1 w.-t. ni 倪維斗 department of physics, national tsing hua university [email protected]...
TRANSCRIPT
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W.-T. Ni 倪維斗Department of Physics,
National Tsing Hua [email protected]
Foundations of Classical Electrodynamics
and Optical Experiments to Measure
the Parameters of the PPM (Parametrized Post-Maxewellian)
Electrodynamics 經典電動力學的基礎 (arXiv 1109.5501)
2011.12.12. NTHUFoundations of Classical Electrodynamics and PPM Framework
W-T Ni
Outline
Introduction – Maxwell equations and Lorentz force law Photon mass constraints Quantum corrections – quantum corrections Parametrized Post-Maxwell (PPM) electrodynamics Electromagnetic wave propagation Measuring the parameters of the PPM electrodynamics Electrodynamics in curved spacetime and EEP Empirical tests of electromagnetism and the χ-g framework Pseudoscalar-photon interaction and the cosmic pol.
rotation Discussion and outlook
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Introduction – Maxwell Equations and Lorentz Force
Law (I)馬克士威方程式與羅倫茲力
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(Jackson)
( 庫倫定律 )
( 法拉第定律 )
( 安培 - 馬克士威定律 )
( 無磁單極 )
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Charges (and currents) produce E and B fields influence the Motion of charges Maxwell Equations Lorentz Force Law
Introduction – Maxwell Equations and Lorentz Force
Law (II)馬克士威方程式與羅倫茲力
( 連續方程式 - 電荷守恆 )
( 羅倫茲力 )
電荷和電流產生電場和磁場;電場和磁場影響電荷的運動
Introduction – Maxwell Equations and Lorentz Force
Law (III)馬克士威方程式與羅倫茲力
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法拉第定律和無磁單極定律相當於電場和磁場可以由標量勢和向量勢 A 表示:
4-vector potential A (, A) Second-rank, antisymmetric field-strength tensor F = ∂A - ∂A
Electric field E [≡ (E1, E2, E3) ≡ (F01, F02, F03)] and magnetic induction B [≡ (B1, B2, B3) ≡ (F32, F13, F21)]
Electromagnetic field Lagrangian density LEM = (1/8π)[E2-B2].
Lagrangian density LEMS for a system of charged particles
in Gaussian units
LEMS=LEM+LEM-P+LP
=-(1/(16π))[(1/2)ηikηjl-(1/2)ηilηkj]FijFkl
-Akjk-ΣI mI[(dsI)/(dt)]δ(x-xI),
LEMS 整个電荷系統拉格朗日
LEM 電磁場拉格朗日 LEM-P 電磁場 - 粒子相互作用拉格朗日 LP 粒子拉格朗日
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Test of Coulomb’s Law 1/r2+
Cavendish 1772 || 0.02
Maxwell 1879|| 5 10-5
Plimpton and Lawton || 2 10-9
Williams, Faller, and Hill 1971
= (2.7 3.1)10-16
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12.1 in
1.5 m
4MHz 10kV p
Proca (1936-8) Lagrangian density and mass of photon
LProca = (mphoton2c2/8πħ2)(AkAk)
the Coulomb law is modified to have the electric potential A0 = q(e-μr/r)
where q is the charge of the source particle, r is the distance to the source particle, and μ (≡mphotonc/ħ) gives the inverse range of the interaction
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Constraints on the mass of photon
Williams, Faller & Hill (1971) Lab Test
mphoton ≤ 10-14 eV (= 2 × 10-47 g) μ-1 ≥ 2 × 107 m
Davis, Goldhaber & Nieto (1975) Pioneer 10 Jupitor flyby
mphoton ≤ 4 × 10-16 eV (= 7 × 10-49 g)
μ-1 ≥ 5 × 108 m
Ryutov (2007) Solar wind magnetic field
mphoton ≤ 10-18 eV (= 2 × 10-51 g) μ-1 ≥ 2 × 1011 m
Chibisov (1976) galactic sized fields
mphoton ≤ 2 × 10-27 eV (= 4 × 10-60 g) μ-1 ≥ 1020 m
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A good Reference: Goldhaber, A. S. & Nieto, M. M. (2010). Photon and Graviton Mass Limits. Review of Modern Physics, Vol.82, No.1, (January-March 2010), pp. 939-979
Quantum corrections to classical electrodynamics
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Heisenberg-Euler Lagrangian
Born-Infeld Electrodynamics
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Parametrized Post-Maxwell (PPM) Lagrangian density
(4 parameters: ξ, η1, η2, η3)
LPPM = (1/8π){(E2-B2)+ξΦ(E∙B)
+Bc-2[η1(E2-B2)2 +4η2(E∙B)2+2η3(E2-B2)(E∙B)]}
LPPM = (1/(32π)){-2FklFkl -ξΦF*klFkl
+Bc-2 [η1(FklFkl)2+η2(F*klFkl)2+η3(FklFkl)(F*ijFij)]}
(manifestly Lorentz invariant form) Dual electomagnetic field F*ij ≡ (1/2)eijkl Fkl
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Unified theory of nonlinear
electrodynamics and gravity
A. Torres-Gomez, K. Krasnov, & C. Scarinci PRD 83, 025023 (2011)
A class of unified theories of electromagnetism and gravity with Lagrangian of the BF type (F: Curvature of the connection 1-form A (), with a potential for the B () field (Lie-algebra valued 2-form), the gauge group is U(2) (complexified).
Given a choice of the potential function the theory is a deformation of (complex) general relativity and electromagnetism.
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Equations for nonlinear electrodynamics (1)
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Equations for nonlinear electrodynamics (2)
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Electromagnetic wave propagation
in PPM electrodynamics
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Birefringence or no Birefringnce
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Measuring the parameters of the PPM electrodynamics Δn = n║ - n┴ = 4.0 x 10-24 (Bext/1T)2
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Let’s choose z-axis to be in the propagation direction, x-axis in the Eext direction and y-axis in the Bext direction, i.e., k = (0, 0, k), Eext = (E, 0, 0) and Bext = (0, B, 0).
n± = 1 + (η1+η2)(E2+B2-EB)Bc-2± [(η1-η2)2(E2+B2-EB)2+η3
2(E2-B2)]1/2 Bc-2.
(i) E=B as in the strong microwave cavity, the indices of refraction for light is n± = 1 + (η1+η2)B2Bc
-2±(η1-η2)B2Bc-2,
with birefringence Δn given by Δn = 2(η1-η2)B2Bc
-2; (ii) E=0, B≠0, the indices of refraction for light is n± = 1 + (η1+η2)B2Bc
-2±[(η1-η2)2+η32]1/2B2Bc
-2,
Δn = 2[(η1-η2)2+η32]1/2B2Bc
-2.
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Measuring the parameters of the PPM electrodynamics
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Measuring the parameters of the PPM electrodynamics
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Lab Experiment:Principle of Experiment
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Apparatus and Finesse Measurement
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Suspension and Analyzer’s Extinction
ratio
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Injection Optical Bench
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Vacuum Chamber and Magnet
目前出光狀態與 Finesse( 將耗散 / 投影損失視為反射率較差的表現 )
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Current Optical Experiments
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Foundations of Classical Electrodynamics and PPM Framework W-T Ni 30
LNLFerrara
PVLAS
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Rotation and ellipticity sensitivity comparisons using ellipsometers
with optical path multipliers
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PVLAS Ferrara on 3 competing experiments
(I) Q & A in Taiwan: They have the mirrors of the FP installed in two
distant vacuum chambers suspended with attenators of ambient vibrations of the type developed for interferometric gravitational wave detectors. The separation of the two optical halves seems to limit the sensitivity of their apparatus. The finesse is below 10^5
OSQAR at CERN: uses a LHC dipole magnet 15 m long that can reach a 9 T field. The ellipsometer will exploit a FP to maximize the number of reflections and a novel optical techique to modulate the MBV effect. Since it is not feasible to set the LHC magnet in rotation and a modulation of the LHC magnet field intensity could be achieved only at very low frequency, the experiment foresees to modulate the polarization of the light entering the ellipsometer by setting in rotation the polarization plane.
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PVLAS Ferrara on 3 competing experiments
(II) According to our experience in this set-up the
rotation of the polarization will generate a very large signal due to the intrinsic birefringence of the FP mirrors.
BMV in Toulouse: homodyne, high intensity magnetic field, employing pulsed magnets (few ms), 40 cm long, that have already reached peak intensities in excess of B = 15 T, L = 0.5 m total length, 5 shots/hour. Finesse 10^5, 10^(-7) per square root Hertz ellipticity sensitivity. For ten times improvement in sensitivity, it takes 650 years of continuous datataking.
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Comparisons on the N2 magnetic birefringence
measurement
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PVLAS 2004Q&A 2009BMV2011
(Pseudo)scalar field: WEP & EEP in EM field
Foundations of Classical Electrodynamics and PPM Framework W-T Ni 362011.12.12. NTHU
(Pseudo)scalar-Photon Interaction
Modified Maxwell Equations Polarization Rotation in EM Propagaton
(Classical effect)Constraints from CMB polarization observation This talk
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Galileo’s experiment on inclined plane (Contemporary painting of Giuseppe Bezzuoli)
Galileo Equivalence Principle: Universality of free-fall trajectories
GP-B and Rotational EP
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Einstein Equivalence Principle
EEP:(Einstein Elevator)
Local physics is that of Special relativity
Study the relationship of Galileo
Equivalence Principle and EEP in a
Relativistic Framework: framework g
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Electromagnetism :Charged particles and
photons
)()()16
1( 2/1
II
IIk
kklijijkl
I xxdt
dsmgjAFFL
]21
21
[)( 2/1 ijklkjiljlikijkl ggggg ψ
Special Relativity
g framework
Galileo EP constrains to :
)()()16
1( 2/1
II
IIk
kklijjlikjl
I xxdt
dsmgjAFFL
ηη
(Pseudo)scalar-Photon Interaction
Various terms in the Lagrangian
(W-T Ni, Reports on Progress in Physics, next month /also in arXiv)
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Empirical Constraints: No Birefringence
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Empirical Constraints from Unpolarized EP Experiment: constraint on Dilaton for
EM: φ = 1 ± 10^(-10)
Cho and Kim, Hierarchy Problem, Dilatonic Fifth, and Origin of Mass, ArXiv0708.2590v1
(4+3)-dim unification with G=SU(2), L<44 μm (Kapner et al., PRL 2007) L<10 μm (Li, Ni, and Pulido Paton,
ArXiv0708.2590v1 Lamb shift in Hydrogen and Muonium gr-
qc
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Emprirical constraints: H g (One Metric)
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Constraint on axion: φ < 0.1Solar-system 1973 (φ < 10^10)
Metric Theories of Gravity General Relativity Einstein Equivalence
Principle recovered For a recent exposition, see Hehl & Obukhov ArXiv:0705.3422v1
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Change of Polarization due to Cosmic Propagation
The effect of φ is to change the phase of two different circular polarizations of electromagnetic-wave propagation in gravitation field and gives polarization rotation for linearly polarized light.[6-8]
Polarization observations of radio galaxies put a limit of Δφ ≤ 1 over cosmological distance.[9-14]
Further observations to test and measure Δφ to 10-6 is promising.
The natural coupling strength φ is of order 1. However, the isotropy of our observable universe to 10-5 may leads to a change (ξ)Δφ of φ over cosmological distance scale 10-5 smaller. Hence, observations to test and measure Δφ to 10-6 are needed.
The angle between the direction of linear polarization in the UV and the direction of the UV axis for RG at z > 2. The angle predicted by the scattering model is 90^o
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The advantage of the test using the optical/UV polarization over that using the radio one is that it is based on a physical prediction of the orientation of the polarization due to scattering, which is lacking in the radio case,
and that it does not require a correction for the Faraday rotation, which is considerable in the radio but negligible in the optical/UV.
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Constraints on cosmic polarization rotation from CMB polarization
observations[See Ni, RPP 73, 056901 (2010) for detailed references]
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CMB Polarization Observation
In 2002, DASI microwave interferometer observed the polarization of the cosmic background.
With the pseudoscalar-photon interaction , the polarization anisotropy is shifted relative to the temperature anisotropy.
In 2003, WMAP found that the polarization and temperature are correlated to 10σ. This gives a constraint of 10-1 rad or 6 degrees of the cosmic polarization rotation angle Δφ.
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CMB Polarization Observation
In 2005, the DASI results were extended (Leitch et al.) and observed by CBI (Readhead et al.) and CAPMAP (Barkats et al.)
In 2006, BOOMERANG CMB Polarization DASI, CBI, and BOOMERANG detections of
Temperature-polarization cross correllation QuaD Planck Surveyor was launched last year with
better polarization-temperature measurement sensitivity. Sensitivity to cosmic polarization rotation Δφ of 10-2-10-3 expected.
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References
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Space contribution to the local polarization rotation angle -- [μΣ13φ,μΔxμ] = |▽φ| cos θ Δx0. The time contribution is φ,0 Δx0. The total contribution is (|▽φ| cos θ + φ,0) Δx0. (Δx0 > 0)
Intergrated:φ(2) - φ(1)φ(2) - φ(1)
1: a point at the 1: a point at the decoupling epochdecoupling epoch
2: observation 2: observation pointpoint
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Variations and Fluctuations
Rotation φ(2) - φ(1)Rotation φ(2) - φ(1) δδφ(2) - φ(2) - δδφ(1): φ(1): δδφ(2) variations and φ(2) variations and
fluctuations at the last scattering fluctuations at the last scattering surface of the decoupling epoch; surface of the decoupling epoch; δδφ(1), φ(1), at present observation point, fixedat present observation point, fixed
<[<[δδφ(2) - φ(2) - δδφ(1)]^2> variance of φ(1)]^2> variance of fluctuation ~ [couplingfluctuation ~ [couplingξ × 10^(-5)]^2 × 10^(-5)]^2
The coupling depends on various The coupling depends on various cosmological modelscosmological models
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COSMOLOGICAL MODELS
PSEUDO-SCALAR COSMOLOGY, e.g., Brans-Dicke theory with pseudoscalar-photon coupling
NEUTRINO NUMBER ASYMMETRY BARYON ASYMMETRY SOME other kind of CURRENT LORENTZ INVARIANCE VIOLATION CPT VIOLATION DARK ENERGY (PSEUDO)SCALAR
COUPLING OTHER MODELS
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Constraints on cosmic polarization rotation from
CMB
All consistent with null detection and with one another at 2 σ level
Newest : Brown et al. 11.2±8.7 ±8.7 mrad QuaD 2009
Outlook
Precision tests of Classical Electrodynamics will continue to serve physics community in frontier research, in the quantum regime, in gravitation and in cosmology
Thank you for your attention
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