The Spacetime Metric

Historical research guide · 0874 · 2016

The PVLAS experiment: measuring vacuum magnetic birefringence and dichroism with a birefringent Fabry–Perot cavity

Federico Della Valle · Aldo Ejlli · Ugo Gastaldi · Giuseppe Messineo · Edoardo Milotti · Ruggero Pengo · Giuseppe Ruoso · Guido Zavattini

In one minute

Quantum electrodynamics says that a strong magnet turns empty space into something like a crystal: light polarised along the field should travel very slightly slower than light polarised across it. At 2.5 tesla the predicted difference is about 2.5 parts in a hundred thousand million million million, and nobody has yet resolved it directly. Federico Della Valle, Guido Zavattini, Giuseppe Ruoso and their colleagues in Ferrara describe the instrument that came closest — a laser bouncing hundreds of thousands of times between two mirrors, through the bores of two rotating permanent magnets. Their central point here is a practical one that touches every experiment of this kind: the mirrors themselves are slightly birefringent, so the two polarisations resonate at slightly different frequencies, the signal is attenuated by a known factor, and birefringence and dichroism leak into each other. Turn that leak around and it becomes useful — one measurement now yields both quantities, and it gives new laboratory limits on light particles that couple to two photons.

Connection

Chapter 2 says the vacuum is a real, structured medium, and vacuum magnetic birefringence is its cleanest optical signature: put a magnet in empty space and light itself changes speed depending on how it is polarised. This is the paper where the Ferrara group states exactly how well that can be measured and what stands in the way. Chapter 1 gets a model case of the evidence ladder — a published noise budget, a calibration against a gas whose birefringence is known, a specific list of what is being changed next, and limits that hold no matter which theory of light particles you prefer. The collaboration’s twenty-five-year account of the whole programme is on the site at /library/stm-08601764f6.

From the source

  1. The Euler-Heisenberg-Weisskopf Lagrangian makes electrodynamics non-linear even in vacuum. To lowest order the magnetic birefringence is three times the parameter A-sub-e times the square of the external field, and with that parameter equal to 1.32 times ten to the minus twenty-four per tesla squared this gives a birefringence of 2.5 times ten to the minus twenty-three at 2.5 tesla, with the accompanying magnetic dichroism negligible.Sect. 1, Eqs. (1) to (4)

  2. The method is heterodyne polarimetry inside a very long optical path. Over a magnetic field length of 1.64 metres at 2.5 tesla with 1064 nanometre light, the QED ellipticity would be 1.2 times ten to the minus sixteen; a Fabry-Perot cavity of finesse near seven hundred thousand multiplies the optical path by 445,000 and lifts that ellipticity to the order of ten to the minus ten.Sect. 2, Eq. (7); Sect. 2.1, Eqs. (13) to (15); Sect. 3

  3. The paper’s central methodological result is that the dielectric mirrors are themselves birefringent in reflection, which has three consequences for every polarimeter of this type: the two polarisation resonances of the cavity are separated in frequency, the extinguished beam is attenuated by a calculable factor, and ellipticity and rotation mix into one another. The ratio of the spurious rotation to the true ellipticity is minus half the amplification factor times the mirror phase difference, so the mixing itself measures the sum of the two mirrors’ birefringences.Sect. 2.2, Eqs. (18) to (23); Sect. 3.2, Eqs. (24) and (25)

  4. The vacuum results, weighted averages over four determinations each, are a magnetic birefringence of minus 1.5 plus or minus 3.0 times ten to the minus twenty-two and a magnetic dichroism of minus 1.6 plus or minus 3.5 times ten to the minus twenty-two, both at 2.5 tesla. All the numbers are compatible with zero, and the birefringence result is an order of magnitude larger than the QED prediction, so it serves as an upper limit.Sect. 4, Eqs. (26) and (27); Tables 2 and 3

  5. The same measurements exclude new regions in the parameter space of axion-like and milli-charged particles, model-independently: the ellipticity result dominates above one milli-electron-volt of axion-like-particle mass, and the fermion milli-charged-particle plot applies to all types of neutrinos, limiting their charge to less than about three times ten to the minus eight of the electron charge for masses below ten milli-electron-volts.Sect. 4.2; Figs. 14 and 15

  6. The sensitivity, four times better than the 2014 apparatus, is still far from the six times ten to the minus nine per root hertz computed from the known noise sources. The noise comes from the cavity, seismic modulation of the mirror birefringence was excluded by shaking the bench at a known amplitude in all three directions, thermal instability shows up only below about one hertz, and the noise is largely independent of the attenuation factor — which points at diffused light. The named next steps are faster magnet rotation, less scattered light, better mirrors, and cooling the mirrors toward liquid nitrogen temperature.Sect. 4.1; Sect. 5, Conclusions

The way in

https://doi.org/10.1140/epjc/s10052-015-3869-8

How to cite it

Federico Della Valle, Aldo Ejlli, Ugo Gastaldi, Giuseppe Messineo, Edoardo Milotti, Ruggero Pengo, Giuseppe Ruoso, Guido Zavattini (2016) The PVLAS experiment: measuring vacuum magnetic birefringence and dichroism with a birefringent Fabry–Perot cavity doi:10.1140/epjc/s10052-015-3869-8

Where it sits in the curriculum

Provenance: Retrieved 2026-09-08

Summary by: The Spacetime Metric editorial rail (AI draft from the source text, 2026-09-07)

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