Why the interpretation of"Measuring propagation speed of Coulomb fields"stands

The experimental findings reported in our original paper [1] (arXiv:1211.2913) have been criticized in ref.[2] (arXiv:1606.00710). We believe that the arguments brought in ref. [2] are not correct and we show evidence for this.


Introduction
In ref. [2], our measurements [1] have been criticized: the authors imply that the responses of our sensors are not caused by the Coulomb field carried by the electron beams, but are rather due to electromagnetic radiation, generated in the last magnetic bend the electron beam undergoes entering the experimental hall. The detail of their main points are: 1. Inconsistencies in our longitudinal timing measurements.
2. Sloping level of background vs.transverse distance for the beam dump measurements.
3. Sensor signals due to synchrotron radiation in the last bend of the beam line.
In the following we will address the stated points separately.

Longitudinal time measurements
It is clearly stated in our paper [1] ( fig. 13) that no timing dependence on the transverse position of our sensors was measured, and that the correlation timing-longitudinal position was the one pertaining to an electron beam moving with γ ≈ 1000 in the experimental hall. Out of the six measurements reported in table 1 of ref. [1], there is just one, −2.8σ away from the above mentioned hypothesis, and is the one that has been speculated upon in ref. [2]. The authors point out that the measurement might infringe the speed of light barrier. To put things into perspective the 2.8 σ discrepancy corresponds to less than 150 psec in time or less than 4 cm in space.
We stress that, considering the entire set of data reported in the aforementioned table, one readily sees that timing for sensor A5 tend to be early while timing for sensor A6 tend to be late. Averaging the timing for A5 and A6, in fact, wipes out completely the fluctuation, and strongly suggests that there be a systematic effect due to a less than perfect flatness of the experimental hall floor. A 35 mrad angle would grant the effect seen in table 1 of ref. [1].
We summarize the time distance correlations in Table 1, where the sensors' A5,A6 average time obtained at the three different longitudinal positions are shown. 3 Sloping background in the beam-dump measurements.
No quantitative statement was made in [2] for this effect. In order to have a quantitative understanding of the data, we fit the four point reported in fig 15 of ref [1] either with a constant or with a first order polinomial. A comparison between the χ 2 DOF for the two hypotheses might give an insight, in relative terms, as to which one is more suited to represent the data. While it is clear that neither hypothesis fits the data very well, the zeroth order polynomial shows a better agreement to the experimental points; it is worth noticing that the linear function's fitted slope is really ill determined with a relative error close to 80%.

Synchrotron radiation out of the last bend
Here too we do not have any quantitative statement in ref. [2], so we evaluate here the electromagnetic power released in the last bend and compared it with the power of our sensors' signal.
The beam line into the experimental hall has a 45 degrees bend at 1.72 m curvature radius: this translates into a synchrotron radiation (total) power of ≈ 510 × 10 −3 W for a typical pulse of 10 8 electrons at 500 MeV. The critical frequency for the bend is ωc ≈ 3 × 10 17 Hz.
We did evaluate the synchrotron radiation power hitting our sensor either with no angular cut or by means of a full Monte Carlo simulation [3] taking into account the angular distribution of the emitted radiation at the position of the most exposed detector (radial detector(s) at 5 cm transverse distance and 92 cm. longitudinal distance) As clearly stated in ref. [1], our sensors have a cut-off frequency of ≈ 250 MHz.
The results are summarized in table 3. The amount of power synchrotron radiation conveys onto our sensors is at least ≈ 50000 times smaller than the one pertaining to our measured pulse amplitude.