dark Matter the Quest

Title: No Slide Title Last modified by: vagelis Created Date: 5/8/2000 9:24:56 AM Document presentation format: On-screen Show Other titles: Times New Roman Arial ...

An abridged review of axion

The number density of clusters above a certain mass threshold is sensitive to Wm, ... predicted by Bullock et al. (2001) g M180c ...

Direct Detection of Cold Flows of Dark Matter. Ling Fu-Sin ... Earth's eccentricity. Frequency shift on the measurement time scale. Density modulation ...

Title: dark matter Author: High Energy Physics group Description: Schools presentation Last modified by: Susan Cartwright Created Date: 5/19/1998 3:51:11 PM

Searching for Anomalous Extra Z' at the LHC. Claudio Coriano' ... Golden plated process: Drell-Yan lepton pair production. but also other s-channel processes ...

mt! Unification Textures? LMA Presents a Challenge. Lopsided Mass Matrices ... ( Strange Stars??) Gravity Waves. Cosmological (Inflation) Extreme Collisions ...

Composition of the Cosmos. March 25, 2003. Lynn Cominsky - Cosmology ... National Center for Supercomputing Applications http://www.ncsa.uiuc.edu/Cyberia/Cosmos ...

Title: Diapositiva 1 Author: Decarli Last modified by: Guido Chincarini Created Date: 10/15/2005 4:30:14 PM Document presentation format: On-screen Show

... axion, represented as two wave packets of particle antiparticle of width d(t) ... Continuous axion photon duality and its consequences.E.I. ...

Dark matter particles: weakly interacting bosons and scalar fields may ... Can one form a central dark ... no solid surface ('boson sponge') and no horizon ...

Scottish Universities Summer School. Aug 21, 2001. Isothermal Spheres: A Cultural Aside... COBE: FIRST ANISOTROPY! COBE: FIRST ANISOTROPY! ...

Roberto Decarli Dark Matter Nature First evidences of Dark Matter in Universe Baryonic or non baryonic? Thermal or non thermal? Hot, Warm, Cold or other?

Dark Matter Projects at the Uppsala Observatory: Quasar Microlensing. Galaxy Kinematics ... A Gallery of Multiply-Imaged Quasars. Uppsala Project I: ...

Bubble Bubble Toil and Trouble. Bubble bubble toil and trouble ... For a charm of powerful trouble. Like a hell-broth boil and bubble. Shakespeare (Macbeth) ...

Dark Matter-Baryon segregation in the non-linear evolution of coupled Dark Energy models ... within top-hat considered: escaped baryon fraction neglected ...

WIMP candidates motivated by particle experiments ... Mayer-Hasselwander (1998) - EGRET point source 'close to' the galactic center. Spatial analysis ...

The Invisible Universe Dark Matter and Dark Energy

HiSparc

Small scale modifications to the power spectrum and 21 cm observations. Kathryn Zurek ... May reach to smaller scales on account of less gas heating at high redshifts ...

Different kinds of experience condition the brain in different ways. ... they are driven by different physiological mechanisms and by different events. ...

subdominant candidates variety is common in Nature. may be easier to detect ... thermal (ma 10-3 eV, subdominant) otherwise: smaller ma possible [Tegmark, ...

If neutrinos have mass, they account for part of the missing mass problem, but ... France (AGAPE) and POINT-AGAPE Collaboration. France (EROS) ...

Four or less: potentials for moduli, tadpoles (perturbative or non-perturbative) ... Tadpole cancellation conditions: c(X)/24= ND3 k102 T3 sM H3 F3 ...

Emily Dickinson, 1860. Spectrum of Perturbations. Total number of inflation e-foldings Ntot 60 ... TO DO: perturbations (with S. Watson) Rolling Models: ...

3 main collaborations MACHO, EROS, OGLE new groups and M31 ... The EROS experiment. EROS1 (1990-1995) photographic plates (25 deg2) ...

Low-z galaxy with pairs of high-z quasars (with z1 z2) aligned along minor axis ... explain the long-term optical variability of quasars Hawkins is wrong! ...

Low and very low Energy Recoils for fun and profit J'I' Collar, UC

(Explicit form of K, W, f. For N=1 compactifications) Why LARGE volume? ... Simplest case ?=1/3. General Conditions for LARGE Volume. h12 h11 1 ...

Silk (1968), Gunn et al (1978), Davis et al ... Predictions depend on the DM halo profile -2. C.B., T. Ensslin, J. Silk ... Sagittarius Dwarf Elliptical Galaxy ...

Sagittarius Dwarf Spheroidal. Sgr dwarf is closest satellite at 24 kpc ... Stellar density profile. Mass-to-Light Ratio. Leading-to-Trailing Stream Ratios ...

Luminous matter does not account for enough mass to explain rotational velocities of galaxies ... Also groups pursuing Argon (WARP/ArDM), Helium (HERON), Neon (CLEAN) ...