Clusters of Clicks

We’ve been analysing your clicks on the images to see just how good human beings are at identifying off-centre vertices, and the news so far is pretty encouraging – I’ve produced a few images that highlight the clusters of clicks on data images where you saw three or more vertices: here are a few of the more striking images. This is just a very small sample, as the algorithm identified over a thousand such clusters of clicks:

a

AHH0000k2d has an interesting track that appears to go backwards!

b

AHH0000k1h

As discussed in the FAQ, the colourful tracks usually indicate OCV tracks found by a computer algorithm. In this case it’s pretty clear that humans found some tracks that the computer missed!

c

AHH0000j04

Again, a mixture of tracks that were found by the computer and those which required humans to find!

d

AHH0000hnk

This is one of the many images you’ve identified with missing muons – we’ve seen a few of these which were diagnosed as cosmic rays, but this one seems to have an OCV as well.

Another notable observation from this data is that lots of people have been identifying the colourful ellipses that are sometimes produced in the detector as “weird”. They do look very unusual, but again, these are artefacts produced by the algorithm that draws the tracks, and aren’t (unfortunately) physically interesting. A reminder that things like large deposits of energy, tracks that bend suddenly in the detector, or beams of particles at wide angles are potentially candidates for “weird” observations – although, if in doubt, it’s best to flag it as weird, as we’re looking into analysing the images that lots of you have flagged up as being unusual (regardless of where you click.)

Good work, everyone – keep it up!

LHC Run-2

Since the last time this blog was updated, the LHC has been restarted and, in the last month or two, the floodgates have been reopened and data from the detector has again started to flow. In the finest traditions of Hollywood, the sequel will take all the elements of the original and turn it up to eleven – or, in this case, 13 TeV, the new collision energy for protons in the LHC. These record-breaking energies mean that the protons are travelling at a brisk 0.99999999c. At such speeds, the relativistic effect of time dilation means that – if you survived – every second you experienced would be nearly two hours for your friend remaining on earth. These effects, while fascinating, have been well-understood for many years: even the Higgs boson had been predicted in 1964. The exciting prospect with the second run of the LHC is that we are entering the realm of new and sometimes controversial physics. While the first run had a clear target, the Higgs, at a known energy, the second run aims to ramp up the collision energy and simply see what we find.

The potential candidates for discovery by this second run-through are numerous. If there is a new ‘holy grail’ of particle physics after the discovery of the Higgs, then arguably it’s dark matter – a name to make film studio executives drool, certainly. On the face of it, you might wonder how particles which are apparently so arcane and difficult-to-produce can really be relevant to our world at large. After all, none of the potential candidates for dark matter have ever been isolated or observed in the laboratory. But it is a testament to the beauty and complexity of the universe that the smallest details of the fundamental particles that make it up can have a huge impact on the grandest possible scale. Take another boson – not the Higgs, but the W boson, which mediates the weak interaction, detailed in this post.

If the mass of this particle were to be slightly greater, the rate of nuclear fusion in the sun would be quicker, it would have burned for a briefer time, and humanity may never have had time to evolve. If its mass were below a certain threshold, the Sun may never have produced enough energy to allow life to evolve. For the first particle physicists, this fortunate lifespan was observed by measuring the length of a line of bubbles in a cloud chamber. The detectors in the LHC are the spiritual heirs of these slightly less sophisticated methods, but the inferences we can make still have profound consequences.

Dark matter provides another example of how the nature of subatomic particles can influence structure on the grandest scale. The predicted gravitational interactions between stars, galaxies and other large-scale structures were inconsistent with the amount of mass that was actually observed. As well as this, the universe seems to be flat – having no overall curvature. At the same time, cosmologists can measure how its expansion is accelerating using the light from distant supernovae. For these results to be consistent, matter in the universe should have a certain average density of around 6 hydrogen atoms per cubic metre: but visible matter is only 4% of this. Most cosmologists are certain that dark matter explains these phenomena, so particle physicists are looking for a new subatomic particle that – unlike protons and electrons – doesn’t interact electromagnetically, and so doesn’t absorb or emit light. Like the Higgs boson, predictions of dark matter have been around for decades, and models that feature it have become very sophisticated, but until it is actually observed there will still be some controversy, with leading alternative models including modifications to our current theory about gravity.

One of the historical candidates for dark matter are WIMPs, or weakly interacting massive particles. The fact that we expect dark matter particles to be “invisible” and also stable makes them difficult to detect. A lot of the experiments attempting to detect WIMPs use the same method as the Kamiokande experiment in Japan, which principally looks for neutrinos. A large vat of water, usually deep underground to reduce the effects of background radiation, is filled with detectors which look for the effects of collisions between the WIMPs and the nuclei of atoms in the water. These experiments have not yet produced convincing evidence of WIMPs, and it’s also worth noting that their mass was predicted to be around 100GeV, so not beyond the range of the LHC even in its original run.

With WIMPs still not yet observed, the search has moved towards more exotic particles. The theory of supersymmetry, which was also discussed in a previous blog post, is a key theoretical development that physicists hope can be confirmed by this run.

Elementary particles are divided into fermions, with spin ½, 3/2 etc. and bosons, with spin 0, 1, 2…. Supersymmetry suggests that for every particle in the standard model there is a partner with a significantly higher mass, and in the opposite category – so for each of the quarks, there’s a “squark”, and for gluons which are the force-carriers for the strong interaction, there are “gluinos”, and so on for every elementary particle. Each boson has a superpartner that is a fermion, and vice versa. One advantage of the supersymmetry extension to the standard model is that it predicts a set of particles over a range of masses, and the lowest of these is expected to be stable; it could be a weakly interacting particle that still exists from the early universe. Again, the lightest supersymmetric particle could be produced in the LHC, but would be difficult to detect. To date, there has not been convincing evidence of superparticle partners, although the wide range of possible masses that these models allow means that we also can’t eliminate the theory based on data from the LHC. Particle physicists instead focus on narrowing down the possible ranges for the parameters which define this model.

There are other targets for the latest run of the LHC. Just recently the news has reported the discovery of the pentaquark – a new type of baryon. Previously, all detected subatomic particles that were made up of quarks either had three quarks (baryons) or a quark and an antiquark (mesons) bound together by the strong force. As the name suggests, the pentaquark consists of five – more specifically, four quarks and one antiquark, giving it a spin of 1 and a range of possible charges. The specific configuration of quarks that has been observed is two up quarks, a down quark, a charm quark and an anti-charm quark. The pentaquark was certainly an unexpected discovery by the LHC, and has not yet been confirmed entirely; scientists are likely to be cautious, because the claims that a pentaquark was discovered ten years ago were eventually refuted. Pentaquarks are not candidates for dark matter, because they will interact electromagnetically, but the fact that new and unexpected discoveries have been made so soon after the start of the new run is indicative of just how much there is left for us to find in the ever-increasing particle zoo!

In the next entry, I’ll give you a quick update on the analysis of your clicks so far. Happy hunting!

Tell me the truth!

As you know, on HiggsHunters we have been giving you not just real data images from the ATLAS detector. We have also been showing simulated images of what ATLAS detector events would look like if the Standard Model were extended with various new particles and interactions that would give displaced vertices. So what are these simulations of exactly, and why are they important for the science at HiggsHunters?

The simulations are of Z plus Higgs events, where the Z decays to a pair of muons (see last post!) and the Higgs boson decays to a pair of new, long-lived, neutral particles (called “a” bosons). Such a model is predicted by various theories which are possible extensions of the SM. These “a” bosons can then themselves decay, after some lifetime, back to SM particles. The parameters of this model are:

  • the mass of the “a” boson
  • the average lifetime of the “a” boson
  • what SM particles the “a” boson decays to

Since this is unknown new physics, these parameters are not known! But we can make some educated and motivated guesses based on theories of SM extensions and exclude values that would have allowed the “a” boson to be seen at previous experiments. For our simulations on HiggsHunters, we chose the following values:

  • mass of either 8, 20, or 50 GeV. Recall the Higgs boson mass is 125 GeV, so we need the “a” boson mass to be less than half the Higgs boson mass if the Higgs boson is to decay to a pair of “a” bosons.
  • average lifetime (times the speed of light) of 1, 10, or 100 mm. We’d like to have a chance of seeing it decay displaced, and within the detector. Note that this does not mean the displaced vertex will always be 1, 10, or 100 mm away from the collision point, anymore than dogs who live an average of 11 years will all die on their 11th birthday! The probability that a particle with average lifetime, L, decays after a length of time, t, is proportional to e^(-t/L). Dogs have a more complicated distribution!)
  • “a” boson decays to either a pair of bottom quarks (for an “a” mass of 20 or 50 GeV) or tau leptons (for an “a” mass of 8 GeV). This is based on the expectation that Higgs-like bosons usually decay to pairs of heavy SM particles more often, since they couple to mass.

This gives us 3×2+3×1=9 possible parameter combinations to simulate. We present a roughly equal number of all 9 on HiggsHunters. Below is an image of an event simulated with the parameters: “a” mass = 20 GeV, “a” decay to a pair of bottom quarks, and “a” lifetime = 100 mm. Since this is a simulation, we know where the decays took place – they are drawn on the image as pink dots.

truth_atlantisXY_110202953_004966

Here are a bunch more of these (XY, XYzoom, RZzoom), for your viewing pleasure! (These have “a” mass = 20 GeV, “a” decays to bottom quarks, and “a” lifetime = 10 mm.)

But when we give them to you on the site, you don’t get to see the pink dots! Wouldn’t that make life easier for you?! Well, yes, but the point is that by testing you all with these simulations we can measure your ability (efficiency) to have found such displaced vertices if they were to exist in the real data. This is very important for us to draw scientific conclusions from the results of the HiggsHunters project! (We also can’t show the pink dots to you right after you classify it, since each image gets classified by ~20 people. We can’t reveal the truth until after the image is done being classified by everyone! We could make the truth images available on talk at some point in the far future.)

If you all manage to find evidence for some new particle giving displaced decays, we need to know how often this process is occurring in the LHC pp collisions. (Well, we would also need to celebrate with some Champagne first!) How often it happens is given by how often you see it happening divided by your efficiency to see it happen. It is this efficiency which we can measure using the simulations, for each set of model parameters.

If instead you manage to go through all the data and find no new particles, we have still learned something very interesting! (No Champagne needed though, unfortunately.) We will have learned that these new particles are not being created at a rate that is large enough so that you would have seen them. This rate (for each particular set of model parameters) is very interesting to theorists who work on possible extensions to the SM and is given by about 3 divided by your efficiency to see it happen. So here again, these efficiencies measured with the simulations are essential. (In case you’re curious, the “3” in the formula above comes from the fact that to have at least a 95% chance of having at least 1 event occur, you need to expect about 3 events to occur on average. You can always just get a little unlucky and the events don’t occur even if on average you would have expected them to! For more info, read about the Poisson distribution. I also love this Poisson calculator – try typing in x=1 and avg. rate of success=3, you should see P(X>=1)=0.95!)

That’s it! Be proud that your abilities have been calibrated, and you are now ready to tackle the larger sets of real data we plan to upload to the site soon!

What you’re seeing on HiggsHunters

Since you’ve all been diligently classifying for over a week (and doing a fantastic job!), we from the science team thought we should explain to you all a bit more about the physics you’re looking at and what these events are! How do we go from the 20 million proton bunch collisions each second happening inside the ATLAS detector in 2012 to the images on your screens?

First, remember we’re trying to find exotic decays of the Higgs boson. If you just chose random collisions, you’d have just about a 1 out of 10 billion chance of picking one with a Higgs decay in it! So we need to select events (proton bunch collisions) which are enriched in Higgs bosons. Most of the time, the Higgs is produced by itself, and then decays. Unless you know what it is decaying to and can select on that, you have no way of enriching the sample. (This works for many SM Higgs searches/measurements, e.g. where its decays to photons or Z bosons can be selected.) We chose a method that is blind to what the Higgs decays to, thus letting us potentially see any new exotic decay. About 2% the time, the Higgs boson is produced along with a Z boson, in the same event (according to the SM calculations). About 3.3% of the time, this Z boson decays to a pair of muons. We select this 0.07% of Higgs bosons using the di-muon trigger and record them. There should be about ~150 events like this in our 2012 data (with 2 muons with transverse momentum above 20 GeV/c and |eta|<2.5 and dimuon invariant mass within 20 GeV of the Z boson mass).

Unfortunately, these 150 events are accompanied by ~4 million events that just have a Z decay to two muons and no Higgs boson! To improve our chances of having a Higgs, we use another trick – require the Z to be moving away from the beamline. If there’s a Higgs and a Z, they tend to move away from each other in opposite directions. A Z by itself tends to go almost nowhere. By asking that the Z has a transverse momentum above 60 GeV/c, just 5% of lonely Z events survive, but we retain 60% of the 150 Z+Higgs events, so 90 left out of 200k Z background. (Not bad, we’ve gone from about 1 / 10 billion to about 1 / 2000!) Finally, we enhance the chance of something interesting going on by asking for missing transverse momentum  above 40 GeV/c. This means that some particles have escaped without interacting (like neutrinos, or dark matter!), or some of the particles were mismeasured. This leaves us finally with 50 Z+Higgs events if the Higgs decays to long-lived particles which themselves decay to pairs of bottom quarks or tau leptons (more on our simulations and models later!) and “just” ~50,000 Z events for you all to search through to find them (along with those simulations).

Now that the events are selected, we have to reconstruct those displaced tracks! To do this, we save all events with a Z decaying to muons in a format that has all tracker hits saved (those thousands of little dots in the tracker pictures). Standard ATLAS tracking only reconstructs tracks that start from within 10 mm of the collision point, but for this study we reconstruct track paths that start up to 10 cm from the collision point. We also run a custom vertexing algorithm which attempts to find displaced vertices (hence the colored tracks and little ovals). But we hope you will do better! Reconstructing the data with these settings is slow… it takes about 10 minutes on average per event! For 50,000 events, that’s ~1 year of CPU time. Of course, we are clever and split the work up over hundreds of machines as part of the “world wide grid”, so is just takes a couple days.

Finally, we download all the reconstructed data (about ~250 GB, from 5 MB per event) and make these wonderful pictures! This process happens on a machine in my office (see below). Running several instances in parallel, I can make about 1 image each second, which lets me finish all 50,000 overnight.

2014-09-08 17.51.57

Not everything is being shown in the pictures. We cut down the information so you can ignore the boring stuff and more easily see displaced vertices. We only draw tracks with transverse momentum above 2 GeV/c, which start at least 0.5 mm from the collision point. (Most particles come directly from the collision point, and are low momentum.) We also don’t draw tracks that start more than 20 cm from the center of the detector or the selected collision point in the direction along the beamline. To cut down on fake tracks, they must have at least 7 hits in the silicon strip tracker. Vertices shown must have at least 3 tracks. Muon tracks must have transverse momentum above 10 GeV/c, and jets of hadrons must have transverse momentum above 40 GeV/c. Other objects (photons, electrons, bottom quark jets, etc.) are drawn as long as they have transverse momentum above 5 GeV/c.

Once done, they’re zipped up and sent to the Higgs Hunters site!

That’s it! Happy hunting!

ATLAS: How do particle detectors work?

The Large Hadron Collider (LHC) is a truly sophisticated machine; weighing in a 37,000 tonnes and residing in a 27km long tunnel it is the most sophisticated machine ever built. With over 9,500 magnets super-cooled to a temperature of 1.9K (-271.3C, colder than space!), the LHC can accelerate two beams of protons to 99.999999% the speed of light, before smashing them together inside four giant particle detectors. In doing so, it can recreate the conditions that were present less than a billionth of a second after the Big Bang.

ATLAS at the LHC - an incredible feat of engineering!

ATLAS at the LHC – an incredible feat of engineering!

ATLAS is one of those particle detectors, and was one of two experiments to discover the Higgs boson in 2012. It is over 46m long, 25m in diameter, weighs over 7,000 tonnes and contains around 3,000km of cable. Over 3,000 physicists from over 175 different institutions in 38 different countries work together on the project. Following the Higgs discovery, ATLAS is working on learning more about the properties of this new particle, as well as looking to discover new exciting physics (such as extra dimensions and dark matter candidates).

When two beams of particles collide at extremely high energies, new particles of matter can be created from that energy. This is possible because of Einstein’s famous equation, E=mc^2, which tells us that mass(m) and energy(E) are actually the same thing. These events take place inside machines called particle detectors, sending showers of particles in all different directions.

Diagram of ATLAS

Diagram of ATLAS

As charged particles move outwards, they allow electrons to move in atoms of silicon or strip electrons from gas atoms (the gas used is Xenon). By detecting these signals in the particle tracker and joining them up, a picture of the path the charged particle took can be built up. These paths are curved because the detector is immersed in a strong magnetic field, how curved they are tells us the momentum (related to their speed) of the particles. Outside the tracker are the calorimeters, which are designed to absorb the charged and neutral particles so we can measure their energy. With this information, we can work backwards and find out the properties of the particles produced in the collision.

If we see an off-centre vertex, it tells us that an uncharged particle (which is invisible to the tracker) has decayed into charged particles, which could be a sign of an exotic Higgs decay!

The Higgs boson Part 3: Exotic Higgs decays

The Standard Model predicts that the Higgs boson is unstable and falls apart (decays) only 10-22 s (0.0000000000000000000001 seconds) after it is created. Theoretically, it can decay to a quark-anti quark pair (except for top, anti-top), a lepton anti-lepton pair or to two bosons (like photons or gluons).

However, there is also the possibility that it could decay to new particles that have not been observed until now, so-called long-lived scalar particles (scalar means they are spinless just like the Higgs boson). Some theories beyond the Standard Model (e.g. http://arxiv.org/abs/1312.4992) predict that these particles would be unique in that only the Higgs boson would decay to them, meaning it would have been impossible to study them until now – these are one example of what we call ‘exotic particles‘.

An exotic Higgs decay producing two off-centre vertices

An exotic Higgs decay producing two off-centre vertices

The diagram above shows a Higgs boson decaying into two exotic particles, which then themselves decay into many more particles – this is how an off-centre vertex could be produced. In fact, looking for off-centre vertices was proposed way back in 2006 as a way of detecting the Higgs boson, before it had been discovered (http://arxiv.org/abs/hep-ph/0605193)!

Since this process is not predicted by the Standard Model, if we see these in our detector then we will finally be able to realise the dream of obtaining direct evidence for a new theory of nature – opening our eyes to an entirely new realm of physics.

If these exotic decays are real, then they have already happened at the LHC and are sitting in the data we have right now, just waiting to be found by a keen pair of eyes. By helping with this project, you can take us one step closer to a deeper understanding of reality – to answering some of the greatest unsolved mysteries in the universe.

(Next time: ATLAS: How do particle detectors work?)

Simulation Overload

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We had a great launch last week and Higgs Hunters was off to a flying start. After a day or two though, we realised that something wasn’t right. Over the weekend, you all began seeing way too many simulations. That should start to fix itself now. Here’s what happened, and how we want to move forward:

On many Zooniverse projects, there are simulated data mixed in with the real data. We do this to help calibrate the project as a whole, and, in the case of Higgs Hunters, to see what sort of events can easily be seen in this data, and what can’t. It became apparent over the weekend that the balance of real and simulated data on Higgs Hunters was wrong. Several weeks ago when the ATLAS team delivered the Higgs Hunters data to the Zooniverse, a piece of metadata was missing and the developers at Zooniverse thought that a whole batch of simulated data was actual data. The entire dataset was uploaded and the project launched as planned.

We realised a day or two after launch that we weren’t telling volunteers when they had seen a simulation. This is important to know — especially if you think you found something really cool — and so we moved quickly to get the sims flagged as such after each classification. However, as many of you noticed, this fixed made it apparent that, in fact, 8/10 images were sims! Fixing the one mistake brought the other to the surface — and after a lot of searching we figured out what had happened.

Today we have done the following:

  1. We have paused 90% of the simulated data — so you won’t be asked to classify it now.
  2. We are aggressively retiring the simulations — so they’ll be removed 4x faster than the real data.
  3. ATLAS are preparing more data for Higgs Hunters — 10 times as much!
  4. Hopefully we can upload the new data before the end of 2014, and we’ll email participants to let them know.

After all of this, we now have ~8k subjects in Higgs Hunters and ~30% are sims — that means we’ll be done in ~100k classifications. So let’s call this Round One and see where it takes us. In the meantime, we thank everyone for their efforts on Higgs Hunters, and we apologise for all the confusion and frustration that this has caused some users.

We’re really sorry, and hope that this helps to explain some of the problems that have occurred and the ways in which we’re moving forward.

The Higgs boson Part 2: Discovery of the Higgs

On July 4th 2012, the ATLAS and CMS collaborations at the Large Hadron Collider (LHC) at CERN, Geneva, independently announced the discovery of a new particle with a mass over 130 times greater than a proton. This was in the range that had been predicted for the elusive Higgs boson, and it had been verified to extremely high certainty.

Experimental detection of the Higgs boson

Experimental detection of the Higgs boson

But what do we mean by ‘high certainty’? In Particle Physics everyone agrees on how sure you need to be to declare something as a discovery, and it’s quite stringent. Firstly, we assume that there is no new particle and calculate the probability that the signal we measure is consistent with there not being a particle there. If that probability is less than 0.32 than we say we are 1 sigma certain, 0.046 = 2 sigma (this is usually good enough for most science), 0.0027 = 3 sigma… We could stop at 3 sigma, as 0.27% chance of being wrong seems awfully small, but there have been a number of possible particle discoveries at 3 sigma level that later turned out just to be statistical anomalies. So just to be absolutely sure, the usual threshold to claim a discovery is 5 sigma (0.0000003 chance of observed signal being consistent with no new particle hypothesis).

Illustration of first 3 sigma levels

Illustration of first 3 sigma levels

Right, so we’re now pretty sure there is a new particle (that is a boson). But is it the Higgs boson?  Luckily, by March 2013, evidence surfaced that the new particle is what we call ‘spinless’ (meaning it looks the same from every direction) and that its interactions match the theoretical predictions of the famed Higgs boson. Further testing will take place from 2015 onwards, as the LHC ramps up towards its maximum energy of 14 TeV for the first time (double the energy it was running at in 2011 – more on particle energies in a future blog post).

(Next time: Exotic Higgs decays)

The Higgs boson Part 1: What is the Higgs?

The Standard Model is remarkably successful at explaining all the variety of particles we see in nature in terms of 16 fundamental particles. But there was one mystery yet remaining: why do some of those particles have mass but not others?

It seemed odd that photons and gluons (the force carriers of the electromagnetic and strong forces) were completely massless, and yet the W and Z particles (the force carriers of the weak force) weighed more than an entire atom of iron! It was clear that there had to be some kind of new mechanism that could give mass to some particles and none to others.

The solution came in 1964, when six physicists in three different groups (including Peter Higgs and François Englert, the 2012 noble prize winners) postulated that a field filling the entire universe, the Higgs field, is what gives fundamental particles their mass. The smoking gun signature of the existence of such a field would be a seventeenth fundamental particle: the Higgs boson.

Professor Peter Higgs Image credit: Claudia Marcelloni/ATLAS

Professor Peter Higgs
Image credit: Claudia Marcelloni/ATLAS

So how does it work? Imagine a field (the kind with grass and sheep) coated in snow. A skier passes by, gliding easily over the snow. Then a woman wearing snowshoes shuffles by, being slowed down by the snow. Next, a man in heavy boots struggles onwards, at each step being slowed by the snow. Finally, imagine a bird flying overhead, completely unaffected by the snow. In this analogy, the field of snow is the Higgs field and each character is a different fundamental particle. The bird is a massless particle like a photon, passing by without interacting with the field. The skier is a really light particle such as an electron, with very little mass at all. The woman in the snowshoes is a slightly heavier particle, such as a quark, and finally the man with the heavy boots is a truly massive particle like the W and Z particles, slowed by the Higgs field at every opportunity. So we see that the mass of a particle depends on how strongly it interacts with the Higgs field.

(Next time: Discovery of the Higgs)

Introduction to Particle Physics Part 4: Beyond the Standard Model

We know the Standard Model can’t be everything, as it only explains 3 of the fundamental forces of nature (the missing one being gravity). When we look out into the universe, we see that galaxies are spinning at the wrong speeds, that things that should be unstable are stable and that galactic clusters are bending light more than they should. This is strong evidence for a new form of matter that doesn’t interact with light – so called dark matter.

And if that isn’t crazy enough, the universe seems to be getting bigger at a faster rate (imagine throwing a ball in the air and it shooting upwards with ever increasing speed, totally counter intuitive). This is caused by something we call dark energy, which is a mysterious substance now believed to make up the vast majority of the energy content of our universe. As to what it actually is, we still don’t know.

Galaxy rotation curves - evidence for dark matter

Galaxy rotation curves – evidence for dark matter

So after all that hard work, it seems that the Standard Model only explains about 5% of the universe, oh well, it was nice trying. BUT WAIT! If there’s one thing Physicists are good at, it’s creating seemingly crazy ideas that just might turn out to be right…

One potential explanation of dark matter is that there is a whole new collection of super-heavy particles that we haven’t seen yet – the so called theory of supersymmetry. If we find evidence of such particles in particle colliders, it could even help us pave the way towards understanding if string theory is correct or not!

A Calabi-Yau manifold – welcome to the strange world of string theory

A Calabi-Yau manifold – welcome to the strange world of string theory

A recurring theme throughout our story was how things that once seemed disconnected are actually part of a deeper underlying truth, so it’s natural to wonder if one day we could unify all the fundamental forces into a single explanation – a theory of everything. The Large Hadron Collider may finally be the window to open our eyes to such new and exciting possibilities.

One thing is clear though: we stand on the precipice of perhaps the greatest change in our understanding of the universe – and the Higgs boson might just be the key to unlocking it all.

(Next time: What is the Higgs boson?)