The Search for New Physics at CERN  Matthew Buckley

March 16, 2016

Anomalous collision events observed in Run 2 of CERN's Large Hadron Collider in 2015 may point to new physics beyond the Standard Model. Image courtesy of CERN.

In February, I spent a few days at CERN, the European Organization for Nuclear Research. I spoke with physicists who devote themselves to understanding the stuff the universe is made of. These were the people who collaborated with thousands of other physicists to find the Higgs boson. Now they are looking for physics that lies beyond the Standard Model—the theory of nature that has dominated the field for more than forty years.
Some of our conversations focused on a puzzling anomaly that was announced at CERN in December 2015. The physicists I spoke with were calm, perplexed, and excited. Calm, because they thought the anomaly might well disappear as evidence accumulates over the coming months. Perplexed, because they did not know what to make of what they had observed. Excited, because they hoped they would find something new and strange that would upset their understanding of nature.
It was depressing to come back to the current political season, with its breathtaking blend of authoritarian bluster, racist garbage, and sheer bullshit. True, politics is not particle physics. Physicists do not declare a discovery until they think the chance of a mistake is less than one in three million. In politics, we do not have that luxury: we need to act. Still, we have a lot to learn from the fallibilist humility that defines fundamental physics: you make your ideas clear, acknowledge your ignorance, and hope for a surprising refutation of settled expectations.
With this piece, Matt Buckley, a theoretical physicist and professor at Rutgers University, begins a series of eight articles that will lead us into these waters. The series starts from the anomaly announced in December and will end with another announcement from CERN in summer 2016, which will tell us whether the anomaly is nature’s signal or just statistical noise. Buckley will lay the foundations for understanding the current calm and perplexed excitement. He will give us a feel for the physics and a sense of how physicists think and work. Politics may not be particle physics, but we have much to learn from this remarkable practice of submitting our beliefs to the discipline of evidence and argument. Physicists will ask questions; nature will talk back; and we will get to watch it unfold in real time.
— Joshua Cohen, co-editor

December 15, 2015, was a very big day at CERN. Certainly it was the biggest since July 4, 2012, when scientists announced that they had found the Higgs boson. This discovery—like the recent discovery of gravitational waves from the merger of black holes more than a billion years ago—was one of the most important scientific events of the last forty years. Named for Peter Higgs, the Scottish physicist who predicted it in 1964, the particle was the final missing piece in the Standard Model, physicists’ fundamental theory of visible matter. Though physicists at CERN were pretty confident that they would find the Higgs, actually finding it was a remarkable achievement: a stunning feat of science, engineering, and human collaboration. The particle was produced by colliding protons at enormous energies in CERN’s Large Hadron Collider (LHC). (Protons are one type of hadron, a special type of subatomic particle.) After it was produced, the Higgs was identified by two big detectors, ATLAS (A Toroidal Large Hadron Collider Apparatus) and CMS (Compact Muon Solenoid).
Following the Higgs announcement, CERN was shut down for upgrades for more than two years. It was fired up again in early 2015, and on December 15, ATLAS and CMS announced the initial findings from this new run. The results were the first taste of the physics of energy scales vastly higher than anything we have ever seen—nearly twice as high as the energies that yielded the Higgs. Buried deep in the talks in December, among the outcomes of many other results from ATLAS and CMS, were a couple of innocuous slides with a few tentative suggestions of something we call “new physics.” Nothing solid, nothing that could rise to level of discovery, but their mere existence had sparked rumors for weeks before the official announcements.
These hints were enough to set wheels in motion. Immediately after the December presentation, all around the world, a thousand physicists ran out of their offices to find someone to start arguing with about the results. Within a day, the first papers hit the arXiv, a public repository of physics and mathematics research, where papers can be posted for comment before peer review. By the end of the month at least 150 papers had appeared. The questions on everyone’s mind then are still on everyone’s mind now. What did the results mean? Are we seeing experimental error? Or random noise, like a blast of static on the radio? Or was this the first sign of physics beyond the Standard Model?
The Standard Model has been the consensus theory in physics for roughly forty years. It tells us that the visible world is made of a small set of fundamental particles, and it tells us how those particles work and interact. If the hints in the CMS and ATLAS data are vindicated—and that’s a big “if”—then particle physics would enter a new era. Our fundamental theory of the natural world would need to change, and no one knows quite how. This chance, however slight, has driven the extraordinary response among physicists to the announcement of the ATLAS and CMS results. Everyone wants to be part of what would be the biggest news in our field—perhaps the biggest scientific news—in nearly a half century.
So what is this Standard Model? What exactly are these experiments? And what did they see that got so many physicists so worked up?
I will explore these questions in a series of articles. CERN scientists will clarify the findings over the next several months and announce new results this summer. As the research proceeds, I will set the stage for the announcement. The idea is to provide you with a basic understanding of the results when they come in—and a sense of why we are all so excited.
• • •
The puzzling new data were gathered at the LHC, a twenty-seven kilometer ring more than a hundred meters underground that curves from CERN headquarters in Geneva, Switzerland, and into France before completing its circuit. When the LHC is in full swing, two beams of protons speed around the ring at 99.9999991 percent of the speed of light. They are kept on their curved path by titanic magnetic fields generated by nearly 10,000 superconducting magnets.
The two beams circulate in opposite directions, just over seven inches apart. But at four points along their underground course, the beams are bent just a bit more and made to cross. The protons come in bunches, roughly 100 billion in each bunch. When the beams cross, which happens 40 million times every second, virtually all of the protons miss their counterparts on the opposite beam and continue back onto the ring to complete another circuit in 0.0009 seconds. But a precious few—maybe fifteen or twenty pairs—collide.
Was this the first sign of physics beyond the Standard Model? If two cars collide head-on, their kinetic energy—their energy of motion—has to go somewhere: to sound waves, to compression of structures in the frame, to propelling pieces of the cars long distances at high speeds. The same is true for the LHC’s protons, except, proportionally, they carry vastly more energy than cars on a highway. In the LHC’s first run (2010–2012), each proton carried enough kinetic energy to make—in principle—over 4000 new protons. (Remember Einstein’s famous equation E = mc2, which means that energy and mass are interconvertible, and that the speed of light squared is the rate of conversion.) In the LHC’s second run in 2015, this value had been increased; each proton carried more than 6500 times the energy needed to make a single proton. (In the units used by particle physicists, a proton “weighs” a bit less than a gigaelectronvolt, abbreviated GeV. The LHC beams now consist of protons with 6500 GeV of energy.) This extra burst of energy, made possible by even stronger superconducting magnets, is what makes this new run of the LHC so exciting.
To understand what happens when protons collide, bear in mind that even though protons are really small, they are not elementary particles—the most fundamental particles in nature. Rather, protons are made of a roiling ocean of particles called quarks and their antimatter counterparts called antiquarks (always with three more quarks than antiquarks), held together by still more particles called gluons. Often a collision of protons just results in a rearrangement of those constituents: the huge kinetic energy is redirected to throw quarks, antiquarks, and gluons off in random directions, much like pieces of a car flying off in a head-on wreck or the insides of a watch when it is smashed against a wall.
Sometimes, however, the kinetic energy from the collisions is channeled into the production of completely new particles. These new particles aren’t constituents of protons, but they can be summoned into existence—for a very, very short time—by the colossal amount of energy available when protons collide. In a later article, I’ll explain in more detail about how to picture this process of producing fast-fading particles. For now, just know that this is why we built the LHC: to give us a chance to see what new stuff comes out when you focus enough energy into a tiny region.
• • •
One thing that can (and did) come out of these collisions is the Higgs boson. Officially, the LHC’s principal aim was to produce and detect the Higgs. Its discovery significantly advanced our understanding of the Standard Model.
Yet although the Standard Model is the most precise and accurate theory ever devised in science, from nearly the moment of its discovery it was known to be incomplete: a hitherto unseen particle with very unique properties had to exist. Otherwise the whole theory of visible matter falls apart. Searching for the Higgs was made harder by the fact that the Standard Model does not predict its mass, so we did not know exactly where to look. Since the 1970s we’ve been searching, in one way or another, for the Higgs: experiments such as the Large Electron Positron collider (at CERN) and the Tevatron (at Fermilab, thirty miles west of Chicago) did not find it. (It turns out that they lacked the ability to pump enough energy into the collisions to create the Higgs in large numbers, though we had no way of knowing that at the time.) The Superconducting Supercollider, planned to be constructed in Texas, would have reached energies vastly greater than the LHC in the late 1990s. But in 1993, after half the ring was built and much political conflict, the project was cancelled. The LHC was the machine that was going to find the Higgs: there were “no-lose” theorems to prove that it could be done, and find it the LHC did.
Of course, throwing two protons together at vast energies is only half the battle. It isn’t enough to create the Higgs; you also have to detect it, which is hard because the particle lasts only for 0.0000000000000000000001 seconds before decaying into other particles. The only way to find it is indirect: by detecting the less massive particles that it decays into. To do this, at each point where the proton beams cross, massive detectors were constructed. ATLAS and CMS are two of them; think of them as very big and very complicated cameras. (ATLAS is 45 meters long, 25 meters in diameter, weighs 7000 tons, and has 10 million components.) These two detectors have very different designs and are run by separate teams of physicists, some 3000 for CMS and 5000 for ATLAS. This redundancy serves as a quality control check: each experiment gathers its own data, analyzes it independently, and each team has a burning desire to beat their counterparts to the punch.
ATLAS and CMS are designed to detect and measure the properties of as many different particles coming out of a proton-proton collision as possible, and to decide whether the collision meets some minimal, if vague, standard of “likely to contain interesting physics.” Most collisions do not pass that test, but for the few that do, the detector relays the information to the outside world, where it is saved for later analysis.
This whole effort is a massive engineering and physics challenge: particles do not come with handy ID cards telling you what they are and where they’re going. Instead, the ATLAS and CMS experiments must track how energy appears to be deposited in various materials that make up their detectors (starting with lots of silicon pixels close to the collision point), and then carefully unravel this pattern to determine what particles went where. The combination of the LHC and its four experiments (ATLAS, CMS, and two more specialized detectors, ALICE and LHCb) are among the most complicated artifacts ever constructed by humanity, and it is all custom-made, designed and constructed by thousands of physicists in labs around the world.
Once the information about what happened in a collision—the “event,” as it is called—has been safely stored “on tape” (a terminological throwback to the days when data-storage was on magnetic tape, rather than solid-state hard drives), the analysis can begin. Though the Higgs boson was the principal reason for the LHC’s construction, it was never the only target. The Standard Model is known to have problems that cry out for solutions. For various reasons, which I will explore in later articles, we suspect that some of these will be solved by physics that becomes manifest at energies not too far above the mass of the Higgs boson itself. There is no no-lose theorem here, however, and the possibilities for what could be lurking at high energies are not quite endless, but certainly immense.
Thus, the experimental physicists working on ATLAS and CMS look for as many things as they can think of. Part of the job of a theoretical physicist is to think up more things to look for, all for the sake of figuring out what the world is ultimately made of and how those ultimate constituents work. One great fear is that there is something new at the LHC and we’re just not clever enough to figure out where to look for it. The other great fear is that there is nothing new to be found. All we can do is cast as wide a net as we can, and be diligent.
• • •
The method of looking for new physics that sparked all the rumors prior to December 15 were the “diphoton” searches done separately by ATLAS and CMS experimentalists. These are very simple searches, as far as these things go. They require none of the baroque tricks that theorists like myself had spent many years developing (though of course they still require the dedicated work of many trained scientists to complete).
Every event at the LHC contains photons (particles of light), thousands of them in fact, with about the energy of the photons coming from an X-ray machine. The experimentalists were interested not in those everyday photons but the ones that contain tens or hundreds of billions times more energy. And not just any photons: pairs of photons (diphotons) that show up at the same time in a layer of the detector that is very good at photon detection. The hope was that these diphotons would be the signal of something new. But, as with many types of particles at the LHC, pairs of extremely energetic photons can be made in lots of different ways, including interactions from the physics of the Standard Model as well as interactions that could arise from a new particle. So seeing a bunch of diphoton events isn’t necessarily interesting; the experimentalists needed some way to distinguish diphotons that might have come from new physics and those that originated in well-understood physics. In particular, they needed a way to pick out pairs of photons that come from some new particle that was produced in a collision of LHC protons and then promptly fell apart (“decayed”), emitting two particles of light.
One fear is that there's something new to be discovered and we're just not clever enough to find it. To do this, they relied on a useful property of particles—useful, but a little complicated. One of the things that defines a particle is its mass, and one of the properties of mass is that no matter how you are moving relative to a particle, or how the particle is moving relative to you, you will always measure the mass to be the same value. (In other words, mass is what physicists call a “relativistic invariant.”) A proton always has a mass equivalent to a bit less than 1 GeV in energy, for example. A massless photon is always seen as having zero mass.
Suppose now that you create a new particle in a collision between protons, and suppose that the new particle decays eventually into two photons. Those two photons inherit some information about their parent. While an individual photon is massless, you can take two photons and combine their energy and momentum to construct something called the “invariant mass” of the pair. This invariant mass, denoted mγγ (pronounced “m-gamma-gamma”), is the same as the mass of the parent particle. So if you can make many such new particles and capture the light from their decay in the detector, you will see many pairs of photons, all with the same invariant mass. For example, if you make some Higgs particles, and they decay eventually into photon pairs, the invariant mass of all the pairs will be the same as the mass of the Higgs.
For pairs of photons that are just produced from some random smashing of a proton against another proton, this quantity, the invariant mass of the two photons, will not always be exactly the same, as the photons can be produced in all sorts of ways, not just from the decay of a single type of particle with a unique mass. In general, in such collisions mγγ will be smoothly distributed, roughly tracking how much energy went in to making the pair of photons; the bigger the invariant mass of the photon pair, the less often we will see it.
So when you create a new particle (say, a Higgs) that sometimes decays to create diphoton events, you will see an elevated number of those events, all with the same invariant mass. If you plot the number of events with a given invariant mass, this results in a “bump,” which will stick out like a sore thumb over the “background” of diphotons created in other ways. For this reason, such searches at the LHC are called “bump-hunts.”
Here is an example. The Higgs is one particle that can decay into a pair of photons; one of the ways that the Higgs was discovered was through exactly this sort of bump-hunt. The Higgs has a mass equivalent to 125 GeV of energy. (Particle physicists use the same unit for mass and energy, again because of E = mc2.) So, when ATLAS and CMS collected events, they started to see an excess of diphoton events around an mγγ of 125 GeV. Of course, they didn’t know ahead of time that the Higgs mass was 125 GeV: they learned it only by seeing this bump and working their way back from there.
You can see the progression of the Higgs search in a handy gif the ATLAS experiment created afterwards. In the animation, the number of diphoton events collected is increasing as time goes by. The horizontal axis is the invariant mass mγγ of the diphotons measured by ATLAS, and the vertical axis is the number of events with diphotons that have a particular invariant mass.
Animation showing ATLAS evidence for the Higgs boson during Run 1 of the LHC. Image courtesy of ATLAS/CERN.
In this animation, there is a nice smoothly falling “background” of diphoton events. These are coming from well-known Standard Model processes. Then, at an invariant mass of 125 GeV, you start seeing a visible excess creep out over the background, once enough data has been collected. That’s the Higgs, as it was discovered at ATLAS: it was created in collisions of protons and then decayed into a pair of photons, which remembered enough of their parent to show up on this plot as a bump at a particular invariant mass.
• • •
As the Higgs discovery demonstrates, diphotons can be used to discover new physics. But it isn’t the only way to do so, of course. There are literally hundreds of possible ways to look for something new at the LHC. But diphotons are a “clean” way to look: the particles in the collision are relatively straightforward for the experimentalists to see in their detectors (they show up as pairs in what is called the "electromagnetic calorimeter"). They are also relatively straightforward to analyze; the invariant mass gives a simple way to see new physics jump out at you from the data. All this sort of search needs, then, is a new particle that can decay into a pair of photons.
This finally brings us back to the results of the ATLAS and CMS searches announced on December 15. Here is the ATLAS data:
Diphoton ATLAS data from Run 2 of the LHC. Image courtesy of ATLAS/CERN.
And here is the CMS data:
Diphoton CMS data from Run 2 of the LHC. Image courtesy of CMS/CERN.
These plots, like the Higgs plots above, show the number of events with diphotons that have a particular invariant mass. The difference is that these new plots come from the second run of the LHC, which collides protons at higher energies. That means the experimentalists can hope to make more massive new particles and can look at higher invariant masses of diphoton pairs than they could before.
There are a bunch of things going on with these plots, so let me draw your eye to particular features. First, in both cases, the experimentalists have drawn a background line (red for ATLAS, blue for CMS). This is their best estimate for the number of events that they should see at a given invariant mass, according to the Standard Model. Notice that the actual number of events at any given invariant mass doesn't always match the prediction. Such departures are especially pronounced at the far right side of the plots, where the invariant mass is largest. Here, the number of predicted diphoton pairs is very small, less than one per range of invariant mass. Since you can't actually see a fraction of an event—it either happened or it didn't—the predicted and observed numbers of events are expected to deviate, and the way experimentalists compare what they expected to see and what they actually saw takes these small number of events into account.
Away from the right-side tail, however, the background prediction and actual number of events are in pretty good agreement, though they are not exactly the same. That’s as it should be. A background estimate is exactly that: an estimate. If you flip a coin a hundred times, you expect it to come up heads about fifty times. But you’re not going to be very surprised if, after a hundred flips, you have sixty heads. That’s not quite the expectation, but some percentage of the time you’re going to get fluctuations away from that value. As long as those fluctuations aren’t too far away from your expectation, you’re not too bothered. Of course, if you flip a coin a hundred times and see ninety-four heads, you might start to suspect that your coin isn’t a fair coin. Critically, though, you couldn’t say for certain that the coin is biased, no matter how frequently and extremely it departs from the average value you expect. All you can say for sure is that it’s extremely unlikely that the coin is fair (and you could put a specific number on how unlikely it is).
The background lines in the CERN plots are like the expectation of seeing fifty heads in a hundred flips of a coin. Deviations around that expected value are consistent with the Standard Model, as long as those deviations are small compared to the number of diphotons collected. But if you see a large fluctuation away from that expectation, you have some reason to believe that there’s something else going on (new physics, or a biased coin in the analogy). I’m simplifying a little, of course, since the background expectation for ATLAS and CMS have to be determined using the data itself. This is unlike the fair coin example, where the background expectation is something you can figure out ahead of time.
As you read the ATLAS plot from left to right (increasing invariant mass along the horizontal axis), you see the actual number of events detected (the black crosses). They more or less track the background expectation, though there are some small deviations both up and down. But then, at an invariant mass of 750 GeV, there is a rather large bump: there are about twenty photons around this invariant mass. Now twenty is not a lot in absolute terms, but the Standard Model tells us that the number should be closer to eight. So we have a huge upward fluctuation from the background. That can happen simply due to random chance, just as it can happen that you can flip a fair coin a hundred times and get seventy-five heads. But if that happened with a coin, you would start looking at it pretty closely, wondering if something was going on.
We can put a number on how unlikely it is. Remember that the Higgs was found through a diphoton bump. How likely was it that the bump was due to chance? Not very likely: 1 in 3,488,560.
Similar calculations show that the ATLAS bump at 750 GeV could occur by chance only once in 6285 tries. That sounds pretty convincing. But recall that we had no special reason for looking at 750 GeV. We would have been equally happy with a big fluctuation at any invariant mass: 740, 730, 720, and so on. In effect, we “tried” many times to see a fluctuation, and we have to take that promiscuity into account. This is called the “look-elsewhere” effect.
Think of the look-elsewhere effect using the following analogy. You have a 1 in 365.25 chance of sharing the same birthday as any random individual. Imagine that you meet exactly one person, and you ask what their birthday is, and it is the same as yours! You’d be right to be very surprised. However, imagine that you run into a hundred people, and you ask all of them what their birthday is. Suddenly, the chance that someone shares a birthday with you is about 25 percent. You’ve looked in a lot of places, and so getting one result that’s somewhat rare becomes a lot more likely. Seek and ye shall find—or have a pretty good chance of finding, anyway.
Applying this “look-elsewhere” reasoning to the ATLAS search drops the odds of the bump being the result of random fluctuation from 1 in 6285 to around 1 in 44. That’s really not very low: in physics such numbers are routinely filed under “maybe interesting, but wait and see.” ATLAS does hundreds of searches, so about 1 in 22 will have a fluctuation of that order of magnitude in their results. We’re used to that.
But now look at the CMS plot. Instead of scanning your eye from left to right along increasing invariant mass, jump straight to 750 GeV. ATLAS already told you to look there, after all. And what’s that? At 750 GeV in the CMS data, you find a few more events than there “should” be, according to the Standard Model. Maybe ten events, while you were expecting four.
By itself, this result should happen due to random chance about 1 in 214 tries. If CMS were the only experiment to report such results, you’d have to apply the look-elsewhere effect again, and the significance of this result would drop precipitously. But ATLAS already told us this particular region was interesting; we no longer need to look elsewhere. And since the CMS and ATLAS experiments are completely separate from one another, we’ve basically tried twice to test the physics at this particular invariant mass, and in both cases we’ve come up with something that is really unlikely.
That is what makes this result so interesting: seeing something unusual not once, but twice, in results from groups that have different experiments, different ways of collecting data, and different ways of analyzing their data, and that don’t share their results with each other ahead of time. To some degree, one experiment provides an independent validation of the other.
But even this convergence of independent evidence is not definitive. This kind of coincidence has happened before even though the results turned out to be insignificant upon closer inspection. Two experiments can see unusual results in the same spot, and then, when more data comes in, everything can revert back to the expectation. After all, the LHC experiments look for new physics in a lot of places, so unlikely things can happen. Therefore, the safest bet, based on past experience, is that these results will also disappear once we get more data from another LHC run. Perhaps we just stopped the LHC collisions at a time when both experiments had a few more diphotons than normal. Physicists who say this have an annoying track record of being correct.
The flip side is that this particular result—as far as I can tell—is the most surprising result to come out of the LHC other than the discovery of the Higgs itself. In short, the CMS and ATLAS results combined are the mostly unlikely things to have been seen if the Standard Model is the only physics around, other than the one time we discovered a new particle.
That’s enough to get a lot of people sitting up and paying very close attention.
• • •
If the CMS and ATLAS hints pan out, we’ll have discovered something completely and utterly new. That hasn’t happened in a very long time in collider physics.
In fact, we can go even further. Based on this first round of data—and you have to keep in mind that the results are very preliminary—we can say that if these diphoton bumps are real, they are the sign not only of new physics, but of new physics of a kind we were absolutely not expecting. We know they would point beyond the Standard Model, but we do not know the direction they would point us in.
If the elegant idea can't explain the data, so much for the elegant idea. In the years leading up to the construction of the LHC and then the discovery of the Higgs, theoretical physicists had plenty of time to think about what should be lurking above the energies we had tested with other colliders. There were, of course, many ideas. But several gained popular currency thanks to the “elegant” ways they solved the problems we were wrestling with. (Mathematicians and physicists speak often of searching for “elegant” theories. The mathematician G.H. Hardy went so far as to say “there is no permanent place in the world for ugly mathematics.”) These theories tend to predict lots of different particles, with many different signals that would appear at the LHC, given the energies that are now being attained. Simple versions of these theoretical ideas have become benchmarks against which we test the ability of the LHC to find new physics. Interestingly, even though these benchmark theories were chosen specifically because they could result in so many interesting signatures at the LHC, they do not predict the signal we’re seeing in the ATLAS and CMS diphotons. The excess at 750 GeV is a little too weird to be explainable by these elegant ideas we’ve spend several decades honing.
That is why it is such tremendous fun to try to explain these new results. Without new physics, we theorists had to rely on aesthetic criteria—a certain degree of elegance, an economy of design—to guide our intuition about the “right” idea to pursue. But the universe never promised us a rose garden. If the elegant idea can’t explain the data, so much for theoretical aesthetics. The demand for beauty goes out the window in the face of experimental hints, and you’re free to consider ideas that are ugly but get the job done (though everyone will have their own personal measure of what counts as too ugly to consider pursuing). So there’s a flurry of activity, and optimistically, someone will stumble on the right idea, which might turn out of have aesthetic appeal all of its own.
In the end, we can only say one thing for sure: we need more data.
From a personal perspective, it is incredibly frustrating not to know what to make of these new results. The time physicists spend working on this is time we are not working on other ideas, ideas that we can be sure will continue to be important even after the LHC turns back on in a few months. To spend your time pondering something which could be flat out untrue is scary from a career perspective and dispiriting from the perspective of wanting to know how the universe works. To be not just wrong (which is part of the job), but irrelevantly wrong, wrong in a way that teaches you nothing? That’s not what any of us want.
On the other hand, this work is deeply exciting. It is what science is all about—at least the part of science that most scientists dream of (the remaining bits being some mixture of hard work, coffee, grant writing, more coffee, conferences, and gently banging your head against a wall).
For someone like me, in my mid-thirties in particle physics, this is brand new: we’ve never had a truly unbelievable surprise. It was great to find the Higgs boson, but it fit perfectly into the received theories, ideas that I studied in graduate school. We don’t know whether this diphoton excess is the first step into the undiscovered country beyond the Standard Model. But ATLAS and CMS are breaking new ground, reaching energies that have never before been probed by humanity.
In this series, I will try to guide you through this exciting work. By the time I get to the end, I hope to be able to tell you what is going on with those photons we saw at the LHC. The safe bet is that I will have to report that this result, like many others, is not interesting. But maybe not. I don’t know, and neither do you; that’s the beauty of it.
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"You shall not find any new physics, because all physical events are interpreted well-known particles (leptons, quarks, and gauge bosons) and forces which have long known (electroweak, gravity, strong interactions)."
Quznetsov G 2013 Logical foundation of fundamental theoretical physics (Lambert Academic Publ.)


Not so. Our understanding of Gravity is extremely basic. Much less is known about gravity than teh other three forces. Beyond that, in order to unify Gravitry with the other forces, it's probable that there will need to be a paradigm shift in our understanding of physics somewhere on the order of Einsteins Relativity Theory.
The more we learn, the more it becomes clear that we don't know more than we know, you know? I mean, it's only within the last two decades that it was discovered that the Universe is accelerating at an ever increasing rate. Believe me, there is new physics to be discovered.

Dark matter and dark energy make up most of the universe. Neither of them interacts with photons and so they're entirely outside the Standard Model. We still have a long (and exciting!) way to go...

Most of the universe is composed of dark matter and dark energy. These don't interact with photons and lie entirely outside the Standard Model. We still have a long (and exciting!) way to go in understanding the universe.

What an excellent article! Thank you so much. I shall look forward avidly to reading the rest in the series, leading up to the announcement in the summer. Bravo!

Higg's Particles (it has mass of 125 Gev) are not the final mass less fundamental particles for understanding of the origin of mass of subatomic particles in the particle physics at Big Bang and Higgs particles do decays into photons ( Professor peter Higg [ click on URL -…/physics/l…/2013/higgs-facts.html] and Prof François Englert [ Click on URL -…/laureat…/2013/englert-facts.html] were both awarded Nobel prize in physics for higgs particle for theoretical discovery of a mechanism that contributes to our understanding of the origin of mass ) .Gluon's are still now considered as "zero rest mass particles" in standard model of Big Bang ,Now has yet to be proved in LHC in CERN . A new particle found in LHC at CERN's in 2015. Is that particle bi photon or is that particle "Graviton"- the Zero rest mass particle in Planck moment of standard model of Big Bang created before the ghost neutrinos particles billion of. which passes every seconds piercing us. and planets as Ghost particles. Neutrinos has also its mass [ Prof Takaaki Kajita and Prof Arthur B. McDonald were awarded Nobel prize in Physics for 2015 for the discovery of neutrino oscillations, which shows that neutrinos have mass click on URL…/physics/laureates/2015/]
Graviton ,a zero rest mass particles-responsible for the Gravity or it is the Tachyon particle which is faster than light particle{FTL] as we published in 2015 in International Journal of Astronomy, Astrophysics and Space Science Pages: 12-29 | Vol. 2, No. 3, June 2015 |
A new physics has to be written then . Thanks to my youngest sibling brother Mr. Rupak Bhattacharya BSc ( Calcutta university ) MSc (jadavpur univ.) who is s/o late Mr. Bholanath Bhattacharya and late Mrs Bani Bhattacharya of residence 7/51 Purbapalli ,PO- Sodepur ,( north 24 parganas) west Bengal; kolkata- 700110, India ( his D.O.B- 1974 march)- a free Lancer Theoretical physicist who told me in year 1995 that "Gravity" is not a simply force but rather composed of a zero rest mass particle may be called as "Graviton". And I asked his same idea to Nobel Laureate in physics Prof. David Gross[…/physics/l…/2004/gross-facts.html] in "ask a Nobel laureate " on June 28 th 2010 and prof John C Mather[…/laureates/2006/mather-facts.html] in the face book of Nobel The same was published also as a blog article in extreme astronomy under title "what is Gravity? Is it a force by zero mass particle called Graviton" on June 13; 2010 and in Prof Stephen Hawking's face book on August 25 2010. links will be followed here .link is with this face book also for ones check in 2010 June to august .Please scroll down to posts in years 2010 and find those links related with Gravity. Let us await what the new particle now stand for.
Links For Gravitons and ask to Nobel Laureate David Gross as Gravity is not a simple force but a particle " called Graviton" a zero rest mass particle in Nobel prize,org face book[] Links are
4] Link on faster then light particle " tachyon" Tachyon- Faster than Light Particle Exist in Our Universe or an Imaginary Mathematical Particle at International Journal of Astronomy, Astrophysics and Space Science Pages: 12-29 | Vol. 2, No. 3, June 2015 |…
I am dam sure it is not bi photon. nor a new types of higgs particle. May be it is Gravitons or Tachyons Let me hope so


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The Search for New Physics at CERN