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Transcript
Physics Beyond the Standard Model
I think I finally
understand atoms
Democritus 460–370 BC
I.
II.
III.
I. Nestoras
L. Zimmerman
S. Anderl
1
General Outline
Part I (I. Nestoras)
• SuperSymmetry (SUSY)
Part II (L. Zimmerman)
• Dark Matter
Part III (S. Anderl)
• String Theory
2
I think I finally
understand atoms
Democritus 460–370 BC
3
Particle Physics - Intro
• Particle Physics is the study individual particles
(protons, neutrons, electrons muons, kaons, pions,
lambdas,quarks,…)
• And the forces between them.
(gravity, electromagnetism, strong force, weak force).
4
Particle Physics - Intro
Question: how many cuts are required?
Answer: only 84 times!
A nucleus with
orbiting electrons
nanometre
5
Particle Physics - Intro
The forces of nature
Unified?
6
History of Unification
Planets
Apple
Electric
Gravity
Mechanics
Magnetism
Electromagnetism
Atoms
Quantum mechanics
g-decay
QED
Weak force
GR
Special relativity
String theory?
a-decay
Electroweak theory
Strong force
SM
b-decay
SM
SUSY - Grand Unification?
7
Problems of SM (Experimental)
• Gravity
• Dark matter and dark energy
• Neutrino masses
• Matter–antimatter asymmetry
8
Problems of SM (Theoretical)
Problem
• Hierarcy problem
• Strong CP problem
• Number of parameters
9
Problems of SM (Predictions not observed)
In the “Standard Model” the
origin of mass is addressed
using a mechanism named
after the British physicist Peter
Higgs. This predicts a new
particle:
the Higgs boson.
10
11
What about
Supersymmetry?
12
Beyond SM
Super-symmetry
OR
SUSY
13
Brief history of Supersymmetry
•
First proposed by Hironari Miyazawa in 1966
•
Supersymmetry was revealed in two-dimensional string models in 1971
by Ramond, Neveu, Schwarz, Gervais and Sakita
The history of supersymmetry is exceptional. In the past, virtually all
major conceptual breakthroughs have occurred because physicists were
trying to understand some established aspect of nature. In contrast, the
discovery of supersymmetry in the early 1970s was a purely intellectual
achievement, driven by the logic of theoretical development rather than
by the pressure of existing data.
14
What is Supersymmetry ?
There are two types of particles in nature: fermions and bosons.
Fermions have half units of spin, and tend to shy away from each other, like
people who always stay in single rooms at the fermion motel.
Bosons have zero or integer units of spin, and like to be with each other, like
people who stay in shared dormitories at the boson inn.
Supersymmetry says that for every fermion in
Nature there must be a boson and vice-versa.
Super-symmetric particles have not been observed
(yet) so they must be heavier - SUSY must be
broken by some mechanism
15
SuperSymetry
d
s b
 e   
e  
The Generations of Matter
Squarks
u c t
SPIN 0 BOSONS
Sleptons
Leptons
Quarks
SPIN ½ FERMIONS
u c t
d s b
 e   
e  
The Generations of Smatter
16
SuperSymetry
BOSO
NS
FERMIONS
Gravitino
W  W  Z0
Photino
Gluino
17
17
SuperSymetry
18
19
SuperSymetry
Strong
Strong
Not a Problem
Weak
Weak
Electromagnetic
Electromagnetic
20
Quote from Ed Witten in preface of Gordon
Kane’s book “Super-symmetry”
“Super-symmetry, if it holds in nature, is part of the quantum structure of space
and time…
Discovery of super-symmetry would be one of the real milestones in physics…
Indeed, super-symmetry is one of the basic requirements of string theory…
Discovery of super-symmetry would surely give string theory an enormous
boost…
The search for super-symmetry is one of the great dramas in present day
physics.”
21
SuperSymetry
SUSY provides an excellent candidate for
dark matter.
In SUSY we TRUST!!!
22
Welcome Lisa for dark matters (applause)
23