Of Particular Significance

So What Is It? That’s the question one hears in all the bars and on all the street corners and on every Twitter feed and in the whispering of the wind. Everybody wants to know. That bump seen on the ATLAS and CMS two-photon plots! What… IS… it…?

ATLAS_CMS_diphoton_2015
The two-photon results from ATLAS (top) and CMS (bottom) aligned, so that the 600, 700 and 800 GeV locations (blue vertical lines) line up almost perfectly. The peaks in the two data sets are in about the same location. ATLAS’s is larger and also wider. Click here for more commentary.

Well, to be honest, probably it’s just that: a bump on a plot. But just in case it’s not — just in case it really is the sign of a new particle in Large Hadron Collider [LHC] data — let me (start to) address the question.

First: what it isn’t. It can’t just be a second Higgs particle (a heavier version of the one found in 2012) that is just appended to the known particles, with no other particles added in.   (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON December 18, 2015

Was yesterday the day when a crack appeared in the Standard Model that will lead to its demise?  Maybe. It was a very interesting day, that’s for sure. [Here’s yesterday’s article on the results as they appeared.]

I find the following plot useful… it shows the results on photon pairs from ATLAS and CMS superposed for comparison.  [I take only the central events from CMS because the events that have a photon in the endcap don’t show much (there are excesses and deficits in the interesting region) and because it makes the plot too cluttered; suffice it to say that the endcap photons show nothing unusual.]  The challenge is that ATLAS uses a linear horizontal axis while CMS uses a logarithmic one, but in the interesting region of 600-800 GeV you can more or less line them up.  Notice that CMS’s bins are narrower than ATLAS’s by a factor of 2.

ATLAS_CMS_diphoton_2015
The diphoton results from ATLAS (top) and CMS (bottom) arranged so that the 600, 700 and 800 GeV locations (blue vertical lines) line up almost perfectly. (The plots do not line up away from this region!)  The data are the black dots (ignore the bottom section of CMS’s plot for now.) Notice that the obvious bumps in the two data sets appear in more or less the same place. The bump in ATLAS’s data is both higher (more statistically significant) and significantly wider.

Both plots definitely show a bump.  The two experiments have rather similar amounts of data, so we might have hoped for something more similar in the bumps, but the number of events in each bump is small and statistical flukes can play all sorts of tricks.

Of course your eye can play tricks too. A bump of a low significance with a small number of events looks much more impressive on a logarithmic plot than a bump of equal significance with a larger number of events — so beware that bias, which makes the curves to the left of the bump appear smoother and more featureless than they actually are.  [For instance, in the lower register of CMS’s plot, notice the bump around 350.]

We’re in that interesting moment when all we can say is that there might be something real and new in this data, and we have to take it very seriously.  We also have to take the statistical analyses of these bumps seriously, and they’re not as promising as these bumps look by eye.  If I hadn’t seen the statistical significances that ATLAS and CMS quoted, I’d have been more optimistic.

Also disappointing is that ATLAS’s new search is not very different from their Run 1 search of the same type, and only uses 3.2 inverse femtobarns of data, less than the 3.5 that they can use in a few other cases… and CMS uses 2.6 inverse femtobarns.  So this makes ATLAS less sensitive and CMS more sensitive than I was originally estimating… and makes it even less clear why ATLAS would be more sensitive in Run 2 to this signal than they were in Run 1, given the small amount of Run 2 data.  [One can check that if the events really have 750 GeV of energy and come from gluon collisions, the sensitivity of the Run 1 and Run 2 searches are comparable, so one should consider combining them, which would reduce the significance of the ATLAS excess. Not to combine them is to “cherry pick”.]

By the way, we heard that the excess events do not look very different from the events seen on either side of the bump; they don’t, for instance, have much higher total energy.  That means that a higher-energy process, one that produces a new particle at 750 GeV indirectly, can’t be a cause of big jump in the 13 TeV production rate relative to 8 TeV.  So one can’t hide behind this possible explanation for why a putative signal is seen brightly in Run 2 and was barely seen, if at all, in Run 1.

Of course the number of events is small and so these oddities could just be due to statistical flukes doing funny things with a real signal.  The question is whether it could just be statistical flukes doing funny things with the known background, which also has a small number of events.

And we should also, in tempering our enthusiasm, remember this plot: the diboson excess that so many were excited about this summer.  Bumps often appear, and they usually go away.  R.I.P.

ATLAS_dibosonXS
The most dramatic of the excesses in the production of two W or Z bosons from Run 1 data, as seen in ATLAS work published earlier this year. That bump excited a lot of people. But it doesn’t appear to be supported by Run 2 data. A cautionary tale.

Nevertheless, there’s nothing about this diphoton excess which makes it obvious that one should be pessimistic about it.  It’s inconclusive: depending on the statistical questions you ask (whether you combine ATLAS and CMS Run 2, whether you try to combine ATLAS Run 1 and Run 2, whether you worry about whether the resonance is wide or narrow), you can draw positive or agnostic conclusions.  It’s hard to draw entirely negative conclusions… and that’s a reason for optimism.

Six months or so from now — or less, if we can use this excess as a clue to find something more convincing within the existing data — we’ll likely say “R.I.P.” again.  Will we bury this little excess, or the Standard Model itself?

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON December 16, 2015

CMS results are being presented by Jim Olsen of Princeton University.

CMS has magnet problems this year due to cooling system problems but was able to record 3/4 of the data with the magnet on.

The diboson excess widely discussed this summer is, perhaps not surprisingly, not confirmed.  Same for the old dilepton excesses.

With certain assumptions, limits on gluinos jump from 1.3 TeV – 1.4 TeV to 1.6-1.7 TeV.

Big improvement in limits on “Black Holes” or anything else dramatic at very high energy (as we saw also in my post yesterday about ATLAS multijet events.)

Top-primes — limits jump to about 950 GeV relative to 800, again with assumptions.

Some new limits on invisible particles.  W’ resonances ruled out up to 4.2 TeV if they decay to leptons, to 2.4 TeV if they decay to top quark + bottom antiquark (with assumptions.)  No dijet bumps or other unusual dijet behavior.  No dilepton bumps up to 2.5 – 3.1 TeV for simple assumptions.

Diphotons (with 2.6 inverse fb of data)! (Olsen shows an event at 745 GeV).  All diphoton events used.  Peak?  Yes!!  BUT: local 2.6 standard deviations, and with the look elsewhere effect, only 1.2 standard deviations. Not impressive.   Such a peak is not inconsistent with previous results, but doesn’t look like a signal.  Still… combining old and new data we see a signal at 3 standard deviations local, 1.7 standard deviations globally after look elsewhere effect.

Also the peak is rather ragged, though this doesn’t imply anything in particular; it is worth noting.  If you assume the peak comes from a wider bump, the significance goes down.

Now on to ATLAS, with results presented by Marumi Kado (from the French Laboratoire de l’Accelerateur Lineaire and Orsay).

ATLAS has 1.2-1.5 times more useable data than CMS.  This could be important.

Look for Higgs in four leptons.  Big statistical fluke!  They see fewer events than expected! This is, of course, no big deal… if you expect 6 events it is no surprise if you happen to see 2.

No peak in two Z’s at higher mass (i.e. no heavy Higgs seen.)  Some improvement in searches for Heavy Higgs particles decaying to taus at higher mass.

Limits on gluinos (with assumptions) go from 1.2-1.4 TeV to 1.4-1.8 TeV. (Got an improvement by looking for boosted top quarks in the case where gluinos decay to top quarks.)  Bottom squarks (with assumptions) — limits go from 650 GeV to 850 GeV.

The excess in Z + jets + invisible particles in high energy events remains in Run 2, a little smaller than in Run 1 but still there.  [Run 1: 10 expected, 29 observed; Run 2: 10 expected, 21 observed.] CMS still doesn’t see it.  What’s the story here?

Dijets (as I wrote about yesterday.)  Kado shows the highest-energy dijet event ever observed by humans.  Nothing unusual in photon + jet. Nothing in dileptons — limits on typical Z’ bosons in the 3-3.4 TeV range, W’ decaying to leptons limited up to 4.1 TeV,

DIPHOTONS. Here we go.

A completely generic search for photon pairs; nothing special or unusual.  Looking for bump with narrow width up to large width.  3.6 standard deviations local, global significance is 1.9 standard deviations.  Looks amusingly similar to the first hint of a Higgs bump from four years ago!  Large width preferred, as much as 45 GeV. Local significance goes up to 3.9 standard deviations, 2.3 after look elsewhere.  Mass about 750 GeV.  Hmm.  No indication as to why they should have been more efficient than in Run 1, or why such an excess wouldn’t have been seen at Run 1.

WW or ZW or ZZ where there was an excess in Run 1.  As with CMS, no excess seen in Run 2.  WH,ZH: Nothing unusual.

Ok, now for the questions. The diphoton bump seen, with moderate significance in ATLAS and low significance at CMS, is very interesting, but without more information and more thought and discussion, it’s premature to say anything definitive.

Kado says: Run 1 two-photon data was reanalyzed by ATLAS and it is compatible with the Run 2 bump for large width at 1.4 standard deviations, less compatible for narrow width at more than 2 standard deviations.  They have not combined Run 1 and Run 2 data yet.

Kado says: the diphoton excess events look like the background, with no sign of extra energetic jets, invisible particles, etc; nothing that indicates a signal with widely different properties sitting over the standard two-photon background.  (Obviously — if it had been otherwise they could have used this to reduce background and claim something more significant.)  There are about 40 events in the peak region (but how wide is he taking it to be?) Olsen: CMS has 10 events in the same region, too little to say much.

Conclusion?  The Standard Model isn’t dead yet… but we need to watch this closely… or think of another question.

 

 

 

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON December 15, 2015

At CERN, the laboratory that hosts the Large Hadron Collider [LHC]. Four years ago, almost to the day. Fabiola Gianotti, spokesperson for the ATLAS experiment, delivered the first talk in a presentation on 2011 LHC data. Speaking to the assembled scientists and dignitaries, she presented the message that energized the physics community: a little bump had shown up on a plot. (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON December 15, 2015

A few weeks ago, the Large Hadron Collider [LHC] ended its 2015 data taking of 13 TeV proton-proton collisions.  This month we’re getting our first look at the data.

Already the ATLAS experiment has put out two results which are a significant and impressive contribution to human knowledge.  CMS has one as well (sorry to have overlooked it the first time, but it isn’t posted on the usual Twiki page for some reason.) (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON December 14, 2015

The Moon will occult (i.e. move in front of and eclipse) the planet Venus today, as visible (yes, in daytime, if you have binoculars or a telescope) across the United States sometime between 11 and 12:45 this morning, depending on where you live.  Earlier out west, later in the east. If you want to see the heavens are really in motion, here’s a chance.  Below is a link to an article that gives the details:

http://www.skyandtelescope.com/observing/moon-flys-by-catalina-occults-venus-on-dec-7th120220150212/

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON December 7, 2015

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