Dark Matter M DM D DM halo Nuclear recoil Milky Way Sven - - PowerPoint PPT Presentation

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Dark Matter M DM D DM halo Nuclear recoil Milky Way Sven - - PowerPoint PPT Presentation

Dark Matter M DM D DM halo Nuclear recoil Milky Way Sven Vahsen, University of Hawaii Ordinary Matter Ordinary matter consists of atoms Atoms consist of three types of elementary particles Up quark Down quark Electron


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SLIDE 1

Dark Matter

DM halo Milky Way

Nuclear recoil

DM D M

Sven Vahsen, University of Hawaii

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SLIDE 2

Ordinary Matter

3/16/19 Punahou Master Class 2

  • Ordinary matter consists of

atoms

  • Atoms consist of three types of

elementary particles

– Up quark – Down quark – Electron

  • In radioactive decays, also the

electron neutrino is produced

– !"

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SLIDE 3

Ordinary Matter

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SLIDE 4

Three generations of particles

  • “2nd and 3rd generation”

– Discovered with cosmic rays and man-made particle accelerators – Heavier and unstable – Abundant in early universe

mass 175 GeV (=proton masses). Discovered 1995.

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SLIDE 5

What are the Force of Nature?

proton proton Photon

Even forces are due to elementary particles!

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SLIDE 6

The Four Forces of Nature

  • Electromagnetic interaction
  • Strong nuclear force
  • Weak Nuclear force
  • Gravity
  • Four types of forces - each has it’s own force carrier particles

G

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SLIDE 7

Putting it all together

  • Theoretically described

by “Standard Model” of particle physics since early 1970s

  • Standard Model

predicted Higgs Boson

H

mass

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SLIDE 8

Questions:

How can you see matter? What is happening when you see… …the sun? …other students? …yourself in a mirror? …a dark object?

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SLIDE 9

Things we cannot see with photons

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4.6% Ordinary Matter 23% Dark Matter 72% Dark Energy

  • Only 5% of energy in

the universe due to

  • rdinary matter

Punahou Master Class

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SLIDE 10

Question:

Is dark matter… dark?

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SLIDE 11

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What does the Dark Matter consist of?

http://home.slac.stanford.edu/pressreleases/2006/20060821.htm

Atoms

Dark Matter!

Punahou Master Class

  • Standard Model particles cannot explain dark matter
  • We think dark matter may be a new type of elementary particle!
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SLIDE 12
  • We may need to extend the standard model

Supersymmetry

12

H

~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~

H

~

Supersymmetry predicts new particles. Including dark matter particles!

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SLIDE 13

How can we test this hypothesis?

  • 1. Produce dark matter with particle accelerators
  • 2. Try to directly detect dark matter
  • 3. Observe decays of dark matter into visible particle

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SLIDE 14

The Large Hadron Collider (LHC)

  • Highest Energy Accelerator to date: Two beams of 7 TeV protons à E=14 TeV
  • 4 large detectors where protons collide
  • CMS and ATLAS: Search for the Higgs Boson & Physics beyond Standard Model
  • > 10,000 scientists and engineers from over 100 countries

CMS ALICE ATLAS LHCb

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SLIDE 15
  • ATLAS surrounds one of several points where particles will collide.
  • ATLAS “checks” what comes out of these collisions every 25 ns
  • about 100 “snapshots” / second are written to disk

for detailed analysis by the collaboration.

The ATLAS detector*

* ATLAS = A Toroidal LHC apparatus

Length : ~ 46 m Radius : ~ 12 m Weight : ~ 7000 tons ~ 108 electronic channels ~ 3000 km of cables

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SLIDE 16

Pixels: At the Heart of ATLAS

Detection of charged particles takes place in 1744 identical ATLAS Pixel Modules 6 cm Pixel 50 x 400 μm x46080 ATLAS

ATLAS Pixel Detector – Innermost tracking detector, surrounding beam pipe

1.3 m 1744 modules x 46080 pixels = 80 million channels! physicist 16 FE Chips ATLAS DETECTOR Length : ~ 46 m Radius : ~ 12 m Weight : ~ 7000 tons

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How to transport a Muon System

Biggest detector in ATLAS

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How to transport a pixel detector

Completed Detector Installed June 2007 Endcaps integrated at Berkeley Lab On the way to CERN! Barrel integrated at CERN Smallest detector in ATLAS

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SLIDE 19
  • 7-TeV protons kept in orbit by superconducting magnets
  • 8.33T, cooled by superfluid Helium at 1.9K

… after installation 100 m under ground

LHC Construction

Lowering one of 1232 di-pole magnets

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SLIDE 20

First Beams Circulated September 9th 2008

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SLIDE 21

2012 Higgs Discovery!

Higgs announcement seminar on 4 July 2012 Nobel prize in 2013

! → ##

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SLIDE 22

So far, we have not detected dark matter at the Large Hadron Collider…

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SLIDE 23

How can we test this hypothesis?

  • 1. Produce dark matter with particle accelerators
  • 2. Try to directly detect dark matter
  • 3. Observe decays of dark matter into visible particle

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SLIDE 24

Are We Surrounded By Dark Matter?

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dark matter halo? Milky Way

Punahou Master Class

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SLIDE 25

We can also try to directly detect Dark Matter

  • Huge detectors, Looking for 1 “blip”

per year!

  • Very clean, to avoid false detection

from radioactivity

  • Underground, to avoid false detection

from cosmic rays

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LUX detector 368 kg LXe Water shield W I M P , n , ! WIMP, n, ! " r a y " ray

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SLIDE 26

D3 - Directional Dark Matter Detector

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Prototype detector at UH Manoa

I’m working on this!

Punahou Master Class

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SLIDE 27

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Nuclear recoil

Dark Matter D a r k M a t t e r

This is how I want to detect it!

3mm

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SLIDE 28

If this works, I’d like to build a dark matter telescope in the future, to see where the dark matter comes from!

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SLIDE 29

Questions?

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