dark particle hunters - physics and astronomy at...

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LHC: HUNT FOR DARK MATTER Teruki Kamon 1),2) 1) Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University 2) WCU Collider Physics Research, Kyungpook National University 1 Sean Connery as Marko Ramius Summary Teruki Kamon 2 O OUTLINE 3 3 1) Dark Matter and SUSY 2) LHC & CMS Detector 3) Re-discoveries SUSY Prologue The LHC started taking data from proton-proton collisions at a center-of-mass energy of 7 TeV on March 30, 2010 and became the energy frontier machine to lead to discoveries of new particles. The Standard Model (SM) is currently well tested up to ~100 GeV, but is expected to break down in the TeV domain where new physics should occur. This is precisely the domain that we will study at the LHC. New Physics at CMS h http://faculty.physics.tamu.edu/kamon/research/Cosmology_at_Colliders/ http://faculty.physics.tamu.edu/kamon/research/LHCpheno/ Phys. Lett. B 505 (2001) 161 Phys. Lett. B 538 (2002) 121 Phys. Lett. B 611 (2005) 223 Phys. Lett. B 618 (2005) 182 Eur. Phys. J. C46 (2006) 43 Phys. Lett. B 639 (2006) 46 Phys. Lett. B 649 (2007) 73 Phys. Rev. Lett. 100 (2008) 231802 Phys. Rev. D 79 (2009) 055002 hep-ph/1008.3380, accepted for publication in Phys. Rev. D (2010) 3 TAMU-KNU Pheno Projects Today, I focus on theoretical motivation to search for SUSY dark matter and show a experimental readiness of the CMS detector for 2011 run. We have been working on how to determine cosmologically-consistent collider signals. Below are the list of papers. 4 3 2 1 1 splitting normal matter and dark matter apart Another Clear Evidence of Dark Matter (8/21/06) Dark Matter (Gravitational Lensing) Ordinary Matter (NASA’s Chandra X Observatory) time Approximately the same size as the Milky Way Dark Matter in the Universe Teruki Kamon 4 PPC at the LHC

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LHC:

HUNT

FOR

DARK

MATTER

Teru

kiKam

on1),2)

1) Mitch

ell Institu

te for Fu

nd

amen

tal Physics an

d A

stronom

y, Texas A

&M

Un

iversity 2) W

CU

Collid

er Physics R

esearch, K

yun

gpook

Nation

al Un

iversity

1

Sean Connery

as Marko R

amius

Sum

mary

TerukiKam

on2

OOU

TL

INE

33

1)Dark M

atter and SUSY

2)LH

C & CMS D

etector3)

Re-discoveries ��SU

SY

PrologueThe

LHC

startedtaking

datafrom

proton-protoncollisions

ata

center-of-mass

energyof

7TeV

onM

arch30,

2010and

became

theenergy

frontierm

achineto

leadto

discoveriesof

newparticles.

TheStandard

Model

(SM)

iscurrently

welltested

upto

~100GeV,but

isexpected

tobreak

downin

theTeV

domain

wherenew

physicsshould

occur.Thisis

preciselythe

domain

thatwe

willstudyat

theLH

C.

New

Physics at CM

S

hhttp

://fac

ulty.p

hysic

s.tam

u.e

du

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on

/rese

arch

/Co

smo

log

y_at_Co

llide

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lty.ph

ysics.ta

mu

.ed

u/ka

mo

n/re

sea

rch/L

HC

ph

en

o/

Phys. Lett. B 505 (2001) 161

Phys. Lett. B 538 (2002) 121

Phys. Lett. B 611 (2005) 223

Phys. Lett. B 618 (2005) 182

Eur. Phys. J. C46 (2006) 43

Phys. Lett. B 639 (2006) 46

Phys. Lett. B 649 (2007) 73

Phys. Rev. Lett. 100 (2008) 231802

Phys. Rev. D

79 (2009) 055002hep-ph/1008.3380, accepted for publication in Phys. R

ev. D (2010)

3

TA

MU

-KN

U P

hen

oP

rojects

Today,I

focuson

theoreticalmotivation

tosearch

forSU

SYdark

matter

andshow

aexperim

entalreadiness

ofthe

CMS

detectorfor

2011run.

We

havebeen

workingon

howto

determine

cosmologically-consistent

collidersignals.

Beloware

thelist

ofpapers.

4 3 2 11splitting norm

al matter and dark m

atter apart–

Another C

lear Evidence of Dark M

atter –(8/21/06)

Dark M

atter(G

ravitational Lensing)

Ordinary M

atter(N

ASA’s C

handra XO

bservatory)

time

Approxim

ately the sam

e size asthe M

ilky Way

Dark

Matter in

the U

niverse

TerukiKam

on4

yy

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C

Th

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iverseD

o w

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no

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ive

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TerukiKam

on5

PPC at the LH

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Wilkinson M

icrowave A

nisotropy Probe (WM

AP):�

DM

= 23%W

hat is the dark matter?

An elem

entary particle?

CCa

n it b

e o

ne

of th

e kn

ow

n p

article

s?LL

et’s ch

eck o

ut!

It Doesn’t M

atter.R

ight, it doesn’t shake hand with anyone easily. Tw

o dark m

atter clusters (in blue) are just passing each other. It is a long-lived

(stable)object.

It’s a Cold M

atter.Yes, it is a “relativistically” slow

ly moving (“cold”) object.

4

It’s an Invisible Matter.

Right, it doesn’t respond to your flash light.

This means it is a neutralobject.

So, It’s a ���

����

��

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��

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DM

).

Pro

perties o

f Cold

Dark

Matter

TerukiKam

on6

PPC at the LH

C

Quarks,electron,m

uon,tauparticles,and

forcecarriers

cannot

bethe

darkm

atter,sincetheir

interactionsare

strongerthan

whatw

eexpect.

Neutrinos

can,buttheyhave

otherproblems.

XX

XX

XX

XX

XX

XX

XXXXTerukiKam

on7

PPC at the LH

C

CD

M in

Th

e Sta

ndard

Model?

We need an new idea beyond

the Standard Model.

Any guidance?

�e.g.,

Supersymmetry

(SUSY)

Texa

s-style SU

SY

Hu

ntin

g

TerukiKam

on8

PPC at the LH

C

© S. K

amon

SU

SY

is:

a)

Su

persym

metrized

Sta

ndard

Model

(“ Dem

ocra

tic”so

lutio

nbetw

eenFerm

ion

san

dB

oso

ns);

b)

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elegan

tso

lutio

nto

solve

the

pro

blem

asso

ciated

with

the

Higgs

mass;

Su

persym

metry

(SU

SY

)

+

Unification!

c)B

eau

tifully

con

nectin

gth

eSta

ndard

Model

with

an

ultim

ate

un

ificatio

nof

the

fun

dam

enta

lin

teractio

ns;

d)

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olo

gically

con

sistent

with

aD

ark

Matter

can

did

ate

–sta

ble

neu

tralin

o.

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Neutral

Lightest

SUSY

Particle typeTerukiK

amon

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PPC at the LH

C

ME

NU

~S

PE

CIA

LS

~

*Dark E

nerg

y Pow

er Drin

k .. $73-

Ch

ef’s choice

*Dark M

atter Sand

wich

……

$23-

Neu

tral, long-lived

*Atom

ic Soup

……

……

……

. $4-

All elem

ents in

one

No

, Sir. B

ut w

ith

ne

utra

lino

?

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Ca

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ak

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with

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rticle?

“Da

rk M

atte

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nd

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10Teruki K

amon

Probing Supersymm

etric Connection w

ith DM

1111

LHC

annihilation

combination

Pro

bin

g E

arly U

niv

erse

I am

travelin

g a lo

t …

1

2

3

0

1212

Mitch

ell In

stitute

for

Fu

nd

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en

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my, Te

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A&

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WWO

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HY

SIC

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GE

NC

Y

High Energy Physics Special Agent

TERU

KI K

AM

ON

WPA C

ode: XXXX XXXX XXXX 0007(D

ark Matter H

unter)C

ode Nam

e: SUSY

Affiliations: TAMU

, KN

UO

ccupation: Professor

Current Status: AC

TIVE, TravelingC

ountry: Europe, Japan, Korea, U

SA

DO

B: unknow

nLocation: unknow

n

Ialw

ayshave

tocarry

onJapanese

passport,U

Sresidency

card,Texas

A&

Mfaculty

IDcard,

Texasstate

driverslicense

card,andK

oreanresidency

card.1313

© S. K

amon

My D

au

ghter’s Im

age o

f Dad …

27 km ring

14

Large H

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e LH

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erful to

Crea

te Massive O

bjects

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Proton-Proton Collisions

Proton Collisions 1 billion (10

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Bunch C

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On

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CosmologicallyConsistent Signals

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top),since

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inantbackgrounds

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illgo

throughselected

topicson

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searches:

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arr and Claire G

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48

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/

PPC at the LH

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CB

S comedy “B

ig Bang T

heory”(Season 1 E

pisode 15)

52

Sum

mary

RRe

ma

rk: PP

CInterconnection betw

een Particle Physics and Cosm

ology

PPC 2011 at C

ERN

, June 14-18PPC

2012 at ???

TerukiKam

on53

CSI:

Su

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metry

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e LH

CC

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mm

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TerukiKam

on54

LHC –

keep going!

FFY

I: ZZ

Ca

nd

idate

55

Nov. 8, 2010

Pb

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avy Ion

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llision

56

Nov. 14, 2010

FFY

I: Z in

He

avy Ion

Co

llision

57