Term
QM + Special relativity =? who's theory? what is needed to make theory work? |
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Definition
Relativistic QM Paul Dirac Need add. particle for every currently observed particle |
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Term
Matter and Anti Matter of basic particles |
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Definition
Matter Antimatter
p+ ¯p- (anti-proton)
e- e+ (positron)
n ¯n (anti-neutron)
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Term
Positron e+ and electron e- tracks |
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Definition
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Term
How did carl anderson discover the positron |
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Definition
Placed metal bar in center of detection field.
Loses energy when hits bar, can see from where it came
Because the direction of the tracks..
must be positively charged= e+ |
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Term
Where do e+ particles come from? |
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Definition
From cosmic rays= emit high energy sttuff
Nature's accelerator |
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Term
A theory by Pukawa predicted that what mediated strong interaction
mass? |
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Definition
particles called pions
approx. mass of electron |
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Term
How was the muon discovered
What is it? |
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Definition
discovered in photographic emulsion that was exposed to cosmic rays.Did not interact with protons
The muon= secong gen particle that looked like a heavier electron |
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Term
Why do the most interesting cosmic ray events occur at high alts? |
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Definition
Have better chance of seeing unstable aprticles at higher alts |
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Term
Strange particles
How were they identified?
mass? |
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Definition
make "v" like tracks
produced by a new particle= k particles
mass=1/2 of proton |
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Term
Pauli invented what particle?
Why?
Problem with neutrino |
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Definition
Neutrino
to help with the problem of conserving E and P
Can't interact with EM, need new force |
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Term
Klein proposed what to mediate force in weak force interactions |
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Definition
W particle
like pions and strong force |
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Term
How was the neutrino discovered? |
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Definition
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Term
What is a baryon?
what are not? |
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Definition
Something that consists of 3 quarks
pi, muon, electron and k particles |
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Term
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Definition
the # of strange quarks
get more strangeness the more mass you have |
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Term
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Definition
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Term
Particle accelerators were invented to do what?
unit? |
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Definition
to control production of large #s of particles
to produce high-energy beams
Use E and B field combos to ramp up energy of particles.
Unit= elecron volt |
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Term
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Definition
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Term
in the 50's how did particles show up as in scatering data?
Why couldn't they see them? |
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Definition
Resonances (series of particles)
Particles decayed too fast~10-23 sec |
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Term
all types of quarks
charge and strangeness |
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Definition
q s
u=up +2/3 0
d=down -1/3 0
c-charm +2/3
s=strange -1/3 -1
t-top +2/3
b-bottom -1/3 |
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Term
How was the quark model proved
what did they find |
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Definition
used a linear accelerator
shot electron beam at liquid hydrogen
if proton was ball of energy-expect beam to go right through=not observed
OBSERVED= back scattering-happens if had quarks
constituents.
found: 3 quark constituents
proton=uud
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Term
Quark model (baryons and mesons) |
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Definition
All observable particles are either
baryons= 3 quark combo=q1 q2 q3
eg. (p,n, sigma+)
or Mesons= quark–antiquark pairs1 ¯q2
eg. (k+, pi+)
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Term
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Definition
strong force is so strong that particle–antiparticle pairs are produced before quark can seperate |
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Term
November revolution. e- and e+ collider and SPEAR and exp. at AGS observed what?
What did this lead to? |
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Definition
new fairly stable particle
name= J/4
new meson w/charm quark
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Term
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Definition
tau
leptons: Q
tau neutrino= 0
tau = -1
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Term
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Definition
bottom quark
Quark Q
T-top = +2/3
b-bottom = -1/3 |
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Term
Why did it take so long to discover the top-quark |
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Definition
very large mtop=170 GEV
mbottom =4.7 GEV |
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Term
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Definition
electromagnetic — photons
weak — w-,w+, z0 |
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Term
Quantum Chromodynaimcs was theorized for what |
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Definition
for strong interactions between quarks
used generalized photons (gluons) |
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Term
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Definition
3 types of elec charge for quarks
COLORS! red, gree, blue
8-diff colored gluons in this theory |
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Term
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Definition
all observable paarticles must be color neutral or white
white= 3 quarks or particle-anti particle combo |
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Term
problem with color theory
what was invented to fix this |
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Definition
theory requires all matter problems to be massless (weak interaction theory)
Invented Higgs particle to fix this and generate mass. |
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Term
How does the Higgs particle work/fix prob |
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Definition
At very high temps=higgs behaves as force mediator
at low energies, Higgs field freezes out=generates mass. |
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Term
Force carrier particles (4) |
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Definition
QED=electromagnetic — photons
?=Weak Force — w+,w-, z0
QCD=Strong force — gluons
Higgs — H |
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Term
Neutrino physics: solar neutrino problem encountered |
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Definition
discrepancy btwn solar Ve production and the # of neutrinos observed from sun.
saw only 1/2 of predicted particles
reason: Neutrinos can cause oscillations=mass |
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Term
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Definition
certain cloud like gases=galaxies |
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Term
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Definition
intrinsic brightness or power of star to emit light |
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Term
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Definition
a particular type of star that varied in brightness over time.
Period of oscillation realted to luminosity-standard candle
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Term
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Definition
measure distance that the stat moves during the year
Variable star brightness: the shorter the period, the dimmer the star
the longer the period, the brighter the star. |
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Term
How to measure distance to star
what did hubble realize |
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Definition
use star luminosity which is gained from stellar parallox
this allowed hubble to see that the cloud of gas he saw was 100 x further away than any star in our galaxy=universe is huge |
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Term
To test motion of a star:
what did this show |
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Definition
Doppler effect, a star in motion and its light wavelength shift corresponds to color shift.
For star moving away, spectrum is red-shifted.
showed that galaxies are moving away from us |
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Term
Einstein's biggest blunder |
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Definition
was developing general relativity, found equation had no time independent solutions. Always found either contration or expansion of space. Decided to include an extra term to get rid static solution.
w/out the constant he had redicted the expanding universe |
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Term
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Definition
71(km/s)/ mpc
mega=3 million light years
1 par sec=3.26 light years |
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Term
what happened about 8 bil. yrs ago |
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Definition
sun and planets begin to form
when stars collapse, they create all the elements and as it explodes, elements shoot off and end in gases where gravity pulls dense objects togther |
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Term
Timeline of early galaxy
8 bil
6 bil
1 bil
300,00
3 mins
10-6sec
10-12sec |
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Definition
8 bil yrs old=sun and planets begin to form
6 bil yrs old=milky way galaxy is in forming
1 bil yrs old = first stars are forming structure formation
300,000 yrs old= entire univ=one big molecule
-light did not propogate -as sson as light was emitted it was absorbed by another atom
at 3 mins old=entire univ was one giant nucleus
at 10-6 sec= univ=one gigantic nucleon (quarks and gluons)
at 10-12sec= Higgs particle melts-all particles are massless prior to 10-12 sec.
get restoration of symmetry btwn EM and weak force
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Term
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Definition
No idea-purely theoretical
possibly grand unification-symmetry would include strong force
need to include gravity in quantum way |
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Term
In big bang theory what changed after 300,000 yrs |
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Definition
light was able to freely travel through univ for 1st time
prior to 300,000=univ=one big molecule (plasma)
after=atoms form, more space, univ transperant to light
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Term
How was cosmic microwave background radiation discovered?
what is it? |
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Definition
used a radio antenna to look at sources in our galaxy
instrument was sensitive to low intensity radio and microwaves
heard random noise in the signal
thought it was pigions..but signal was still there
realized it was a real physical signal the CMBR
When an object radiates energy it does so across a variety of wavelengths |
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Term
How do we know the earth is not at rest |
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Definition
if it was you would see equal light in all directions-which we don't |
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Term
what happened 3 mins into the big bang |
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Definition
Nucleosynthesis- creation of new atomic particles from nucleoons (quarks and gluons)
which can be ued to measure the density of matter |
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Term
where do heavier elements come from |
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Definition
collapsing stars= when large stars collapse=supernova, heavier elements are created |
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Term
the collapse process of stars |
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Definition
at some point, a few billion yrs after star is formed, it burns up all the H fuel
gravity then takes over and it collapses the star material
then gets hotter and fusion begins again making heavier elements
then=BIG EXPLOSION-elements shoot off, emit light that can emit light brighter than the galaxy it is in. |
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Term
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Definition
- speeds of stars don't agree with calculations
pos. solutions.=
A.modify newtonian gravity-hard to do in a way that works with gen. relativity
B. Dark Matter-much more mass than is seen
-must not interact with photons or EM force
-neutrinos could work but are much too light
-motions of galaxies appear to be missing mass
Gravitational lensing=how mass cluster bend lights and affectd how we see stars-calculated mass is much larger than observed mass
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Term
Problems w/ Gravitational Lensing
indicates what? |
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Definition
frequently indentifies dark matter
more matter needed to bend the light to agree with calcs-90% is missing |
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Term
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Definition
don't know
but...doesn't interact with photon, if it did you would see it
3 catagories
1) Hot dark matter-ultra-relativistic speeds,close to c
2) warm darm matter: slower than hot but still relativistic
3) cold dark matter:slowly moving =, non-relativistic speeds. |
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Term
Some dark mater candidates |
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Definition
1) MACHOS-Massive compact hale objects
-small invisible objects made of ordinary matter
2) WIMPS- weakly interacting massive particles
-postulate particles that interact only via weak interactions
idea: early univ-electrons and positrons and high energy collide to produce WIMPS
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Term
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Definition
when directly in front of star --get brief brightening of star when MACHO passes in front |
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Term
Problem with the explanation of MACHOS as dark matter |
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Definition
a. These events are very rare, 90% of matter should be happening more frequently
b. Nucleosynthesis-4% baryons
if this was right nucleosynthesis would be wrong (closer to one) |
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Term
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Definition
no wimps have ever been in an experiment |
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Term
Bar vogenesis Theories
tries to explain what? |
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Definition
Process that violates Baryon # conservation, these occur in grand unified theories (GUTs)
why there is anti-matter and matter in the univ.
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Term
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Definition
a. Age problem or flatness prob.
-ballance btwn matter and initial kenetic energy to get univ to live longer than 14 billion yrs
b. Smoothness prob.- CMBR is uniform across sky~same temp in regions that have never been thermal contact
c. Lumpiness prob. -universe is not a symmetrical ball of gas |
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Term
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Definition
Our universe is expanding at an exponential rate
fixes prob of flatness problem=curvature naturally flattens out-universe large automatically due to inflation
fixes prob of smoothness-small bit @same temp initially
fixes prob of lumpiness-might have small quantum fluctuations of "small bit"-tiny QF's can expand to structure of univ. |
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Term
alt. theories to inflation |
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Definition
1)cyclic models for univ.-repeated expansion and contraction in cycle- univ. oscillates
-string theory
2) Cosmic strings-field at GUT scale can wrap up into sring like structures that extend across large portions of univ.-studies of CMBR don't match model |
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Term
Supernovae-prob with hubble law
explanations? |
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Definition
supernovae too dim
1)dust--bt only happens at great distances
2) universe is accelerating expansion
-dark matter may be why gravity is isn't causing deceleration as it should
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Term
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Definition
omega>1=energy density is large enough for recollapse
omega<1=not enough energy density for re collapse
omega=1=flat |
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Term
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Definition
1) luminous matter (baryons)
2) Dark matter?
3) Dark energy |
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Term
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Definition
1. initial guess-based on observations
2. compute consequences of guess
compare calculated consequences w/expts
4. if expts disagree with consequences, then theory is wrong |
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Term
Fullman and Zweig developed what? |
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Definition
Quark model-
developed substructure of all mesons and baryons |
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Term
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Definition
generalized electromagnetic force-photon to incorporate weak force- z,w,w,gamma
needed to break smmetry using higgs to get theory to work. |
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Term
Strong force and Quark color |
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Definition
a further generalization of symmetry used in electroweak (w/out the breaking higgs)
QCD-
1 photon—8 gluons |
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Term
Problem with qravity and QM theory |
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Definition
THere are no quantum versions of theory
and cannot test... |
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Term
Kaluza-Klein theory
prob: |
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Definition
wrote down theory of gravity in 4 space dimensions in one time
not visually defined, but mathwise works fine
curled up extra demension into tiny circle that you cant see
prob:makes prediction that EM force is equal to the strength of gravity. |
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Term
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Definition
an attempt to undrstand meson dynamics
didn't work
came back as fndamental theory of nature
quarks, leptons, photons etc=variety of string occilations
included closed string--behaves like gravity-graviton
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Term
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Definition
lowest string mode for closed string was tachyon (not graviton)
tachyon= particle that always is faster than c
but don't really exist
===UNSTABLE
prob 2: need to curl up extra demensions to get theory to work in 4d
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Term
String theory:
using supersymmetry |
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Definition
each observed particle must have a superpartner
photon — photino
electron — selectron
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