early universe What is magnetic helicity The myth of catastrophic - - PowerPoint PPT Presentation

early universe
SMART_READER_LITE
LIVE PREVIEW

early universe What is magnetic helicity The myth of catastrophic - - PowerPoint PPT Presentation

Helical magnetic fields in the early universe What is magnetic helicity The myth of catastrophic quenching Magn helicity in decaying turbulence The chiral magnetic effect Gravitational waves from the resulting turbulence Axel


slide-1
SLIDE 1

1

Helical magnetic fields in the early universe

Axel Brandenburg (Nordita, Stockholm)

  • What is magnetic helicity
  • The myth of catastrophic quenching
  • Magn helicity in decaying turbulence
  • The chiral magnetic effect
  • Gravitational waves from the

resulting turbulence

slide-2
SLIDE 2

2

elix

Curling tendril  Climbing plant Biophysics: Helix Chirality

slide-3
SLIDE 3

3

Helical structures on the Sun (X-ray emission)

Coronal mass ejections

Helicity & topology: math. underpinnings

slide-4
SLIDE 4

4

Helical structures on the Sun (X-ray emission)

Coronal mass ejections

slide-5
SLIDE 5

5

Moffatt coined the term in hydro/MHD

Coronal mass ejections

slide-6
SLIDE 6

6

Magnetic helicity measures linkage of flux

 

V

V H d B A

1

2

2 1

2     H

 

  

1 1

d d

1 S L

H S B A 

2

d

2

      

S

S A

1

S

1

  A B   

Therefore the unit is Maxwell squared

slide-7
SLIDE 7

What produces helicity?

Cyclones: Down: faster Up: slower

north south

g W g W

 u ω  u ω

equator

u ω    No preferred helicity, but + and – possible if result of instability

slide-8
SLIDE 8

8

Catastrophic quenching

2 f 2 1

, b b j B B J b j B J B J k k          

b j B J B J     

2 f 2 1 2 1 1

2 2 b B B k k dt d k     

 

) ( 2 1 2 2

s 2 1

1

t t k f

e k k

 

 

b B

molecular value!!

B J B A      2 dt d

2 f 2 1

, b b j B B J k k     

slide-9
SLIDE 9

9

Energy momentum tensor Conformal time, rescaled equations

Early Universe

slide-10
SLIDE 10

10

Kolmogorov turbulence

 forward cascade

nonlinearity  

2 1 2 1 2

2 cos cos   kx kx k k 2 

constant flux e cm2/s3 e e k E(k)  

2 2 1 u

dk k E

cm3/s2 

 

b a K

k C k E e 

1 2 3 : cm   a a 3 2 : s 

a=2/3, b= 5/3

slide-11
SLIDE 11

11

Magnetic helicity: inverse cascade

Initial slope E~k4

Christensson et al. (2001, PRE 64, 056405)

helical vs nonhelical

slide-12
SLIDE 12

12

Helical decay law: Biskamp & Müller (1999)

const   EL H L E L U / /

2 / 3 3

  e t E d / d   e

H E L E t E / / d / d

2 / 5 2 / 3

    e

3 / 2 

 t E

slide-13
SLIDE 13

13

Forced – decaying

Helical – nonhelical

slide-14
SLIDE 14

14

Self-similar turbulent decay

instantaneous scaling exponents

slide-15
SLIDE 15

15

  • Sect. 2.2

Assessement of the turbulent convective dynamo view

Collapsed spectra and pq diagrams

slide-16
SLIDE 16

16

Chiral magnetic effect: caused by chirality of fermions

Electrons have handedness But also spontaneous spin flip unless

2

c m T k

e B



6x109K electrons left-handed positrons: right-handed

slide-17
SLIDE 17

Chiral magnetic effect

In the presence of B-field chiral electrons produce a current J=…+mB with Leads to a dynamo effect

2

k k  m   

aem is the fine structure constant  quantum effect m is a pseudoscalar

slide-18
SLIDE 18

Total chirality conserved

Uncurled induction equation & chemical potential Coupling between electromagnetic field and chem potential Conservation equation Therefore

(spin flipping)

slide-19
SLIDE 19

Total system of equations

Momentum & continuity equations Together with:

slide-20
SLIDE 20

Characteristic velocities

Different orderings Two velocities from chiral magnetic effect

slide-21
SLIDE 21

Dimensional arguments

21

  • [E(k,t) ] = [r] cm3 s-2 = g s-2
  • E(k,t) = Cm r mab
  • cm: 3 = -a + 2b
  • s: -2 = -b
  •  b = 2, a = 2b - 3 = 4 - 3 = 1
  • E(k,t) = Cm rm2
  •  to determine Cm from simulations
slide-22
SLIDE 22

The spectrum from chiral effect

Governed solely by chiral chemical potential Spectrum build-up from high wavenumbers k EM(k,t) m/2 k-2

slide-23
SLIDE 23

Eventual saturation

23

  • [E(k,t) ] = g s-2
  • E(k,t) = Cl ramblc
  • g: 1 = a – c
  • cm: 0 = – b – c
  • s: – 2 = 2c
  •  c = – 1, b = – c = 1, a = 1+ c = 0
  • E(k,t) = Cl m/l
  •  to determine Cl from simulations
slide-24
SLIDE 24

The final spectrum

slide-25
SLIDE 25

Inverse cascade!

Growth at one wavenumber Then: saturation caused by initial chemical potential

slide-26
SLIDE 26

Early universe: use conservation law

Conseration equation Maximally helical:

slide-27
SLIDE 27

Inserting actual numbers

Magnetic helicity Inverse length scale =(0.2e-18G)2 Mpc G

slide-28
SLIDE 28

28

Science 328, 73 – 75 (2010)

  • Chiral magnetic effect alone may

be too weak to explain B-field

  • But the magnetic stress could still

explain gravitational waves

slide-29
SLIDE 29

29

Cosmological GWs

slide-30
SLIDE 30

30

Correspondence of spectra

  • If spectral slope of

B is -5/3, then

  • Spectral slope of

B2 is -5/3-2 = -11/3

  • But for slope 4, we

don’t get 4-2 = 2, but 0.

slide-31
SLIDE 31

31

Comparison with LISA sensitivity limits

  • Frequency ~3 mHz

– Slope corresponds to turbulence spectrum – magnetic energy 10%

  • r 1% or radiation
  • Observable w/ LISA

– arm length 2-5 milion km – Duration 2 or 5 yr

Större skallängt

1% 10%

slide-32
SLIDE 32

32

Quadratic scaling

  • Acoustic driving  strongest GW field
  • Quadratic scaling
slide-33
SLIDE 33

33

GWs from chiral magnetic effect

slide-34
SLIDE 34

34

GW energy & strain spectra

  • Magnetic helicity causes circular polarized GWs
  • Can reach 100%, and inverse cascade apparent
slide-35
SLIDE 35

35

Correspond to + and x modes

Seto (2006)

slide-36
SLIDE 36

36

Circular polarization in space & time

  • Both plus and cross polarization together
  • Combine the two as a function of space & time
  • Get circular polarization
slide-37
SLIDE 37

Conclusions

37

  • Magnetic helicity nearly perfectly conserved

– Catastrophic quenching in periodic boxes

  • Inverse cascade in decaying turbulence

– Important in early Universe

  • Can be initiated by chiral magnetic effect (CME)

– But may not yet explain lower observational limits

  • CME also drives gravitational waves

– Currently somewhat too weak

slide-38
SLIDE 38

Inverse cascading

Conseration equation