Coherence with applications to Axions.

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Coherence with applications to Axions. Axion Academic Training CERN, 30 November 2005 Coherence with applications to Axions. Yannis K. Semertzidis Brookhaven National Lab Definition Coherence in lasers Axion photon coherence/oscillations Applications Yannis Semertzidis, BNL. ICHEP02, 31 July 2002

Yannis Semertzidis, BNL Coherence The quality or state of cohering, especially a logical, orderly, and aesthetically consistent relationship of parts! The property of being coherent, as of waves! The distance over which interference will occur. The coherence length of an optical source is affected by the size of the source, spatial coherence, the phase purity of the source, temporal coherence, and the spectral bandwidth of the light. Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Temporal/Spatial Coherence A characteristic of laser output, calculated by dividing the speed of light by the linewidth of the laser beam. The temporal coherence length of different lasers thus varies from a few centimeters to many meters and longer. The maintenance of a fixed-phase relationship across the full diameter of a cross section of a laser beam. Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Yannis Semertzidis, BNL Degree of coherence For lightwaves, the magnitude of the degree of coherence is equal to the visibility, V , of the fringes of a two-beam interference test, as given by where I max is the intensity at a maximum of the interference pattern, and I min is the intensity at a minimum. Light is considered to be highly coherent when the degree of coherence exceeds 0.9, partially coherent for values less than 0.9 but more than nearly zero values, and incoherent for nearly zero values. Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Axion/photon oscillations in a magnetic field B with length L Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Axion to photon conversion probability With q=ma2/2, is the momentum transfer and ma,  the axion mass and energy respectively. The coherence length is defined by Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Yannis Semertzidis, BNL Question: How is the momentum transfer q balanced? By the magnetic field, over the De Broglie length All the participating virtual photons along this wavelength take part in the process coherently, hence the L2 effect, similar to the coherent Compton scattering… Also the effect is proportional to the energy density in the magnet, hence the B2 dependence… Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Axion-photon conversion in gas For wave-numbers k and ka, we have coherence when (attention, different units!) Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Hence, (after some algebra) for coherence requirements we get Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Yannis Semertzidis, BNL Example with 4He gas Generalized for any ma Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

How about spatial coherence? axions  r x-rays n’ n i x-ray refraction: The x-rays/axions do not overlap The x-rays travel longer paths than axions The coherence is lost… The important parameter here is pressure uniformity in cross section… Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Yannis Semertzidis, BNL A numerical example For a 10m long magnet and axion/photon missing each other by 1 wavelength Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Two important consequences Pressure (temperature) uniformity requirements are strict with gas buffer. Can use a laser light to probe the uniformity, e.g. 5mK temperature gradient in the cross section, along the whole length of the magnet can produce up to 4mm shift on a red laser light…(effect goes as (1/2)2= 20002). Assuming multiple refractions axion to photon conversion in stars (e.g. sun) does not suffer completely from short coherent lengths but lengths could add linearly over long distances… Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Yannis Semertzidis, BNL Consider the picture: Axions produce the photon field in phase, up to coherence length Beyond that length axions lag behind by  due to their mass. When the phase of the “new” photon field is 180º out of phase it adds destructively and the total photon field is zero! …what happened to the energy conservation? Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Actually photons and axions mix… A transverse magnetic field is necessary The mixing angle is G. Raffelt and L. Stodolsky PRD 37 (1988) 1237. The oscillation length L is Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

For axion and photon planewaves Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Yannis Semertzidis, BNL For solar axions Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Yannis Semertzidis, BNL For axion Production in a magnetic field with a laser light (e.g. PVLAS or E840 @BNL) Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL

Yannis Semertzidis, BNL Summary Coherence is a delicate matter and special attention needs to be taken Axion/photon coherent oscillations happen in magnetic fields as long as they travel together in time and in space Axion Academic Training, 30 November, 2005 Yannis Semertzidis, BNL