Breaking

Symmetries

Each of the four fundamental forces is characterised by a set of symmetry transformations. A symmetry is a change that you can make under which something remains the same. So, for example, a “reflection” is a transformation, under which left and right are swapped over:

Reflection

A reflection [Attribution]

A rectangle has two reflection symmetries:

Another example of a transformation is a rotation. This could, for example, be a rotation in two dimensions. A two-dimensional object can be rotated through any number of degrees: 20º, 59º or even 241.799868º. This kind of transformation is called a continuous symmetry, while a reflection is an example of a discrete symmetry – there is no halfway house between making a transformation and not making one; you can’t “reduce” the “amount” of a reflection.

Triangles are symmetric only under rotations which are multiples of 120º:

while circles are symmetric under any rotation in two dimensions.

These symmetry transformations can be combined by carrying out one after another. Combining symmetries in this way allows one to construct “groups” of symmetry transformations. The study of these groups of symmetries is called group theory. Again, there is a host of information available on group theory. If you are wanting to explore group theory for the first time, I’d highly recommend Teach Yourself Mathematical Groups by Tony Barnard and Hugh Neill, in the Hodder & Stoughton Teach Yourself series.

Rotations can obviously be defined in three dimensions as well. A sphere is perfectly symmetric under three-dimensional rotations. Rotations can equally be defined in higher numbers of dimensions. As mentioned on the page “warping”, changes of reference frame in special relativity can be described as rotations in four-dimensional spacetime.

Typically, in fundamental physics, the symmetry will preserve the field equations.

The field equations of general relativity are preserved by changes of the coordinates used on the spacetime. These changes of coordinates induce transformations on the tangent spaces. The symmetries of tangent spaces are much simpler than those of the underlying curved space. If we exclude discrete symmetries such as reflections, they essentially fall into two categories: those which preserve the lengths of lines and the angles between them – i.e. rotations – and those which don’t.

My analysis of these symmetries can be found in the following notes:

Tangent space symmetries »

Complex numbers

The symmetries characterising the other three interactions are based on a type of number called a complex number. In this subsection, we explain what these are – skip it if you’re already familiar with these. If you’re not, and you want more detail than I’m giving here, a simple internet search should give you a much fuller description of them.

Any number n can be multiplied itself to create its square, n². For example, 3² = 3 x 3 = 9. This is an example of an operation known as a map; it “maps” the number 3 to the number 9. This map can be inverted, to take us from 9 back to 3. This inverse is known as the square root. The square root of any number n is denoted √n or n½. For example, 9½ = 3 and 25½ = 5.

Negative numbers can also be squared, for example (-4)² = -4 x -4 = 16 and (-1)² = -1 x -1 = 1. Positive and negative numbers, such as those in these examples, are called real numbers.

Any positive number has two square roots, both of which are real numbers. One is positive and the other is negative. That is, for any positive number x it is always possible to find a positive number y that has the property y² = x; corresponding to y, there is then a negative number –y which also squares to x: (-y)² = x.

However, the square root of a negative number is not a real number. There is no positive or negative number, for example, which squares to -4. What mathematicians (and physicists) do at this point is to invent a new kind of number, called an imaginary number. They use the letter i to denote the “imaginary” square root of -1, that is, i x i = -1. This number can be multiplied by a real number to create another imaginary number, such as 4i = 4 x i. Any such imaginary number will square to a negative number: (4i)² = 4 x i x 4 x i = 4 x 4 x i x i = 16 x -1 = -16. Conversely, the square root of any negative number is an imaginary number: (-9)½ = 3i. A real number can then be added to an imaginary number to create a complex number, such as 4 + 3i. Perhaps surprisingly, the normal rules of arithmetic can be extended very simply to cover imaginary numbers.

Now this is all just number theory so far (although certainly interesting in its own right). But it turns out that complex numbers are extremely useful in mathematics and physics. They are very helpful in describing wave motion, for example. And they are also very helpful in describing what physicists call “fermionic matter”: matter-like particles, such as electrons, the quarks which are fundamental components of protons and neutrons, and indeed protons and neutrons themselves.

Internal symmetries

Subatomic particles can often be classified into sets where every member of a set is identical apart from one label – for example, you could have a pair of particles which are identical apart from the fact one has a positive electric charge and the other has a negative electric charge. Thus if the equations governing the motion of a set of charged particles don’t change if positively charged particles are substituted for identical negatively charged ones, and vice versa, those equations can be said to be symmetric under a change of charge.

The symmetry groups underlying the electromagnetic, strong and weak interactions relate to these kinds of particle identities. These groups have a similar structure to groups of rotations. In fact, they can be described as rotations of complex vectors – vectors which are characterised by complex numbers. For example, the strong interaction is based on a symmetry group called SU(3). This group describes rotations of a three-dimensional complex vector, that is, a vector in a three-dimensional space where each of the coordinates is a complex number. (Note that we don’t need to know whether this rather peculiar space has any physical meaning in order to carry out physics calculations. That is certainly an interesting question, but it’s enough to know that the mathematics works to do most particle physics calculations.)

Sometimes, the groups of rotations in complex spaces have exactly the same structure as groups of rotations in real spaces. For example, any rotation in two complex dimensions corresponds to two different rotations in three real dimensions. This correspondence holds when rotations are combined: if we combine two rotations, A and B, in the complex space, we get a complex rotation which corresponds to a rotation C in the real space; combining the rotations corresponding to A and B in the real space results in the same rotation C.

There is a similar correspondence between rotations in a four-dimensional complex space and those in a six-dimensional real space. This is analysed in a paper I co-wrote with Ken Barnes and Jason Hamilton-Charlton:

How orbits of SU(N) can describe rotations in SO(6) »

Ken tom

Me with Ken Barnes on the day of my PhD graduation [Attribution]

Unification

The ultimate goal of physicists investigating the four interactions is to develop a single theory which describes all of them, ideally with a single Lagrangian. It is unclear what type of theory this would be; it could be a geometric theory, a quantum field theory as most physicists seem to think, or something else completely. (A quantum field theory is a theory which is consistent with both quantum mechanics and special relativity, in which fundamental particles are described as excitations of a field.) However, it’s pretty clear that a key feature of the theory would be its symmetries.

Over the course of the 20th century, there was considerable progress in unifying the forces in this way.

In the 1960s, a theory was proposed by Abdus Salam and Steven Weinberg for unifying the electromagnetic and weak interactions. This theory predicted the existence of a number of new particles, including the famous Higgs particle, which have since been discovered.

Salam and Weinberg’s theory was later extended to incorporate the strong nuclear force, although it turned out there was no unique way to do this.

The “electroweak theory” is based on the concept of symmetry breaking.

Symmetry breaking

This concept is best described by way of an analogy. Imagine taking a sombrero – yes, a Mexican hat – and putting it on the floor in front of you. Then take a marble and balance the marble on the point of the hat:

If you look down from above, the view will have perfect rotational symmetry – it won’t matter how you rotate the view, it will look the same:

Now let go of the marble. It will roll down the side of the hat into the rim:

The view will no longer have perfect rotational symmetry – the marble will mark out a particular direction:

The starting point of the marble represents a position of high potential energy. When the marble is released, this potential energy is converted into kinetic energy and the ball rolls down the side of the hat. The equations of motion which govern the way it moves are perfectly symmetric – they do not change under a rotation. However, when the marble finally comes to rest, the symmetry has been broken; this is a state of minimum energy.

This is exactly what happens in Salam and Weinberg’s theory. In fact, there is a potential energy term in the Lagrangian called a “Mexican Hat” potential. It’s called this because if you plot the way the potential energy varies with the values of the Higgs fields, the shape you get is, roughly speaking, the shape of a sombrero. In this theory, the interactions between the fields in a high-energy state are associated with a set of symmetries. The equations of motion are preserved under all of these symmetries. When the system is allowed to settle down into a low energy state, all but one of these symmetries are broken. (The Higgs fields are a set of scalar fields which have the original full symmetry.)

The symmetry which remains at low energies is the one associated with electromagnetism. The broken symmetries are associated with the weak interaction. This gives the weak interaction some very strange properties. It is mediated by particles with very large masses, known as W and Z particles. These high masses meant that they weren’t observed until 1983, when they were created in a particle accelerator. Until then, only their effects on other matter had been observed, in which they change particle identities and are responsible for nuclear beta decay and a particular type of supernova.

It’s also possible to use an analogy to demonstrate this idea of some of the symmetries being broken, while others remain unbroken at low energies. Imagine a transparent hollow sphere, with a bead at the very centre:

This system has perfect rotational symmetry in three dimensions. Imagine there is a force which attracts the bead to the surface of the sphere, which grows in strength the closer the bead gets to the surface. Once the bead is released, it will start to move towards the sphere’s surface, increasing in pace until it hits the surface, where it comes to rest:

This marks out a “preferred direction”. We can choose an axis which runs through the bead and the centre of the sphere:

Rotating the sphere about this axis leaves it unchanged:

But rotating through any other axis will change the view. Thus we have broken the symmetry. The equations describing the system have three-dimensional rotational symmetry, as described above. However, the final state is only symmetric under rotations about one particular axis, that is, a group of rotations in two dimensions. All the other symmetries have been broken.

I have written notes on this particular symmetry breaking scheme and how it applies to field theory:

Non-linearly realised O(3) symmetries »

Spontaneous compactification

The only interactions in Kaluza and Klein’s theory (see page “Warping”) were gravity and electromagnetism. The symmetries of the theory were the symmetries of those interactions. Over the following decades there were a handful of papers looking at extending these ideas to include other symmetry groups. This required more than one additional dimension. These extra dimensions would be “compact”, that is, “rolled up” in some way.

However, one of the greatest shortcomings of all of these papers was that there was no explanation of why the extra dimensions should be compact. A possible explanation was provided with the concept of “spontaneous compactification” in the late 1970s and early 1980s. The basic idea was that symmetry breaking could cause the extra dimensions to become compact.

The first papers achieved this by making use of a set of scalar fields with a “Mexican hat” potential or similar. These are essentially Higgs fields which don’t just cause symmetry breaking but also cause the additional dimensions to become compact.

Some later papers avoided using scalar fields. In these later papers, there was a field associated with the non-gravitational interactions, such as the electromagnetic field or the “gluon” field of the strong interaction, included in the Lagrangian. This field acted as a matter distribution and caused the higher-dimensional spacetime to curve. It curved in such a way as to leave the additional dimensions compactified. It was then shown that in some cases, these new theories were equivalent to the ones with scalar fields.

But with either type of spontaneous compactification, the additional fields do not have the full symmetries of the higher-dimensional spacetime.

In recent years, this has been the focus of my research. I have developed a theory which resolves this problem:

Fully covariant spontaneous compactification »

The starting point for this theory was that every set of fields in the Lagrangian and every term in it should have the full symmetries of the higher-dimensional spacetime. The field equations governing curvature should have no symmetries other than those of the vector spaces of the higher-dimensional spacetime. There would then be a symmetry-breaking process which would break these symmetries and cause the extra dimensions to compactify. The unbroken symmetries – those of the resulting spacetime – would include those underlying general relativity.

What I have found is that rather than using a set of scalar Higgs fields, the Lagrangian needs to include a vector field. The symmetry can be broken by including an appropriate potential in the Lagrangian, similar to the Mexican hat potential. Alternatively, it can be broken by “imposing a constraint” on the system – essentially, by saying that the solution of the field equations we are looking for must have particular properties. (Note for researchers in this area: the symmetry-breaking potential or constraints are actually built out of the covariant derivative of the vector field.) I explain in the paper how to calculate these constraints and, if desired, construct the potential.

Imposing the constraints or applying the potential leads to the symmetries of the tangent spaces breaking and the tangent spaces themselves separating. For example, if one starts with a six-dimensional spacetime, it is possible to choose constraints or a potential that breaks the tangent space into a four-dimensional one and a two-dimensional one. The metric splits, or “decomposes”, into separate metrics for the four-dimensional and two-dimensional tangent spaces. Similarly, vector fields then split into four-dimensional vector fields and two-dimensional ones.

This is a sign that the underlying spacetime has become curved. You can get some information about the overall shape of the spacetime from this (known as its “topology”), but to find the exact curvature at any given point, you need field equations. I derived field equations from Poisson’s equation. I wanted field equations which were equally valid in any coordinate system. I also wanted them to be consistent with the key idea in general relativity, that an object’s gravitational acceleration is caused by its motion around a curved spacetime. I found the simplest possible extension of Poisson’s equation consistent with these two principles. This field equation is not that of general relativity, but it can be brought into a similar form.

I was able to show that there are solutions of these equations, satisfying particular constraints, in which four-dimensional spacetime is flat, while the extra dimensions roll up into a separate space with constant curvature. This would represent the situation in deep space – far away from any normal gravitational fields, such as those of stars or galaxies, and far away from any charged matter. For example, with six dimensions, the extra two dimensions have the same shape as the surface of a sphere.

Now the curvature of such as space can be expressed in a single value, known as the Ricci scalar. In my theory, this depends on the density of the vector field used in the potential or constraints. For the extra dimensions to be curled up so tightly that they become subatomic, this field has to have staggeringly high density. For example, if the dimensions have the same size as in the original theory of Klein, the density has to be around 1095 kg m-3. That means that every cubic metre of space is filled with 1095 kg (that’s a 1 followed by 95 zeros) of this stuff.

This means that in this theory, the densest “matter” in the universe – by a long, long way – is something we can’t even see. We can’t see it, because all it does is generate curvature, causing extra dimensions to wrap up small. When you think about it, this makes sense. Something with the density of our sun causes light to bend round it very slightly and planets to move around it in orbits millions of miles across. This is clearly only very mild curvature. In order to cause such huge curvature for dimensions to wrap up to subatomic scales, it’s not surprising that the density would have to be so humungous.

One thing I have noticed with this model is that it is a bit too simplistic to say “symmetry is broken at low energies”. Firstly, even if one uses a potential to break the symmetry, (as opposed to breaking it using constraints), this potential is constructed out of the very high density field. The lower the density, the less the curvature. In the absence of any mass at all, the symmetries are not broken. Secondly, energy is a more complicated concept in relativity. It is no longer a scalar quantity, but forms a four-dimensional vector together with momentum. Energy density is more complicated again, due to lengths – and therefore volumes – contracting at high relative velocities. Furthermore, the energy of the gravitational field cannot be defined in an unambiguous way in general relativity, although it can be in TEGR.

I have shown that in the most general coordinate system, extra fields appear in the connection. Just like the inertial force felt within the accelerating spaceship mentioned above, they are the result of choosing a particular frame of reference. However, there is a strong suggestion that if other matter was included in the system, these “fictitious forces” would be replaced by real fundamental interactions:

  • Curvature in the familiar four-dimensional spacetime, in other words, the force of gravity we’re familiar with;
  • Curvature in the extra dimensions, which would make small changes to the rolled-up shape of these dimensions (for example, making a ball lumpy);
  • Fields mediating non-gravitational interactions, known to physicists as “gauge fields” or “Yang-Mills fields” (the electromagnetic field is an example of a gauge field);
  • New fields with rather strange properties – they carry changes of particle labels, such as “spin” and various charges, meaning that they could effectively turn a scalar field into a vector field or vice versa.

These all represent departures from the situation in which only the very high density field is present. With just the high density vector field, any object travelling in our familiar four-dimensional spacetime travels in a straight line purely in that spacetime. Similarly, a path in the extra compact dimensions stays in those dimensions. But when there is other matter in the system – when masses and charges are present, it appears that other paths may be possible. Our four-dimensional spacetime becomes slightly warped, just as in general relativity. The curvature of extra compact dimensions also changes slightly. Furthermore, there may be paths which don’t stay entirely within these subspaces.

So when you see a science fiction film in which adventurers travel into other dimensions, consider this: every particle we are made of, every electron, proton and neutron, may be an interdimensional traveller. Every non-gravitational interaction may represent spacetime curving in such a way as to allow paths into additional dimensions.


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