Manfred Jeitler December 18, 2009 1 Particle Physics From an experiment-driven to a theory-driven...
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Transcript of Manfred Jeitler December 18, 2009 1 Particle Physics From an experiment-driven to a theory-driven...
Manfred Jeitler December 18, 2009 1
Particle Physics
From an experiment-driven to a theory-driven field
Manfred Jeitler
Institute of High Energy Physics
of the
Austrian Academy of Sciences
Manfred Jeitler December 18, 2009 2
Particle Physicsin a nutshell
elementary particles first postulated in antiquity– Democritus called them ἄτομος (undividable = elementary), atoms
– what we call atoms today is not at all undividable!
– philosophical reasoning, no experimental evidence » maximally underdetermined
indirect evidence for atoms– elements react in ratios of small whole numbers
» John Dalton 1803: “law of multiple proportions”
– erratic movement of small objects» Brownian motion 1827 (Robert Brown)
Manfred Jeitler December 18, 2009 3
1897
the electrone-
ThomsonThomson
direct evidence for first elementary particle: the electron
Manfred Jeitler December 18, 2009 4
1897
the proton
e-
1900-1924
1914
RutherfordRutherford
p
another constituent of matter:the proton
Manfred Jeitler December 18, 2009 5
1897
the photon
1900-1924
PlanckPlanck EinsteinEinstein
ComptonCompton
e-
p
the particle of light:the photon
Manfred Jeitler December 18, 2009 6
1897
the neutron
e-
1900-1924
1914
np
1932
ChadwickChadwick
there is still something else in the nucleus:the neutron
Manfred Jeitler December 18, 2009 7
a particle theory of the world - all aspects nicely determined
a few particles nicely described our world– very simple: for a scientist, beautiful !
– Occam’s razor
each of them had been accurately determined by experiment
almost everything explained – except some details: for instance, what keeps the particles in a nucleus
together?
but experimentalists continued their observations!
Manfred Jeitler December 18, 2009 8
1897
the muon
e-
1900-1924
1914
µp
1932
n
1937
• Hess• Anderson, Neddermeyer
e+
Who ordered this ?
more particles appearing
Manfred Jeitler December 18, 2009 9
1897
„I have heard it said that the finderof a new elementary particle usedto be rewarded by a Nobel Prize,but that now such a discovery ought to be punished by a $10,000 fine.“
e-
1900-1924
1914
K
p
1932
n
1937
µ
1947
e+
1947-...
In his Nobel prize speech in 1955, Willis Lamb expressed nicely the general attitude at the time:
LambLamb
too many particles?
Manfred Jeitler December 18, 2009 10
the theorists’ turn
get some order into this “particle zoo”
after some more work (details later) everything was again classified into a model: The Standard Model (~1970)
Manfred Jeitler December 18, 2009 11
fermions (spin ½)
charge
0
-1
+2/3
-1/3
d
uu
du
d
leptons quarks
+1 0 proton neutron
baryons
interactions
strong
weak
gravitation?
weakW, Z
electromagnetic
strongg
force carriers = bosons (spin 1)
e
e
u c t
d s b
the Standard Modeltwo extra generations
Manfred Jeitler December 18, 2009 12
++
u
uu
u
d
d
us
c
d
D
s
u
b
b
d
uu
du
d
proton neutron
mesons
baryons
...
...
nucleus
He nucleus(-particle)
atom
matter
The Standard Model explaining all the particles
Manfred Jeitler December 18, 2009 13
where did the “extra generations” come from?
“leptons” (like electron) and “quarks” (like in proton and neutron) have heavier, unstable partners
predicted by theory ?
found as a surprise by experiment ?
Manfred Jeitler December 18, 2009 14
the second generation
muon (μ)– 2nd generation of “leptons” (the electron’s partner)
– observed by chance, not expected
“strange” quark (s-quark) – 2nd generation of “hadrons” (the up and down quarks’ partner)
– observed by chance, not expected
puzzle observed: no “flavor-changing neutral currents”– particle decays described by strange quark (inside an unstable particle)
decaying into up quark, but never into down quark
– why ?!
Manfred Jeitler December 18, 2009 16
discovery of the “charm” quark
predicted by theory (1970) but experimentalists payed no attention !
discovered accidentally (1974) – in the “J/ψ” particle
– Sam Ting and Burt Richter
Manfred Jeitler December 18, 2009 20
another question:are particles completely symmetrical ?
e
imagine as little billiards balls
no room for any asymmetry (left - right)?
few people doubted symmetry
but this conviction was underdetermined– and turned out wrong
Manfred Jeitler December 18, 2009 21
parity violation parity (= mirror-image) symmetry
had not been proved for all interactions
C.N.Yang and T.D.Lee conjectured that parity symmetry might be broken in Weak interactions
– based on experimental evidence
C.S.Wu proved this experimentally– in the same year (1956)
the world’s mirror image differs from the world itself
Manfred Jeitler December 18, 2009 22
Chen Ning Yang and Tsung-Dao Lee(Nobel prize 1957)
Chien-Shiung Wu
parity violation
Manfred Jeitler December 18, 2009 23
save the symmetry!
parity violation came as a shock !
physicists hoped to find the lost symmetry again on a higher level
Manfred Jeitler December 18, 2009 24
Charge-Parity symmetry
Parity
Chargecharge conjugation:replace particles by anti-particles
CP
left-handedneutrino
right-handedneutrino
right-handedanti-neutrino
XIn “Weak Interactions”, P and C “maximally violated” but the combined CP symmetry is mostly conserved
Manfred Jeitler December 18, 2009 25
the next shock:CP symmetry is also broken!
but (rarely) K0L also
decays into two π’s K0
L
K0S
CP = -1CP = -1
CP = +1 CP = +1
K0L
CP = -1
CP = +1
Manfred Jeitler December 18, 2009 27
CP-violation
people were unhappy and proposed other explanations for the experimental findings (1964)
but soon had to accept CP-violation as a fact
theories were developed to explain it
one theory predicted a further “generation” of quarks (1973)
Manfred Jeitler December 18, 2009 28
Makoto Kobayashi
Toshihide Maskawa
Nobel prize 2008 (together with Yoichiro Nambu)
Manfred Jeitler December 18, 2009 29
Vud* Vcd
* Vtd*
Vus* Vcs
* Vts*
Vub* Vcb
* Vtb*
Vud Vus Vub
Vcd Vcs Vcb
Vtd Vts Vtb
1 0 0
0 1 0
0 0 1
the Cabibbo-Kobayashi-Maskawa matrixand the”unitarity triangle“
a 3 x 3 “quark mixing matrix” can explain CP-violation
so, there should be two more quarks (“b” and “t”)– “beauty”, or “bottom”
– “truth”, or “top”
“c” (“charm”) had not yet been found in 1973 !
Manfred Jeitler December 18, 2009 30
mechanism of CP-violaiton
one theory (“Standard Model”) predicted:– 3 generations of quarks
– ε’ not equal 0
another theory (“superweak model”) predicted:– nothing concerning a 3rd generation of quarks
– nothing concerning ε’
question to philosophers:– what would the “realist” conclude ?
– what would the “antirealist” conclude ?
Manfred Jeitler December 18, 2009 31
three generations - why so complex?
CP-violation, three generations ... just a whim of nature?
no!
CP-violation is of fundamental importance for our universe – but nobody had thought of this before
Manfred Jeitler December 18, 2009 33
the Big Bang, antimatter, and us
according to present understanding, the Universe was created in the “Big Bang”
matter and antimatter were created in equal quantities– there is almost no antimatter in the Universe
both would have disappeared if no matter excess had developed
CP-violation is necessary condition! – Sakharov, 1965
Manfred Jeitler December 18, 2009 35
we wouldn’t be around without CP-violation – and lots of other facts
– “fine tuning” of constants of nature
... and so we wouldn’t be able to ask these questions!
anthropic principle– don’t invoke it - it’s not politically correct!
– physicists are supposed to understand everything - not just to show it can’t be otherwise
– although we sometimes use it and don’t care» ever wondered why we live on Earth, and not on Venus or Jupiter?
– people don’t like it - but it might still be the right answer!
but why?
Manfred Jeitler December 18, 2009 36
welcome to the Multiverse !
anthropic principle made socially acceptable
maybe our “Universe” is just a bubble – among uncountably infinitely many other bubbles in the Multiverse – in each bubble universe, one set of laws of physics and natural constants
is realized– just “one point in the parameter landscape”
unless we manage to communicate with other universes:– how?– or find some indirect proof …– is this science or theology?
Manfred Jeitler December 18, 2009 39
Standard Model:Complete and proved? No alternatives?
very good description of nature many predictions
but:
does not describe everything:– e.g., neutrino masses not predicted
one important ingredient still not found in experiment: the HIGGS BOSON– predicted by the mechanism proposed to give mass to quarks
Manfred Jeitler December 18, 2009 40
to Higgs or not to Higgs ...
very good evidence for Standard Model in all other respects
but the “allowed mass window” (masses not yet excluded by experiments or theory) is getting smaller
also, it’s taking so long ...– merely psychological factor?
“theoreticians are getting cold feet” – John Ellis (one of the chief theoreticians at CERN)
lots of new theories (no Higgs after all, invisible Higgs, little Higgs, ... you name it) – much time and little data - theoreticians leave no stone unturned (?)
Manfred Jeitler December 18, 2009 41
bosons
SUSY
SUSY particles. green: known particles of the Standard Model red: hypothetical new particles
for each known elementary particle there should exist a supersymmetric partner
fermions
Supersymmetry
Manfred Jeitler December 18, 2009 42
Atome (Bekannte Materie)
3% Dunkle Materie23%
Dunkle Energie74%
massive astrophysical cosmic halo objects?weakly interacting massive particles?
questions of cosmology to particle physics:Why is there more matter than anti-matter in the universe?What is the universe made of? What is dark matter?What is dark energy?
answers to these questions concerning the largest scales might come from the physics of the smallest scales - elementary particle physics
dark matter: MACHOS vs WIMPS
Manfred Jeitler December 18, 2009 44
data dearth
so many theories
so many explored alternatives
probably some unexplored alternatives (?)
give us data !!
Manfred Jeitler December 18, 2009 46
how to observe particles
Tracks of particles in a typical collider experiment (CMS, CERN)
just
sta
rtin
g !
Manfred Jeitler December 18, 2009 48
LIGO (Laser Interferometer Gravitational Wave Observatory, USA)
measurement of gravitational waves
still
wai
ting
for
sign
al!
Manfred Jeitler December 18, 2009 49
important questions of today’s particle physics(ongoing experiments)
• Where do particles get their mass from? (by interaction with the Higgs particle?)
• Why are these masses so different?
• Is there an overall (hidden) symmetry such as supersymmetry (SUSY) “mirror world” of all known particles?.
• What is the nature of “dark matter” and “dark energy” in the universe?
• Why is there more matter than anti-matter?
• Why have neutrinos such small mass?
• Is there a Grand Unification which combines all interactions, including gravitation?
• Are there extra dimensions, D > 4 ? ( string theory, …)
Manfred Jeitler December 18, 2009 50
where are we now ?
many theories in particle physics are strongly underdetermined at present
numerous conceived alternatives– in violation of Latin grammar, and often also common sense
maybe nature has some unconceived alternatives in store for us?
finally, the Large Hadron Collider is online, and we may hope for some answers
Manfred Jeitler December 18, 2009 53
parity violation parity (= mirror-image) symmetry
had not been proved, however, for all interactions
C.N.Yang and T.D.Lee conjectured that parity might not be conserved in Weak interactions (1956)
– θ 2π (positive parity) and – τ 3π (negative parity) – “τ-θ puzzle”– K+ 2π (positive parity) and – K+ 3π (negative parity)
they convinced C.S.Wu to test parity conservation in experiment
β-decay of 60Cobalt the world’s mirror image differs
from the world itself
Manfred Jeitler December 18, 2009 54
CP-eigenvalue particles can be attributed a
“CP-eigenvalue”– like charge, mass, parity
this eigenvalue is multiplicative:– CP () = -1
– CP () = +1
there are 2 kinds of “neutral K-mesons”
– the (long-lived) K0L decays into
3 -mesons
– the (short-lived) K0S decays into
2 -mesons
K0L and K0
S differ by their CP-eigenvalue !
CP(K0L) = -1 CP(K0
S) = +1
K0L
K0S
CP = -1CP = -1
CP = +1 CP = +1
Manfred Jeitler December 18, 2009 55
CP-violation
K0L
K0S
K0L
CP = -1CP = -1
CP = +1 CP = +1
CP = -1
CP = +1
1964: sometimes (0.3 percent) also
Manfred Jeitler December 18, 2009 56
proton decay?
if baryon number conservation is violated (Sakharov condition #1), the proton could decay– for example, p e+ π0
– no other conservation law forbids this
another argument for possible proton decay: there is no field that corresponds to baryon number conservation– in gauge theories, long-range fields give rise to absolutely conserved
quantities
proton decay is definitely very slow– good for us: else, we would have problems with radiation damage!
experimental limits very low– half-life > 1036 years (“Superkamiokande” detector, Japan)
spin-off: neutrino detectors
Manfred Jeitler December 18, 2009 57
• the Standard Model works only with particles which are originally massless!• mass is created through interaction with a (hypothetical) Higgs field• due to spontaneous symmetry breaking this field is present everywhere in the universe• “oscillations” in the Higgs field manifest themselves as Higgs particles, which should be observed at LHC / CERN over the next few years
spontaneous symmetry breaking
energy
Higgs field
hot universe(soon after big bang)
cold universe(condensates in an asymmetric state with Higgs field)0
v
particles are massless
particles acquire mass
the Higgs boson