Where’s all the antimatter? New CERN results show the way.

If you look outside your window at the clouds, the stars, the planets, all that you will see is made of matter. However, when the universe was born, there were equal amounts of matter and antimatter. So where has all the antimatter gone?

The answer, if one is found, will be at the Large Hadron Collider (LHC), the world’s most powerful particle physics experiment, now taking a breather while engineers refit it to make it even more powerful by 2015. Then, it will be able to spot tinier, much more shortlived particles than the Higgs boson, which itself is notoriously shortlived.

While it ran from 2008 to early 2013, the LHC was incredibly prolific. It smashed together billions of protons in each experiment at speeds close to light’s, breaking them open. Physicists hoped the things that’d tumble out might show why the universe has come to prefer matter over antimatter.

In fact, from 2013 to 2015, physicists will be occupied gleaning meaningful results from each of these experiments because they simply didn’t have enough time to sift through all of them while the machine was running.

They will present their results as papers in scientific journals. Each paper will will be the product of analysis conducted on experimental data corresponding to some experiment, each with some energy, some luminosity, and other such experimental parameters central to experimental physics.

One such paper was submitted to a journal on April 23, 2013, titled ‘First observation of CP violation in the decays of B_s mesons‘. According to this paper, its corresponding experiment was conducted in 2011, when the LHC was smashing away at 7 TeV centre-of-mass (c.o.m) collision energy. This is the energy at the point inside the LHC circuit where two bunches of protons collide.

The paper also notes that the LHCb detector was used to track the results of the collision. The LHCb is one of seven detectors situated on the LHC’s ring. It has been engineered to study a particle known as the beauty quark, which is more than 4.2 times heavier than a proton, and lasts for about one-hundred-trillionth of a second before breaking down into lighter particles, a process mediated by some of nature’s four fundamental forces.

The beauty is one of six kinds of quarks, and together with other equally minuscule particles called bosons and leptons, they all make up everything in the universe: from entire galaxies to individual atoms.

For example, for as long as it lives, the beauty quark can team up with another quark or antiquark, the antimatter counterpart, to form particles called mesons. Generally, mesons are particles composed of one quark and one antiquark.

Why don’t the quark and antiquark meet and annihilate each other in a flash of energy? Because they’re not of the same type. If a quark of one type and an antiquark of another type meet, they don’t annihilate.

The B_s meson that the April 23 paper talks about is a meson composed of one beauty antiquark and one strange quark. Thus the notation ‘B_s’: A B-meson with an s component. This meson violates a law of the universe physicists long though unbreakable, called the charge-conjugation/parity (CP) invariance. It states that if you took a particle, inverted its charge (‘+’ to ‘-‘ or ‘-‘ to ‘+’), and then interchanged its left and right, its behaviour shouldn’t change in a universe that conserved charge and parity.

Physicists, however, found in the 2011 LHCb data that the B_s meson was flouting the CP invariance rule. Because of the beauty antiquark’s and strange quark’s short lifetimes, the B_s meson only lasted for so long before breaking down into lighter particles, in this case called kaons and pions.

When physicists calculated the kaons‘s and pions‘s charges and compared it to the B_s meson’s, they added up. However, when they calculated the kaons‘s and pions‘s left- and right-handednesses, i.e. parities, in terms of which direction they were spinning in, they found an imbalance.

A force, called the weak force, was pushing a particle to spin one way instead of the other about 27 per cent of the time. According to the physicists’ paper, this result has been reached with a confidence-level of more than 5-sigma. This means that some reading in the data would disagree with their conclusion not more than 0.00001 per cent of the time, sufficient to claim direct evidence.

Of course, this wouldn’t be the first time evidence of CP violation in B-mesons had been spotted. On 17 May, 2010B-mesons composed of a beauty antiquark and a down quark were shown shown to decay at a much slower rate than B-antimesons of the same composition, in the process outlasting them. However, this is the first time evidence of this violation has been found in B_s mesons, a particle that has been called “bizarre”.

While this flies in the face of a natural, intuitive understanding of our universe, it is a happy conclusion because it could explain the aberration that is antimatter’s absence, one that isn’t explained by a theory in physics called the Standard Model.

Here was something in the universe that was showing some sort of a preference, ready to break the symmetry and uniformity of laws that pervade the space-time continuum.

Physicists know that the weak force, one of the fundamental forces of nature like gravity is, is the culprit. It has a preference for acting on left-handed particles and right-handed antiparticles. When such a particle shows itself, the weak force offers to mediate its breakdown into lighter particles, in the process resulting in a preference for one set of products over another.

But in order to fully establish the link between matter’s domination and the weak force’s role in it, physicists have to first figure out why the weak force has such biased preferences.

This post originally appeared in The Copernican science blog at The Hindu on April 25, 2013.

The strong CP problem: We’re just lost

Unsolved problems in particle physics are just mind-boggling. They usually concern nature at either the smallest or the largest scales, and the smaller the particle whose properties you’re trying to decipher, the closer you are to nature’s most fundamental principles, principles that, in their multitudes, father civilisations, galaxies, and all other kinds of things.

One of the most intriguing such problems is called the ‘strong CP problem’. It has to do with the strong force, one of nature’s four fundamental forces, and what’s called the CP-violation phenomenon.

The strong force is responsible for most of the mass of the human body, most of the mass of the chair you’re sitting on, even most of the mass of our Sun and the moon.

Yes, the Higgs mechanism is the mass-giving mechanism, but it gives mass only to the fundamental particles, and if we were to be weighed by that alone, we’d weigh orders of magnitude lesser. More than 90 per cent of our mass actually comes from the strong nuclear force.

The relationship between the strong nuclear force and our mass is unclear (this isn’t the problem I’m talking about). It’s the force that holds together quarks, a brand of fundamental particles, to form protons and neutrons. As with all other forces in particle physics, its push-and-pull is understood in terms of a force-carrier particle – a messenger of the force’s will, as it were.

This messenger is called a gluon, and the behaviour of all gluons is governed by a set of laws that fall under the subject of quantum chromodynamics (QCD).


Dr. Murray Gell-Mann is an American scientist who contributed significantly to the development of theories of fundamental particles, including QCD

According to QCD, the farther two gluons get away from each other, the stronger the force between them will get. This is counterintuitive to those who’ve grown up working with Newton’s inverse-square laws, etc. An extension of this principle is that gluons can emit gluons, which is also counter-intuitive and sort of like the weird Banach-Tarski paradox.

Protons and neutrons belong to a category called hadrons, which are basically heavy particles that are made up of three quarks. When, instead, a quark and an antiquark are held together, another type of hadron called the meson comes into existence. You’d think the particle and its antiparticle would immediately annihilate each other. However, it doesn’t happen so quickly if the quark and antiquark are of different types (also called flavours).

One kind of meson is the kaon. A kaon comprises one strange quark (or antiquark) and one upantiquark (or quark). Among kaons, there are two kinds, K-short and K-long, whose properties were studied by Orreste Piccioni in 1964. They’re called so because K-long lasts longer than K-short before it decays into a shower of lighter particles, as shown:

Strange antiquark –> up antiquark + W-plus boson (1)

W-plus boson –> down antiquark + up quark

Up quark –> gluon + down quark + down antiquark (2)

The original other up quark remains as an up quark.

Whenever a decay results in the formation of a W-plus/W-minus/Z boson, the weak force is said to be involved. Whenever a gluon is seen mediating, the strong nuclear force is said to be involved.

In the decay shown above, there is one weak-decay (1) and one strong-decay (2). And whenever a weak-decay happens, a strange attitude of nature is revealed: bias.


Handed spin (the up-down arrows indicate the particle’s momentum)

The universe may not have a top or a bottom, but it definitely has a left and a right. At the smallest level, these directions are characterised by spinning particles. If a particle is spinning one way, then another particle with the same properties but spinning the other way is said to be the original’s mirror-image. This way, a right and a left orientation are chosen.

As a conglomeration of such spinning particles, some toward the right and some toward the left, comes together to birth stuff, the stuff will also acquire a handedness with respect to the rest of the universe.

And where the weak-decay is involved, left and right become swapped; parity gets violated.

Consider the K-long decay depicted above (1). Because of the energy conservation law, there must be a way to account for all the properties going into and coming out of the decay. This means if something went in left-handed, it must come out left-handed, too. However, the strange antiquark emerges as anup antiquark with its spin mirrored.


Physicists Tsung-Dao Lee and Chen Ning Yang (Image from the University of Chicago archive)

As Chen Nin Yang and Tsung-Dao Lee investigated in the 1950s, they found that the weak-decay results in particles whose summed up properties were exactly the same as that of the decaying particle, but in a universe in which left and right had been swapped! In addition, the weak-decay also forced any intervening quarks to change their flavour.


In the Feynman diagram shown above, a neutron decays into a proton because a down quark is turned into an up quark (The mediating W-minus decays into an electron and an electron antineutrino).

This is curious behaviour, especially for a force that is considered fundamental, an innate attribute of nature itself. Whatever happened to symmetry, why couldn’t nature maintain the order of things without putting in a twist? Sure, we’re now able to explain how the weak-interaction swaps orientations, but there’s no clue about why it has to happen like that. I mean… why?!

And now, we come to the strong CP problem(!): The laws governing the weak-interaction, brought under electroweak theory (EWT), are very, very similar to QCD. Why then doesn’t the strong nuclear force violate parity?

This is also fascinating because of the similarities it bears to nature’s increasing degree of prejudices. Why an asymmetric force like the weak-interaction was born in an otherwise symmetric universe, no one knows, and why only the weak-interaction gets to violate parity, no one knows. Pfft.

More so, even on the road leading up to this problem, we chanced upon three other problems, and altogether, this provides a good idea of how much humans are lost when it comes to particle physics. It’s evident that we’re only playing catching up, building simulations and then comparing the results to real-life occurrences to prove ourselves right. And just when you ask “Why?”, we’re lost for words.

Even the Large Hadron Collider (LHC), a multi-billion dollar particle sledgehammer in France-Switzerland, is mostly a “How” machine. It smashes together billions of particles and then, using seven detectors positioned along its length, analyses the debris spewn out.


An indicative diagram of the layout of detectors on the LHC

Incidentally, one of the detectors, the LHCb, sifts through the particulate mess to find out how really the weak-interaction affects particle-decay. Specifically, it studies the properties of the B-meson, a kind of meson that has a bottom quark/antiquark (b-quark) as one of its two constituents.

The b-quark has a tendency to weak-decay into its antiparticle, the b*-quark, in the process getting its left and right switched. Moreover, it has been observed the b*-quark is more likely to decay into the b-quark than it is for the b-quark to decay into the b*-quark. This phenomenon, involved in a process called baryogenesis, was responsible for today’s universe being composed of matter and not antimatter, and the LHCb is tasked with finding out… well, why?

(This blog post first appeared at The Copernican on December 14, 2012.)