early universe
play

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


  1. 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 Brandenburg (Nordita, Stockholm) 1

  2. elix Curling tendril  Climbing plant Biophysics: Helix Chirality 2

  3. Helicity & topology: math. underpinnings Helical structures on the Sun (X-ray emission) Coronal mass ejections 3

  4. Helical structures on the Sun (X-ray emission) Coronal mass ejections 4

  5. Moffatt coined the term in hydro/MHD Coronal mass ejections 5

  6. Magnetic helicity measures linkage of flux     1 A B H d V S 1 V  2    B A       H A d B d S 1     H 2 L S 1 1 1 2     Therefore the unit is      A d S 1 2 Maxwell squared S 2 6

  7. What produces helicity? north equator south Cyclones: Down: faster No preferred helicity, Up: slower but + and – possible    ω u if result of instability W W g g  u   u  ω ω 0 0

  8. Catastrophic quenching d      A B 2 J B dt      J B J B j b      2 2 J B k B , j b k b 1 f      J B J B j b      2 2 J B k B , j b k b d 1 f       1 2 2 2 k B 2 k B 2 k b 1 1 f dt molecular value!!   k      2 f 2 2 2 k ( t t ) B b 1 e 1 s k 1 8

  9. Early Universe Energy momentum tensor Conformal time, rescaled equations 9

  10. Kolmogorov turbulence  forward cascade nonlinearity     2 1 1 cos kx cos 2 kx 2 2  k 2 k constant flux e  cm 2 /s 3     cm 3 /s 2  1 u  2 E k dk E ( k ) 2     e a b E k C k K a =2/3, b =  5/3  a  e e cm : 3 2 1  s : 2 3 a k 10

  11. Magnetic helicity: inverse cascade helical vs Initial slope nonhelical E ~ k 4 Christensson et al. (2001, PRE 64, 056405) 11

  12. Helical decay law: Biskamp & Müller (1999)  EL  H const e   3 3 / 2 U / L E / L e   d E d / t e     3 / 2 5 / 2 d E / d t E / L E / H   t 2 / 3 E 12

  13. Forced – decaying Helical – nonhelical 13

  14. Self-similar turbulent decay instantaneous scaling exponents 14

  15. Collapsed spectra and pq diagrams Sect. 2.2 Assessement of the turbulent convective dynamo view 15

  16. Chiral magnetic effect: caused by chirality of fermions electrons left-handed positrons: right-handed But also spontaneous Electrons have handedness spin flip unless  2 k T m c B e 6x10 9 K 16

  17. Chiral magnetic effect In the presence of B -field chiral electrons produce a current J=…+ m B with a em is the fine Leads to a dynamo effect structure constant  quantum effect m is a pseudoscalar   m   2 k k

  18. Total chirality conserved Uncurled induction equation & chemical potential (spin flipping) Coupling between electromagnetic field and chem potential Conservation equation Therefore

  19. Total system of equations Momentum & continuity equations Together with:

  20. Characteristic velocities Two velocities from chiral magnetic effect Different orderings

  21. Dimensional arguments • [ E ( k , t ) ] = [ r ] cm 3 s -2 = g s -2 • E ( k , t ) = C m r m a  b • cm: 3 = -a + 2 b • s : - 2 = -b •  b = 2, a = 2 b - 3 = 4 - 3 = 1 • E ( k , t ) = C m rm 2 •  to determine C m from simulations 21

  22. The spectrum from chiral effect Spectrum build-up from high wavenumbers E M (k,t) k -2 k m/2 Governed solely by chiral chemical potential

  23. Eventual saturation • [ E ( k , t ) ] = g s -2 • E ( k , t ) = C l r a m b l c • g: 1 = a – c • cm: 0 = – b – c • s : – 2 = 2 c •  c = – 1, b = – c = 1, a = 1 + c = 0 • E ( k , t ) = C l m/l •  to determine C l from simulations 23

  24. The final spectrum

  25. Inverse cascade! Growth at one wavenumber Then: saturation caused by initial chemical potential

  26. Early universe: use conservation law Conseration equation Maximally helical:

  27. Inserting actual numbers =(0.2e-18G) 2 Mpc G Magnetic helicity Inverse length scale

  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 28

  29. Cosmological GWs 29

  30. Correspondence of spectra • If spectral slope of B is -5/3, then • Spectral slope of B 2 is -5/3-2 = -11/3 • But for slope 4, we don’t get 4 -2 = 2, but 0. 30

  31. Comparison with LISA sensitivity limits • Frequency ~3 mHz 10% – Slope corresponds to 1% turbulence spectrum – magnetic energy 10% Större skallängt or 1% or radiation • Observable w/ LISA – arm length 2-5 milion km – Duration 2 or 5 yr 31

  32. Quadratic scaling • Acoustic driving  strongest GW field • Quadratic scaling 32

  33. GWs from chiral magnetic effect 33

  34. GW energy & strain spectra • Magnetic helicity causes circular polarized GWs • Can reach 100%, and inverse cascade apparent 34

  35. Correspond to + and x modes Seto (2006) 35

  36. Circular polarization in space & time • Both plus and cross polarization together • Combine the two as a function of space & time • Get circular polarization 36

  37. Conclusions • 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 37

  38. Inverse cascading Conseration equation

Recommend


More recommend