signal diversity and eft in dark matter direct detection
play

Signal Diversity and EFT in Dark Matter Direct Detection Bradley J - PowerPoint PPT Presentation

Sep 02, 2022 •326 likes •820 views

Signal Diversity and EFT in Dark Matter Direct Detection Bradley J Kavanagh GRAPPA, University of Amsterdam 25th June 2018, DSU, Annecy b.j.kavanagh@uva.nl @BradleyKavanagh Last time I was in Annecy was January 2016 and everyone in

  1. Signal Diversity and EFT in Dark Matter Direct Detection Bradley J Kavanagh GRAPPA, University of Amsterdam 25th June 2018, DSU, Annecy b.j.kavanagh@uva.nl @BradleyKavanagh

  2. Last time I was in Annecy was January 2016… … and everyone in the audience looked a little sleep deprived…

  3. Anyway, now we have the XENON1T 1-sigma excess… * @pjtunney * or rather, theorists… 3 Bradley J. Kavanagh (GRAPPA, Amsterdam) Effective Field Theory in Direct Detection

  4. <latexit sha1_base64="uhXdJBMSH9wplrzbRGnJ0WZkSrM=">ACDXicbVDLSsNAFJ34rPUVdelmsAquaiKCrqSgC91Vah/QpGEynbRDZ5I4MymU0B9w46+4caGIW/fu/BsnbRbaeuDC4Zx7ufceP2ZUKsv6NhYWl5ZXVgtrxfWNza1tc2e3IaNEYFLHEYtEy0eSMBqSuqKkVYsCOI+I01/cJX5zSERkbhvRrFxOWoF9KAYqS05JmHjqQ9jqx53Ck+oKntduT2vUYap3DYceCDx3LM0tW2ZoAzhM7JyWQo+qZX043wgknocIMSdm2rVi5KRKYkbGRSeRJEZ4gHqkrWmIOJFuOvlmDI+0oVBJHSFCk7U3xMp4lKOuK87s5PlrJeJ/3ntRAUXbkrDOFEkxNFQcKgimAWDexSQbBiI0QFlTfCnEfCYSVDrCoQ7BnX54njdOybZXtu7NS5TKPowD2wQE4BjY4BxVwA6qgDjB4BM/gFbwZT8aL8W58TFsXjHxmD/yB8fkDMGKa8A=</latexit> <latexit sha1_base64="uhXdJBMSH9wplrzbRGnJ0WZkSrM=">ACDXicbVDLSsNAFJ34rPUVdelmsAquaiKCrqSgC91Vah/QpGEynbRDZ5I4MymU0B9w46+4caGIW/fu/BsnbRbaeuDC4Zx7ufceP2ZUKsv6NhYWl5ZXVgtrxfWNza1tc2e3IaNEYFLHEYtEy0eSMBqSuqKkVYsCOI+I01/cJX5zSERkbhvRrFxOWoF9KAYqS05JmHjqQ9jqx53Ck+oKntduT2vUYap3DYceCDx3LM0tW2ZoAzhM7JyWQo+qZX043wgknocIMSdm2rVi5KRKYkbGRSeRJEZ4gHqkrWmIOJFuOvlmDI+0oVBJHSFCk7U3xMp4lKOuK87s5PlrJeJ/3ntRAUXbkrDOFEkxNFQcKgimAWDexSQbBiI0QFlTfCnEfCYSVDrCoQ7BnX54njdOybZXtu7NS5TKPowD2wQE4BjY4BxVwA6qgDjB4BM/gFbwZT8aL8W58TFsXjHxmD/yB8fkDMGKa8A=</latexit> <latexit sha1_base64="uhXdJBMSH9wplrzbRGnJ0WZkSrM=">ACDXicbVDLSsNAFJ34rPUVdelmsAquaiKCrqSgC91Vah/QpGEynbRDZ5I4MymU0B9w46+4caGIW/fu/BsnbRbaeuDC4Zx7ufceP2ZUKsv6NhYWl5ZXVgtrxfWNza1tc2e3IaNEYFLHEYtEy0eSMBqSuqKkVYsCOI+I01/cJX5zSERkbhvRrFxOWoF9KAYqS05JmHjqQ9jqx53Ck+oKntduT2vUYap3DYceCDx3LM0tW2ZoAzhM7JyWQo+qZX043wgknocIMSdm2rVi5KRKYkbGRSeRJEZ4gHqkrWmIOJFuOvlmDI+0oVBJHSFCk7U3xMp4lKOuK87s5PlrJeJ/3ntRAUXbkrDOFEkxNFQcKgimAWDexSQbBiI0QFlTfCnEfCYSVDrCoQ7BnX54njdOybZXtu7NS5TKPowD2wQE4BjY4BxVwA6qgDjB4BM/gFbwZT8aL8W58TFsXjHxmD/yB8fkDMGKa8A=</latexit> <latexit sha1_base64="uhXdJBMSH9wplrzbRGnJ0WZkSrM=">ACDXicbVDLSsNAFJ34rPUVdelmsAquaiKCrqSgC91Vah/QpGEynbRDZ5I4MymU0B9w46+4caGIW/fu/BsnbRbaeuDC4Zx7ufceP2ZUKsv6NhYWl5ZXVgtrxfWNza1tc2e3IaNEYFLHEYtEy0eSMBqSuqKkVYsCOI+I01/cJX5zSERkbhvRrFxOWoF9KAYqS05JmHjqQ9jqx53Ck+oKntduT2vUYap3DYceCDx3LM0tW2ZoAzhM7JyWQo+qZX043wgknocIMSdm2rVi5KRKYkbGRSeRJEZ4gHqkrWmIOJFuOvlmDI+0oVBJHSFCk7U3xMp4lKOuK87s5PlrJeJ/3ntRAUXbkrDOFEkxNFQcKgimAWDexSQbBiI0QFlTfCnEfCYSVDrCoQ7BnX54njdOybZXtu7NS5TKPowD2wQE4BjY4BxVwA6qgDjB4BM/gFbwZT8aL8W58TFsXjHxmD/yB8fkDMGKa8A=</latexit> ‘Standard’ direct detection Spin-dependent (SD) σ p SI / SD ∼ v 0 q 0 Spin-independent (SI) [1702.07666] But these interactions are not always there… [1805.12562] 4 Bradley J. Kavanagh (GRAPPA, Amsterdam) Effective Field Theory in Direct Detection

  5. 
 
 
 Non-standard interactions? Why? Out of curiosity 
 • Don’t you just want to know…? What could DM look like? What could we be missing? Input for experimental analysis 
 • Experimental searches are not simple cut-and-counts - need to know what the signal looks like to get the best sensitivity Optimisation of future experiments 
 • Which experiments should we use to get the best sensitivity, or the most information out of a future detection? (more on this later) 5 Bradley J. Kavanagh (GRAPPA, Amsterdam) Effective Field Theory in Direct Detection

  6. Experimental analysis Limits depend on a signal hypothesis and we need to know where to look! [1805.12562] So where should we look? [1705.02614] 6 Bradley J. Kavanagh (GRAPPA, Amsterdam) Effective Field Theory in Direct Detection

  7. <latexit sha1_base64="ovfVRFYGmsk+mNITze8OsNZ1u4E=">AB+HicbVBNS8NAEN3Ur1o/GvXoZbEInkoiguKp4MWTVLAf0ISw2U7apZtN3N0Uaugv8eJBEa/+FG/+G7dtDtr6YODx3gwz8KUM6Ud59sqra1vbG6Vtys7u3v7VfvgsK2STFJo0YQnshsSBZwJaGmOXRTCSQOXTC0c3M74xBKpaIBz1JwY/JQLCIUaKNFNhVbw0f5xij3McB3eBXPqzhx4lbgFqaECzcD+8voJzWIQmnKiVM91Uu3nRGpGOUwrXqYgJXREBtAzVJAYlJ/PD5/iU6P0cZRIU0Ljufp7IiexUpM4NJ0x0UO17M3E/7xepqMrP2cizTQIulgUZRzrBM9SwH0mgWo+MYRQycytmA6JFSbrComBHf5VXSPq+7Tt29v6g1ros4yugYnaAz5KJL1EC3qIlaiKIMPaNX9GY9WS/Wu/WxaC1ZxcwR+gPr8wdEXJLK</latexit> <latexit sha1_base64="ovfVRFYGmsk+mNITze8OsNZ1u4E=">AB+HicbVBNS8NAEN3Ur1o/GvXoZbEInkoiguKp4MWTVLAf0ISw2U7apZtN3N0Uaugv8eJBEa/+FG/+G7dtDtr6YODx3gwz8KUM6Ud59sqra1vbG6Vtys7u3v7VfvgsK2STFJo0YQnshsSBZwJaGmOXRTCSQOXTC0c3M74xBKpaIBz1JwY/JQLCIUaKNFNhVbw0f5xij3McB3eBXPqzhx4lbgFqaECzcD+8voJzWIQmnKiVM91Uu3nRGpGOUwrXqYgJXREBtAzVJAYlJ/PD5/iU6P0cZRIU0Ljufp7IiexUpM4NJ0x0UO17M3E/7xepqMrP2cizTQIulgUZRzrBM9SwH0mgWo+MYRQycytmA6JFSbrComBHf5VXSPq+7Tt29v6g1ros4yugYnaAz5KJL1EC3qIlaiKIMPaNX9GY9WS/Wu/WxaC1ZxcwR+gPr8wdEXJLK</latexit> <latexit sha1_base64="ovfVRFYGmsk+mNITze8OsNZ1u4E=">AB+HicbVBNS8NAEN3Ur1o/GvXoZbEInkoiguKp4MWTVLAf0ISw2U7apZtN3N0Uaugv8eJBEa/+FG/+G7dtDtr6YODx3gwz8KUM6Ud59sqra1vbG6Vtys7u3v7VfvgsK2STFJo0YQnshsSBZwJaGmOXRTCSQOXTC0c3M74xBKpaIBz1JwY/JQLCIUaKNFNhVbw0f5xij3McB3eBXPqzhx4lbgFqaECzcD+8voJzWIQmnKiVM91Uu3nRGpGOUwrXqYgJXREBtAzVJAYlJ/PD5/iU6P0cZRIU0Ljufp7IiexUpM4NJ0x0UO17M3E/7xepqMrP2cizTQIulgUZRzrBM9SwH0mgWo+MYRQycytmA6JFSbrComBHf5VXSPq+7Tt29v6g1ros4yugYnaAz5KJL1EC3qIlaiKIMPaNX9GY9WS/Wu/WxaC1ZxcwR+gPr8wdEXJLK</latexit> <latexit sha1_base64="ovfVRFYGmsk+mNITze8OsNZ1u4E=">AB+HicbVBNS8NAEN3Ur1o/GvXoZbEInkoiguKp4MWTVLAf0ISw2U7apZtN3N0Uaugv8eJBEa/+FG/+G7dtDtr6YODx3gwz8KUM6Ud59sqra1vbG6Vtys7u3v7VfvgsK2STFJo0YQnshsSBZwJaGmOXRTCSQOXTC0c3M74xBKpaIBz1JwY/JQLCIUaKNFNhVbw0f5xij3McB3eBXPqzhx4lbgFqaECzcD+8voJzWIQmnKiVM91Uu3nRGpGOUwrXqYgJXREBtAzVJAYlJ/PD5/iU6P0cZRIU0Ljufp7IiexUpM4NJ0x0UO17M3E/7xepqMrP2cizTQIulgUZRzrBM9SwH0mgWo+MYRQycytmA6JFSbrComBHf5VXSPq+7Tt29v6g1ros4yugYnaAz5KJL1EC3qIlaiKIMPaNX9GY9WS/Wu/WxaC1ZxcwR+gPr8wdEXJLK</latexit> <latexit sha1_base64="8bjGlFK2DGL2GhXlV23VRPv0wEM=">AB9HicbVBNS8NAEJ34WetX1aOXxSJ4KokIiqeCF48V7Ac0oWy2k3bpZhN3N4US+ju8eFDEqz/Gm/GbZuDtj4YeLw3w8y8MBVcG9f9dtbWNza3tks75d29/YPDytFxSyeZYthkiUhUJ6QaBZfYNwI7KQKaRwKbIeju5nfHqPSPJGPZpJiENOB5BFn1Fgp8MfI8vGU+EIQ1qtU3Zo7B1klXkGqUKDRq3z5/YRlMUrDBNW67mpCXKqDGcCp2U/05hSNqID7FoqaYw6yOdHT8m5VfokSpQtachc/T2R01jrSRzazpiaoV72ZuJ/Xjcz0U2Qc5lmBiVbLIoyQUxCZgmQPlfIjJhYQpni9lbChlRZmxOZRuCt/zyKmld1jy35j1cVeu3RwlOIUzuAPrqEO9CAJjB4gmd4hTdn7Lw4787HonXNKWZO4A+czx9qw5HT</latexit> <latexit sha1_base64="8bjGlFK2DGL2GhXlV23VRPv0wEM=">AB9HicbVBNS8NAEJ34WetX1aOXxSJ4KokIiqeCF48V7Ac0oWy2k3bpZhN3N4US+ju8eFDEqz/Gm/GbZuDtj4YeLw3w8y8MBVcG9f9dtbWNza3tks75d29/YPDytFxSyeZYthkiUhUJ6QaBZfYNwI7KQKaRwKbIeju5nfHqPSPJGPZpJiENOB5BFn1Fgp8MfI8vGU+EIQ1qtU3Zo7B1klXkGqUKDRq3z5/YRlMUrDBNW67mpCXKqDGcCp2U/05hSNqID7FoqaYw6yOdHT8m5VfokSpQtachc/T2R01jrSRzazpiaoV72ZuJ/Xjcz0U2Qc5lmBiVbLIoyQUxCZgmQPlfIjJhYQpni9lbChlRZmxOZRuCt/zyKmld1jy35j1cVeu3RwlOIUzuAPrqEO9CAJjB4gmd4hTdn7Lw4787HonXNKWZO4A+czx9qw5HT</latexit> <latexit sha1_base64="8bjGlFK2DGL2GhXlV23VRPv0wEM=">AB9HicbVBNS8NAEJ34WetX1aOXxSJ4KokIiqeCF48V7Ac0oWy2k3bpZhN3N4US+ju8eFDEqz/Gm/GbZuDtj4YeLw3w8y8MBVcG9f9dtbWNza3tks75d29/YPDytFxSyeZYthkiUhUJ6QaBZfYNwI7KQKaRwKbIeju5nfHqPSPJGPZpJiENOB5BFn1Fgp8MfI8vGU+EIQ1qtU3Zo7B1klXkGqUKDRq3z5/YRlMUrDBNW67mpCXKqDGcCp2U/05hSNqID7FoqaYw6yOdHT8m5VfokSpQtachc/T2R01jrSRzazpiaoV72ZuJ/Xjcz0U2Qc5lmBiVbLIoyQUxCZgmQPlfIjJhYQpni9lbChlRZmxOZRuCt/zyKmld1jy35j1cVeu3RwlOIUzuAPrqEO9CAJjB4gmd4hTdn7Lw4787HonXNKWZO4A+czx9qw5HT</latexit> <latexit sha1_base64="8bjGlFK2DGL2GhXlV23VRPv0wEM=">AB9HicbVBNS8NAEJ34WetX1aOXxSJ4KokIiqeCF48V7Ac0oWy2k3bpZhN3N4US+ju8eFDEqz/Gm/GbZuDtj4YeLw3w8y8MBVcG9f9dtbWNza3tks75d29/YPDytFxSyeZYthkiUhUJ6QaBZfYNwI7KQKaRwKbIeju5nfHqPSPJGPZpJiENOB5BFn1Fgp8MfI8vGU+EIQ1qtU3Zo7B1klXkGqUKDRq3z5/YRlMUrDBNW67mpCXKqDGcCp2U/05hSNqID7FoqaYw6yOdHT8m5VfokSpQtachc/T2R01jrSRzazpiaoV72ZuJ/Xjcz0U2Qc5lmBiVbLIoyQUxCZgmQPlfIjJhYQpni9lbChlRZmxOZRuCt/zyKmld1jy35j1cVeu3RwlOIUzuAPrqEO9CAJjB4gmd4hTdn7Lw4787HonXNKWZO4A+czx9qw5HT</latexit> More general interactions Can write non-relativistic (NR) DM- nucleon Lagrangian as an expansion in: [Fan et al - 1008.1591, Fitzpatrick et al. - 1203.3542] Recoil momentum - � q � m N DM velocity - � v � c L ⊃ L 0 + L 1 ( � v ) + L 2 ( � q ) + L 3 ( � q ) + ... v, � ‘Non-standard’ interactions ‘Standard’ interactions (higher order) (zeroth order) 7 Bradley J. Kavanagh (GRAPPA, Amsterdam) Effective Field Theory in Direct Detection

Recommend

DIRECT DETECTION OF NUCLEAR DARK MATTER USING TONNE-SCALE EXPERIMENTS What is Nuclear Dark

DIRECT DETECTION OF NUCLEAR DARK MATTER USING TONNE-SCALE EXPERIMENTS What is Nuclear Dark

DIRECT DETECTION OF NUCLEAR DARK MATTER USING TONNE-SCALE EXPERIMENTS What is Nuclear Dark Matter? Signal and sensitivity in DEAP-3600 and XENON1T Can it be distinguished from a vanilla WIMP signal? arXiv:1610.01840 ALISTAIR

335 views • 15 slides
Direct Detection of Dark Matter - Signal or No Signal? - The Best Way Forward Rick Gaitskell

Direct Detection of Dark Matter - Signal or No Signal? - The Best Way Forward Rick Gaitskell

Direct Detection of Dark Matter - Signal or No Signal? - The Best Way Forward Rick Gaitskell (gaitskell@brown.edu) Co-Spokesperson, LUX Collaboration Particle Astrophysics Group, Brown University, Department of Physics (Supported by US

766 views • 32 slides
Direct Detection Lecture 1: Introduction to Dark Matter Homework Efgective Lagrangians 1 / 37

Direct Detection Lecture 1: Introduction to Dark Matter Homework Efgective Lagrangians 1 / 37

Basics Frontiers in Dark Matter, Neutrinos, and Particle Physics July 2017 Dark Matter Direct Detection Zhao-Huan Yu (Melbourne) July 27-28, 2017 Sun Yat-Sen University, Guangzhou Theoretical Physics Summer School http://yzhxxzxy.github.io

690 views • 40 slides
HeRALD: Dark Matter Direct Detection with Superfluid 4He Doug Pinckney on behalf of the HeRALD

HeRALD: Dark Matter Direct Detection with Superfluid 4He Doug Pinckney on behalf of the HeRALD

HeRALD: Dark Matter Direct Detection with Superfluid 4He Doug Pinckney on behalf of the HeRALD collaboration 10 December 2019 Phys. Rev. D 100, 092007 1 Low Mass Dark Matter Direct Detection Parameter space wide open, O(10 g-day)

593 views • 31 slides
Direct and Indirect Detection of Dark Matter Zhao-Huan Yu School of Physics, Sun

Direct and Indirect Detection of Dark Matter Zhao-Huan Yu School of Physics, Sun

Dark Matter Direct Detection Indirect Detection Direct and Indirect Detection of Dark Matter Zhao-Huan Yu School of Physics, Sun Yat-Sen University http://yzhxxzxy.github.io June 18, 2019 Zhao-Huan Yu (SYSU) Direct and

967 views • 62 slides
Hydrodynamic simulations and dark matter direct detection Nassim Bozorgnia GRAPPA Institute

Hydrodynamic simulations and dark matter direct detection Nassim Bozorgnia GRAPPA Institute

Hydrodynamic simulations and dark matter direct detection Nassim Bozorgnia GRAPPA Institute University of Amsterdam Based on work done with F. Calore, M. Lovell, G. Bertone, and the EAGLE team arXiv: 1601.04707 Outline Dark matter direct

1.54k views • 75 slides
Direct Detection and Collider Searches of Dark Matter Lecture 2 Graciela Gelmini - UCLA Dark

Direct Detection and Collider Searches of Dark Matter Lecture 2 Graciela Gelmini - UCLA Dark

Direct Detection and Collider Searches of Dark Matter Lecture 2 Graciela Gelmini - UCLA Dark Matter School, Lund, Sept. 26-30, 2016 Graciela Gelmini-UCLA Content of Lecture 2 Introduction to WIMP dark matter searches, direct detection

769 views • 46 slides
Direct Detection Searches Bruno Serfass - UC Berkeley CGI Workshop, Oct. 2012 Dark Matter Halo

Direct Detection Searches Bruno Serfass - UC Berkeley CGI Workshop, Oct. 2012 Dark Matter Halo

Status of Dark Matter Direct Detection Searches Bruno Serfass - UC Berkeley CGI Workshop, Oct. 2012 Dark Matter Halo Evidence of Dark Matter at various galactic scales In particular, rotation curve of spiral galaxies imply the presence of

749 views • 49 slides
Direct Dark Matter Searches: an Overview GGI Conference on Dark Matter Florence, February 9, 2009

Direct Dark Matter Searches: an Overview GGI Conference on Dark Matter Florence, February 9, 2009

Direct Dark Matter Searches: an Overview GGI Conference on Dark Matter Florence, February 9, 2009 Laura Baudis University of Zurich 1 Goal of Direct Detection Experiments Detect new, yet undiscovered particles, which may be responsible

491 views • 35 slides
DEAP/CLEAN-ing Dark Matter: the Search for Direct Detection with Liquid Argon Jocelyn Monroe,

DEAP/CLEAN-ing Dark Matter: the Search for Direct Detection with Liquid Argon Jocelyn Monroe,

DEAP/CLEAN-ing Dark Matter: the Search for Direct Detection with Liquid Argon Jocelyn Monroe, Royal Holloway University of London Particle Physics Seminar Birmingham University February 8, 2012 Outline Direct Dark Matter Detection

767 views • 57 slides
Direct Detection of Dark Matter with Cryogenic Experiments Lauren Hsu Fermi National

Direct Detection of Dark Matter with Cryogenic Experiments Lauren Hsu Fermi National

Direct Detection of Dark Matter with Cryogenic Experiments Lauren Hsu Fermi National Accelerator Laboratory TeV Particle Astrophysics, Paris July 19, 2010 Is Dark Matter a WIMP? particles with mass and annihilation cross section at the weak

646 views • 43 slides
Towards Direct Detection of WIMPs with the Cryogenic Dark Matter Search Enectali

Towards Direct Detection of WIMPs with the Cryogenic Dark Matter Search Enectali

Towards Direct Detection of WIMPs with the Cryogenic Dark Matter Search Enectali Figueroa-Feliciano Massachusetts Institute of Technology For the CDMS Collaboration Towards Direct Detection of WIMPs with the Cryogenic Dark Matter Search

887 views • 61 slides
Closing in on mass-degenerate dark matter scenarios with antiprotons and direct detection On the

Closing in on mass-degenerate dark matter scenarios with antiprotons and direct detection On the

Closing in on mass-degenerate dark matter scenarios with antiprotons and direct detection On the complementarity of direct and indirect detection Stefan Vogl with Mathias Garny (DESY), Alejandro Ibarra and Miguel Pato (TUM) to appear soon S.

516 views • 23 slides
Direct Detection and Collider Searches of Dark Matter Lecture 4 Graciela Gelmini - UCLA Dark

Direct Detection and Collider Searches of Dark Matter Lecture 4 Graciela Gelmini - UCLA Dark

Direct Detection and Collider Searches of Dark Matter Lecture 4 Graciela Gelmini - UCLA Dark Matter School, Lund, Sept. 26-30, 2016 Graciela Gelmini-UCLA Content of Lecture 4 Halo-dependent and halo-independent direct detection data

698 views • 52 slides
Direct Detection of Dark Matter Dan McKinsey Yale University SUSY2011 August31,2011

Direct Detection of Dark Matter Dan McKinsey Yale University SUSY2011 August31,2011

Direct Detection of Dark Matter Dan McKinsey Yale University SUSY2011 August31,2011 Searching for WIMPs Accelerators: Look for dark matter candidates at the LHC. Squark and gluino decays result in leptons, jets, and missing

1.03k views • 55 slides
Dark matter direct detection Alvaro E Chavarria KICP at The University of Chicago 1 Overview

Dark matter direct detection Alvaro E Chavarria KICP at The University of Chicago 1 Overview

Dark matter direct detection Alvaro E Chavarria KICP at The University of Chicago 1 Overview Dark matter direct detection. DAMA and new NaI experiments. Recent results from PICO. Recent results from DarkSide. DAMIC

431 views • 39 slides
DANAE - a new experiment for direct dark matter detection using RNDR DEPFET detectors Hexi

DANAE - a new experiment for direct dark matter detection using RNDR DEPFET detectors Hexi

DANAE - a new experiment for direct dark matter detection using RNDR DEPFET detectors Hexi Shi HEPHY AW 11 April 2018 DEPFET workshop Schloss Ringberg DANAE (DANA) Direct dArk matter search using DEPFET with

587 views • 46 slides
Direct Detection of Dark Matter: Status and Issues Chris Savage University of Utah Overview

Direct Detection of Dark Matter: Status and Issues Chris Savage University of Utah Overview

Direct Detection of Dark Matter: Status and Issues Chris Savage University of Utah Overview CDMS Si Overview Are any/all of the experiments seeing dark matter? Are the results truly incompatible? Outline Dark matter: what is it and how

588 views • 56 slides
Novel Signatures of Dark Matter Clusters in Direct Detection Experiments Yongchao Zhang

Novel Signatures of Dark Matter Clusters in Direct Detection Experiments Yongchao Zhang

Novel Signatures of Dark Matter Clusters in Direct Detection Experiments Yongchao Zhang Washington University in St. Louis Based on: Shmuel Nussinov &amp; YCZ, 1807.00846 Oct 6, 2018 6 th PIKIO meeting, University of Notre Dame 2 Direct

635 views • 30 slides
Learning from Dark Matter direct detection Riccardo Catena Chalmers University of Technology

Learning from Dark Matter direct detection Riccardo Catena Chalmers University of Technology

Learning from Dark Matter direct detection Riccardo Catena Chalmers University of Technology September 12, 2019 Measuring the local Dark Matter density at direct detection experiments Riccardo Catena Chalmers University of Technology

309 views • 20 slides
Results of direct dark matter detection with CDEX experiment at CJPL Hao Ma ( ) for the

Results of direct dark matter detection with CDEX experiment at CJPL Hao Ma ( ) for the

Results of direct dark matter detection with CDEX experiment at CJPL Hao Ma ( ) for the CDEX Collaboration Tsinghua University XVI International Conference on Topics in Astroparticle and Underground Physics 9-13 Sept. 2019, Toyama, Japan

448 views • 29 slides
A scalable quantum architecture for dark matter detection Daniel Carney JQI/QuICS, University of

A scalable quantum architecture for dark matter detection Daniel Carney JQI/QuICS, University of

A scalable quantum architecture for dark matter detection Daniel Carney JQI/QuICS, University of Maryland/NIST Theory Division, Fermilab Based on Gravitational direct detection of dark matter DC , S. Ghosh, G. Krnjaic, J. M. Taylor,

387 views • 36 slides
Closing in on the velocity distribution of Dark Matter with direct detection and neutrino

Closing in on the velocity distribution of Dark Matter with direct detection and neutrino

DMUK Meeting - Oxford (08/12/2014) Closing in on the velocity distribution of Dark Matter with direct detection and neutrino telescopes 10 - 37 10 - 1 C D D Mattia Fornasa A M 10 - 38 10 - 2 M I S C ( l 2 2 ) 0 1 i t e 10 - 39

234 views • 6 slides
QUANTUM MATERIALS &amp; DARK MATTER DETECTION MOTIVATION NEW DIRECTIONS IN DARK MATTER THEORY

QUANTUM MATERIALS &amp; DARK MATTER DETECTION MOTIVATION NEW DIRECTIONS IN DARK MATTER THEORY

K. ZUREK Leveraging the many faces (and phases) of matter QUANTUM MATERIALS &amp; DARK MATTER DETECTION MOTIVATION NEW DIRECTIONS IN DARK MATTER THEORY Old paradigm: weak scale dark matter (with relic density fixed by freeze-out)

644 views • 29 slides

More recommend