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Some open questions in physics Krzysztof A. Meissner Instytut Fizyki Teoretycznej UW Instytut Problem ´ ow Ja ¸ drowych Kraków, 23.10.2009 K.A. Meissner, Unsolved problems – p. 1/25

Krzysztof A. Meissner Instytut Fizyki Teoretycznej UW ... · Some open questions in physics Krzysztof A. Meissner Instytut Fizyki Teoretycznej UW Instytut Problemow Ja¸drowych´

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Some open questions in physics

Krzysztof A. MeissnerInstytut Fizyki Teoretycznej UWInstytut Problemow Jadrowych

Kraków, 23.10.2009

K.A. Meissner, Unsolved problems – p. 1/25

Content

• Quantum Mechanics• Standard Model• dark matter and dark energy• quantum gravity• summary

K.A. Meissner, Unsolved problems – p. 2/25

The most incomprehensible fact about theUniverse is that it is comprehensible

A. Einstein

K.A. Meissner, Unsolved problems – p. 3/25

Introduction

• (part of) reality can be described by numbers• there are correlations among these numbers

– physical laws• with proper idealization these laws seem to

be universal and rigorous

K.A. Meissner, Unsolved problems – p. 4/25

Introduction

• (part of) reality can be described by numbers• there are correlations among these numbers

– physical laws• with proper idealization these laws seem to

be universal and rigorous• we have no idea why these statements hold

the answer belongs to meta-physics ratherthan physics...

K.A. Meissner, Unsolved problems – p. 4/25

Introduction

• use of mathematics is the source oftremendous success of physics

K.A. Meissner, Unsolved problems – p. 5/25

Introduction

• use of mathematics is the source oftremendous success of physics

• but mathematics gives us also a rigorousproof that cognition has its limits:

Gödel theorem + finite resources⇓

“Theory of Everything” is impossible

K.A. Meissner, Unsolved problems – p. 5/25

Introduction

• in any physical phenomenon we distinguish“accidental” properties (depending on theinitial conditions)and “inevitable” properties (following from thelaws of physics)

K.A. Meissner, Unsolved problems – p. 6/25

Introduction

• in any physical phenomenon we distinguish“accidental” properties (depending on theinitial conditions)and “inevitable” properties (following from thelaws of physics)

• the fact that there are 8 (formerly 9) planetsseems to be “accidental” but once we have aplanet a3 ∼ T 2 is “inevitable”

K.A. Meissner, Unsolved problems – p. 6/25

Introduction

• in any physical phenomenon we distinguish“accidental” properties (depending on theinitial conditions)and “inevitable” properties (following from thelaws of physics)

• the fact that there are 8 (formerly 9) planetsseems to be “accidental” but once we have aplanet a3 ∼ T 2 is “inevitable”

• explanation in physics means converting“accidental” into “inevitable”

K.A. Meissner, Unsolved problems – p. 6/25

Introduction

• in any physical phenomenon we distinguish“accidental” properties (depending on theinitial conditions)and “inevitable” properties (following from thelaws of physics)

• the fact that there are 8 (formerly 9) planetsseems to be “accidental” but once we have aplanet a3 ∼ T 2 is “inevitable”

• explanation in physics means converting“accidental” into “inevitable”

• how far can we go?

K.A. Meissner, Unsolved problems – p. 6/25

Cube of theoriesFundamental dimensionful constants: 1/c, ~, G

K.A. Meissner, Unsolved problems – p. 7/25

Quantum Mechanics

• the most fundamental and extremelysuccessful in our description of the physicalworld but...

K.A. Meissner, Unsolved problems – p. 8/25

Quantum Mechanics

• the most fundamental and extremelysuccessful in our description of the physicalworld but...

• conceptual foundations (and limits) of locality,causality, Heisenberg relations unclear

K.A. Meissner, Unsolved problems – p. 8/25

Quantum Mechanics

• the most fundamental and extremelysuccessful in our description of the physicalworld but...

• conceptual foundations (and limits) of locality,causality, Heisenberg relations unclear

• problem of measurement (Copenhagen,Everett, Bohm, Penrose, ...) totally unclear...

K.A. Meissner, Unsolved problems – p. 8/25

Particles of the Standard Model• Leptons (spin 1/2, qν = 0, qe = −1):

νe

e

L

νµ

µ

L

ντ

τ

L

eR, νeRµR, νµR τR, ντR

• Quarks (3 colors, spin 1/2, qu = 2/3, qd = −1/3):

u

d

L

c

s

L

t

b

L

uR, dR cR, sR tR, bR

• Spin 1: 8 gluons g (SU(3)),

W± and Z0, photon γ (SU(2) × U(1))

• Spin 0: Higgs H

K.A. Meissner, Unsolved problems – p. 9/25

Standard Model• extremely successful theory

• no single experimental deviation• verified to unbelievable precision

but it cannot be the ultimate theory...

K.A. Meissner, Unsolved problems – p. 10/25

Standard Model• extremely successful theory

• no single experimental deviation• verified to unbelievable precision

but it cannot be the ultimate theory...• no gauge anomalies ⇒

# of leptons = # of quarksbut why 3 generations???

K.A. Meissner, Unsolved problems – p. 10/25

Standard Model• extremely successful theory

• no single experimental deviation• verified to unbelievable precision

but it cannot be the ultimate theory...• no gauge anomalies ⇒

# of leptons = # of quarksbut why 3 generations???

• why the observed values of masses andcoupling constants???any change ⇒ we are not here...

K.A. Meissner, Unsolved problems – p. 10/25

Standard Model• extremely successful theory

• no single experimental deviation• verified to unbelievable precision

but it cannot be the ultimate theory...• no gauge anomalies ⇒

# of leptons = # of quarksbut why 3 generations???

• why the observed values of masses andcoupling constants???any change ⇒ we are not here...

• why CP violation (and why not enough)???

K.A. Meissner, Unsolved problems – p. 10/25

Standard Model• why spontaneous symmetry breaking〈H〉 = v 6= 0???

K.A. Meissner, Unsolved problems – p. 11/25

Standard Model• why spontaneous symmetry breaking〈H〉 = v 6= 0???

• why such huge differences in masses???

mt

v≈ 1,

me

v≈ 3 · 10−6,

(mν

v≈ 10−12

)

K.A. Meissner, Unsolved problems – p. 11/25

Standard Model• why spontaneous symmetry breaking〈H〉 = v 6= 0???

• why such huge differences in masses???

mt

v≈ 1,

me

v≈ 3 · 10−6,

(mν

v≈ 10−12

)

• why proton mass ≈ 1 GeV???(main source of luminous mass)

K.A. Meissner, Unsolved problems – p. 11/25

Standard Model• why spontaneous symmetry breaking〈H〉 = v 6= 0???

• why such huge differences in masses???

mt

v≈ 1,

me

v≈ 3 · 10−6,

(mν

v≈ 10−12

)

• why proton mass ≈ 1 GeV???(main source of luminous mass)

• hierarchy problemv

MP≈ 10−16

(supersymmetry, conformal symmetry)

K.A. Meissner, Unsolved problems – p. 11/25

Present content of the Universe

radiation p ≈ ρ3

negligibleluminous matter p ≈ 0 4 %

(stars 0.5%interstellar gas 0.5%intergalactic gas 3%)

dark matter p ≈ 0 23 %dark energy p ≈ −ρ 73 %

K.A. Meissner, Unsolved problems – p. 12/25

Nucleosynthesis abundances

K.A. Meissner, Unsolved problems – p. 13/25

WMAP

K.A. Meissner, Unsolved problems – p. 14/25

Dark Matter and Dark Energy

• what is dark matter (supersymmetricneutralino, axion, ...)?

K.A. Meissner, Unsolved problems – p. 15/25

Dark Matter and Dark Energy

• what is dark matter (supersymmetricneutralino, axion, ...)?

• the answer probably within conventional QFT

K.A. Meissner, Unsolved problems – p. 15/25

Dark Matter and Dark Energy

• what is dark matter (supersymmetricneutralino, axion, ...)?

• the answer probably within conventional QFT• what is dark energy (cosm. constant?)???

K.A. Meissner, Unsolved problems – p. 15/25

Dark Matter and Dark Energy

• what is dark matter (supersymmetricneutralino, axion, ...)?

• the answer probably within conventional QFT• what is dark energy (cosm. constant?)???• why

ρDM

M 4

P

≈ 10−120,ρDM

M 4

W

≈ 10−54

K.A. Meissner, Unsolved problems – p. 15/25

Dark Matter and Dark Energy

• what is dark matter (supersymmetricneutralino, axion, ...)?

• the answer probably within conventional QFT• what is dark energy (cosm. constant?)???• why

ρDM

M 4

P

≈ 10−120,ρDM

M 4

W

≈ 10−54

• the answer probably requires new (not QFTlike) physics – quantum gravity?

K.A. Meissner, Unsolved problems – p. 15/25

Galaxy collision

K.A. Meissner, Unsolved problems – p. 16/25

Gravity• gravitational interaction between elementary

particles is extremely weak – why???

αG =Gm2

p

~c≈ 10−38

(for EM interactions α = e2/(4πǫ0~c) ≈ 1/137)

K.A. Meissner, Unsolved problems – p. 17/25

Gravity• gravitational interaction between elementary

particles is extremely weak – why???

αG =Gm2

p

~c≈ 10−38

(for EM interactions α = e2/(4πǫ0~c) ≈ 1/137)• αG is so small ⇒ stars are so large

MC ≈ mp

α3/2G

≈ 1030kg

(Chandrasekhar limit)

K.A. Meissner, Unsolved problems – p. 17/25

Quantum Gravity• when gravity ≈ EM? (G. Stoney, 1881)

Gm2

S

r2=

e2

4πǫ0 r2⇒ mS ≈ 1.86 · 10−9 kg

K.A. Meissner, Unsolved problems – p. 18/25

Quantum Gravity• when gravity ≈ EM? (G. Stoney, 1881)

Gm2

S

r2=

e2

4πǫ0 r2⇒ mS ≈ 1.86 · 10−9 kg

• Planck (1899) introduced (mP =√

αmS)

mP =√

~cG ≈ 2.176 · 10−8 kg

we expect that QG sets in when E → mP c2

K.A. Meissner, Unsolved problems – p. 18/25

Quantum Gravity• when gravity ≈ EM? (G. Stoney, 1881)

Gm2

S

r2=

e2

4πǫ0 r2⇒ mS ≈ 1.86 · 10−9 kg

• Planck (1899) introduced (mP =√

αmS)

mP =√

~cG ≈ 2.176 · 10−8 kg

we expect that QG sets in when E → mP c2

• QG – “fluctuating space-time” (???)

K.A. Meissner, Unsolved problems – p. 18/25

Quantum Gravity• when gravity ≈ EM? (G. Stoney, 1881)

Gm2

S

r2=

e2

4πǫ0 r2⇒ mS ≈ 1.86 · 10−9 kg

• Planck (1899) introduced (mP =√

αmS)

mP =√

~cG ≈ 2.176 · 10−8 kg

we expect that QG sets in when E → mP c2

• QG – “fluctuating space-time” (???)• black hole entropy may be the key issue

pointing to QG (as black body radiation did)

K.A. Meissner, Unsolved problems – p. 18/25

Cube of theoriesFundamental dimensionful constants: 1/c, , ~, G

K.A. Meissner, Unsolved problems – p. 19/25

Quantum gravity – proposals• very interesting results from the (Lorentzian)

path-integral approach (DynamicalTriangulations)

K.A. Meissner, Unsolved problems – p. 20/25

Quantum gravity – proposals• very interesting results from the (Lorentzian)

path-integral approach (DynamicalTriangulations)

• String Theory• Loop Quantum Gravity

K.A. Meissner, Unsolved problems – p. 20/25

Quantum gravity – proposals• very interesting results from the (Lorentzian)

path-integral approach (DynamicalTriangulations)

• String Theory• Loop Quantum Gravity

• both claim solving BH entropy problem• neither solved the CC problem• nor the initial singularity and initial

conditions problems ...

K.A. Meissner, Unsolved problems – p. 20/25

String theory

• Quantum description of gauge theories andgravity

K.A. Meissner, Unsolved problems – p. 21/25

String theory

• Quantum description of gauge theories andgravity

• UV finite (?) – modular symmetry (not provenbeyond two loops)

K.A. Meissner, Unsolved problems – p. 21/25

String theory

• Quantum description of gauge theories andgravity

• UV finite (?) – modular symmetry (not provenbeyond two loops)

• extremely beautiful mathematically

K.A. Meissner, Unsolved problems – p. 21/25

String theory

• Quantum description of gauge theories andgravity

• UV finite (?) – modular symmetry (not provenbeyond two loops)

• extremely beautiful mathematically• but...

K.A. Meissner, Unsolved problems – p. 21/25

String theory

• lack of underlying principle

K.A. Meissner, Unsolved problems – p. 22/25

String theory

• lack of underlying principle• only first quantized formulation with unknown

equations of motion

K.A. Meissner, Unsolved problems – p. 22/25

String theory

• lack of underlying principle• only first quantized formulation with unknown

equations of motion• theory contains higher-dimensional objects

(branes) – no consistent quantum description

K.A. Meissner, Unsolved problems – p. 22/25

String theory

• lack of underlying principle• only first quantized formulation with unknown

equations of motion• theory contains higher-dimensional objects

(branes) – no consistent quantum description

• > 10500 admissible (?) vacua (landscape)

K.A. Meissner, Unsolved problems – p. 22/25

String theory

• lack of underlying principle• only first quantized formulation with unknown

equations of motion• theory contains higher-dimensional objects

(branes) – no consistent quantum description

• > 10500 admissible (?) vacua (landscape)• no mechanism to break supersymmetry to

leave QFT on almost flat space

K.A. Meissner, Unsolved problems – p. 22/25

String theory

• lack of underlying principle• only first quantized formulation with unknown

equations of motion• theory contains higher-dimensional objects

(branes) – no consistent quantum description

• > 10500 admissible (?) vacua (landscape)• no mechanism to break supersymmetry to

leave QFT on almost flat space• no single new result relevant for “low energy”

particle physics or cosmology

K.A. Meissner, Unsolved problems – p. 22/25

Loop Quantum Gravity

• defined quantum mechanically

K.A. Meissner, Unsolved problems – p. 23/25

Loop Quantum Gravity

• defined quantum mechanically• diffeomorphism invariance (background

independence) built in and onlydiffeomorphism invariant operators allowed(volume, area...)

K.A. Meissner, Unsolved problems – p. 23/25

Loop Quantum Gravity

• defined quantum mechanically• diffeomorphism invariance (background

independence) built in and onlydiffeomorphism invariant operators allowed(volume, area...)

• but no connection (yet?) to usual gravity

K.A. Meissner, Unsolved problems – p. 23/25

Loop Quantum Gravity

• defined quantum mechanically• diffeomorphism invariance (background

independence) built in and onlydiffeomorphism invariant operators allowed(volume, area...)

• but no connection (yet?) to usual gravity• no dynamics• mathematically very difficult (inseparable

Hilbert spaces, forbiddingly complicatedhamiltonian etc.)

K.A. Meissner, Unsolved problems – p. 23/25

Loop Quantum Gravity

• defined quantum mechanically• diffeomorphism invariance (background

independence) built in and onlydiffeomorphism invariant operators allowed(volume, area...)

• but no connection (yet?) to usual gravity• no dynamics• mathematically very difficult (inseparable

Hilbert spaces, forbiddingly complicatedhamiltonian etc.)

K.A. Meissner, Unsolved problems – p. 23/25

Quantum Gravity

• no sign of convergence of differentapproaches

K.A. Meissner, Unsolved problems – p. 24/25

Quantum Gravity

• no sign of convergence of differentapproaches

• problems of initial singularity, existence (oremergence) of time and space at distances∼ lP , interpretation of the “wave function ofthe Universe” etc. totally unclear

K.A. Meissner, Unsolved problems – p. 24/25

Quantum Gravity

• no sign of convergence of differentapproaches

• problems of initial singularity, existence (oremergence) of time and space at distances∼ lP , interpretation of the “wave function ofthe Universe” etc. totally unclear

• we are still very far away from understandingquantum gravity

K.A. Meissner, Unsolved problems – p. 24/25

Summary

• list of unsolved problems doesn’t getshorter...

K.A. Meissner, Unsolved problems – p. 25/25

Summary

• list of unsolved problems doesn’t get shorter...• probably the biggest challenges in physics

(that we know of!)• measurement problem in QM• explanation of values of physical constants• cosmological constant and quantum gravity

K.A. Meissner, Unsolved problems – p. 25/25

Summary

• list of unsolved problems doesn’t get shorter...• probably the biggest challenges in physics

(that we know of!)• measurement problem in QM• explanation of values of physical constants• cosmological constant and quantum gravity

• the biggest (meta-physical) mystery:why anything is subject to any law at all?

K.A. Meissner, Unsolved problems – p. 25/25

Summary

• list of unsolved problems doesn’t get shorter...• probably the biggest challenges in physics

(that we know of!)• measurement problem in QM• explanation of values of physical constants• cosmological constant and quantum gravity

• the biggest (meta-physical) mystery:why anything is subject to any law at all?

• Socrates’ statement invariably true:“I neither know nor think that I know”

K.A. Meissner, Unsolved problems – p. 25/25