Danish Institute for Advanced Study Lecture Series

Effective  Field  Theory  of  Gravity:  When  General     Relativity  and  Quantum  Mechanics  Meet   Alessandro Codello DIAS Universe

Friday, 28 March 2014 12:00, CP3 seminar room www.dias.sdu.dk

A TALE OF TWO FORCES from coulomb’s law to quantum gravity

electrostatics (gauss’s law)

V

S

flux of the electric field trough S is equal to the total electric charge in V

coulomb’s law

q Q

first published by Coulomb in 1785

coulomb’s law

q

Q 2 4πr E = �0 Q E= 4π�0 r2

Q

first published by Coulomb in 1785

coulomb’s law

q

Q 2 4πr E = �0 Q E= 4π�0 r2

Q

F = qE dV F =− dr Q V = 4π�0 r

first published by Coulomb in 1785

magnetostatics (gauss’s law)

S

flux of the magnetic field through S is zero (there are no magnetic monopoles!)

ampere’s law and lorentz’s force

2πrB = µ0 I

I

µ0 I B= 2πr

F = q(E + v × B)

faraday’s law

maxwell/ampere law

time dependent magnetic fields generate electric fields and vice versa!

vacuum maxwell’s equations

vacuum maxwell’s equations

wave equation...

...and there be light!

...and there be light!

1 8 −1 c= √ = 2.99792458 × 10 m s µ0 � 0

special relativity c time

space

understood by Einstein in 1905

special relativity c time

space

E = mc

2

fields of a moving charge 1 E∼B∼ 2 r 1 EB ∼ 4 r 1 4πr EB ∼ 2 → 0 r 2

a charge in uniform motion does not radiate...

radiation from an accelerating charge

radiation from an accelerating charge

  q  1 E= 2 4π�0  R 

� �� ˆ × R ˆ − v × a2  � v R ˆ R− c c c 1 � � � �3 + � �3  � R v v  2 ˆ ˆ γ 1−R· c 1−R· c � ��

� 1 ˆ � B = R × E� c ret



ret

radiation from an accelerating charge

radiation from an accelerating charge

radiation from an accelerating charge

classical electrodynamics

a theory of photons and electrons

quantum electrodynamics







Feynman diagrams (the sixties)

corrections to coulomb’s interaction

+

+ .. . photons are the mediators of electromagnetic interactions

vacuum polarization

empty space is a dielectric medium of electron-positron dipoles

running charge

an electric charge is screened by a cloud of electron-positron pairs

effective field theory

at low energy just a modified classical theory

gravity (gauss’s law)

V

S

flux of the gravitational field trough S is equal to the mass in V

newton’s law

G

foud by Isaac Newton in the 17th century

newton’s law

mM F = −G 2 r dV F =− dr

G

mM V = −G r

foud by Isaac Newton in the 17th century

gravitational radiation

only quadrupoles radiate

discovered indirectly by Hulse and Taylor in 1973 observing a system of binary pulsars

binary neutron stars

classical gravity

the source of the gravitational field is mass-energy and the field carries it: self-interaction!

.. .

.. .

+

+

+

+

+ .. .

+ .. .

+

+

+

+

+ .. .

+ .. .

=

=

curvature

energy–momentum

this incredible sum was performed by Deser 1973

general relativity

curvature

=

energy–momentum

developed by Albert Einstein in 1916

quantum gravity

.. .

.. .

quantum gravity

.. .

.. . G

c



corrections to newton’s interaction

corrections to newton’s interaction �

=





iκ 3 µν 2 µ ν µ ν µ ν Pαβ,γδ k k + (k − q) (k − q) + q q − η q 2 2 � � +2qλ qσ I λσ,αβ I µν,γδ + I λσ,γδ I µν,αβ − I λµ,αβ I σν,γδ − I σν,αβ I λµ,γδ � � � � � + qλ q µ ηαβ I λν,γδ + ηγδ I λν,αβ + qλ q ν ηαβ I λµ,γδ + ηγδ I λµ,αβ � � � µν, µν, 2 µν λ σ −q ηαβ I γδ + ηγδ I αβ − η q q (ηαβ Iγδ,λσ + ηγδ Iαβ,λσ ) � � λ + 2q I σν,αβ Iγδ,λσ (k − q)µ + I σµ,αβ Iγδ,λσ (k − q)ν � σν, σµ, −I γδ Iαβ,λσ k µ − I γδ Iαβ,λσ k ν � � � �� σµ, σµ, ρσ, ρσ, +q 2 I αβ Iγδ,σν + Iαβ,σν I αδ + η µν q λ qσ Iαβ,λρ I γδ + Iγδ,λρ I αβ � � � � 2 � 1 µν σµ, σν, µ 2 ν + k + (k − q) I αβ Iγδ,σ + I αβ Iγδ,σ − η Pαβ,γδ 2 � ��� − k 2 ηγδ I µν,αβ + (k − q)2 ηαβ I µν, γδ the truth behind Feynman diagrams...

corrections to newton’s interaction

V =−

� GM m r

G� G(M + m) 1+a + b + · · · c2 r c3 r 2



corrections to newton’s interaction

V =−

� GM m r

m3 [G] = Kg s2

G� G(M + m) 1+a + b + · · · c2 r c3 r 2 m2 Kg [�] = s



m [c] = s

corrections to newton’s interaction

V =−

� GM m r

41 G� G(M + m) 1+3 + + ··· 2 3 2 c r 10π c r

leading quantum corrections to newton’s law first computed in 1994 by John Donoghue



corrections to newton’s interaction

GM⊙ −6 ∼ 10 c 2 r⊙ G� −88 ∼ 10 2 3 c r⊙

sun

leading quantum corrections to newton’s law are incredibly small!

can we ever observe quantum gravity effects?

cosmos

can we ever observe quantum gravity effects?

cosmos maybe there are some inside here?

Thank you

2014-03-28-codello.pdf

Page 1 of 46. Danish Institute for Advanced Study. Lecture Series. Effective(Field(Theory(of(Gravity:(When(General(. Relativity(and(Quantum(Mechanics(Meet. Alessandro Codello. DIAS Universe. Friday, 28 March 2014. 12:00, CP3 seminar room. www.dias.sdu.dk. Page 1 of 46 ...

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