The Fischbach & Jenkins result has been talked about a bit in nuclear physics circles, so I'm reasonably well qualified to comment on it. First, a couple of general comments:
There are a large number of experiments (looking for dark matter, extrasolar planets, other exotica, etc.) which involve looking for a
seasonal change in some detector. The detector has more counts in summer than winter, or higher-energy counts in spring than in fall, or the distant star's redshift seems to vary on a 7-day timescale, or whatever. The main lesson of 30 years' experience with these experiments is
it's maddeningly difficult. One very rarely understands
all of the environmental effects on one's detector---does it care a little about humidity? That varies seasonally, but of course one can try to measure or control for it. Does it care about the quality of your mains power? That varies seasonally (In some places, there's a seasonal switch from hydro to coal, with detectable effects on the power.) Does it care who's babysitting the experiment? (The personnel change seasonally---undergrads in the summer, for example.) How about the experiment two doors down the hall with the stray magnetic field? How about the jackhammers which are outside all summer? Etc.
It's similarly difficult to find day-night effects and 7-day effects. The former encounter all sorts of systematics (temperature, power, humans, etc.) and the latter encounter
weekends. This is seriously a big deal: take any raw data from any (say) neutrino experiment, do a Fourier transform on it, and you'll see a big peak at 24 hours and 7 days. There are more people poking at the experiment 9-5 weekdays, and fewer at other times, and this always sneaks into the detector performance somehow. (Day-night differences are actually very interesting in neutrino experiments, but you can see that the good data on these topics is supported by a maddening level of calibration. You almost have to treat it like two detectors, the "day detector" and the "night detector", which you subject to totally separate calibrations.)
Fischbach and Jenkins report correlations for 32Si (a low-energy beta emitter) and 226Ra (a fairly typical alpha emitter). Rick Norman at LBL looked back at several long datasets of
(see here) including 22Na, 44Ti, 108Ag, 121Sn, 133Ba, and 241Am, and saw nothing. Peter Cooper at Fermilab looked at the Pioneer Pu244 source and saw no sun-dependent variation whatsoever.
http://arxiv.org/abs/0809.4248---certainly not the particular one proposed by Fischbach.
It's also worth noting that Fischbach has published something sort of like this before. his 1986 paper
Reanalysis of the Eotvos experiment was *also* a re-analysis of someone elses' data, and *also* claimed to see evidence for a new fundamental force in the details of the data. (This prompted lots of reanalysis at the time; modern experiments fairly quickly ruled out the effect Fischbach reported.)
Finally, let me just comment on the actual data Fischbach is looking at. This data is reported in
Astroparticle Physics (and the preprint version
here. I think the content is the same, but I notice that the preprint has bitmapped figures. If you're interested in the details and have access to the Astropart. Phys., it is worth zooming in on the higher-quality graphs.)
First, some of the data is shown, not as raw data, but as a 5 point moving average. Moving averages introduce "fake" correlations when there are none in the raw data, see
http://bactra.org/weblog/666.html for discussion. So ignore Figs. 1 and 4. (The actual analysis is done on raw data---I think---so this seems to be just a display/presentation issue.)
Where they do show raw data, it reveals the problem. The raw data
has systematic errors in it. You don't have to take my word for it---you can see it. The count rate is drifting all over the place, both high and low---for example, look at the end of the trace in Fig. 2. (In addition, of course, it usually drifts in the directions suggested by Fischbach's hypothesis; the waves which are obvious to the eye are the same ones that pop out in his statistics.) Why is it able to drift so far? Remember that the claim, or the assumption, is that this is a detector which is
only detecting this radionuclide and which is immune to minor environmental effects. Well, sorry, no it's not. The hump at the end, and the variation in the size of the peaks, are all perfectly clear evidence that this detector's count rate depends on
something other than radioactivity and the Sun-Earth distance.
So the author wants to say "This detector is picking up the exponential decay of the nuclide, and also a season-dependent term"; he infers that the season dependent term is evidence for new particle physics. But that's not what the data show. The data show the detector picking up at least three things: 1) the exponential, AND 2) a season-dependent term, AND 3)
some other unexplained medium-to-long-term drifts. But this doesn't suggest new physics at all; if there are medium-to-long-term unexplained detector drifts, you have no reason to believe that one of those drifts isn't a seasonal one. In spite of perfectly clear evidence that their detector has systematic drifts, Fischbach allows himself to
assume that this particular annual effect is not such a drift. This assumption is unjustified.
Likewise in Fig. 3---this data shows that there's
something other than just statistics+seasons altering these count rates; that's simply not what statistical-error-dominated data looks like.