The evolving Universe
The evolving Universe

Start this free course now. Just create an account and sign in. Enrol and complete the course for a free statement of participation or digital badge if available.

Free course

The evolving Universe

1.5 The quark-lepton era

Time: l0−11s to 10−5s

Temperature: 3 × 1015 K to 3 × 1012 K

Energy: 1000 GeV to 1 GeV

During the time interval 10−32 s to 10−11 s, i.e. for the 10−11 seconds or so after inflation, nothing new happened in the Universe! It merely carried on expanding and cooling, but no new processes took place. The desert (as it is known) - came to an end when the Universe reached a temperature of about 3 × 1015 K, and this is where the next stage in our history begins. At this point the mean energy per particle was around 1000 GeV and the electromagnetic and weak interactions became distinct (Figure 1). The energies corresponding to this transition are becoming attainable in experiments here on Earth. So it could be argued that all particle reactions that models propose after the first 10−11 s of the history of the Universe are directly testable in Earth-based laboratories.

By 10−11 s after the Big Bang, the X bosons had long since decayed in reactions like those shown in Equation 2, but the temperature of the Universe was still too high for the familiar baryons (protons and neutrons) to be stable. The Universe contained all types of leptons, quarks, antileptons, and antiquarks as well as photons. In fact, there would have been approximately equal numbers of particles and antiparticles at this time — but note that word approximately — we shall return to the implications of this in a moment. There would also have been equal amounts of radiation (photons) and matter/antimatter (particles or antiparticles).

Now is a good time to go over some of the basics about the fundamental particles from which the Universe is built.

Question 5

How do the properties of one generation of particles differ from those of each other generation?

Answer

The third-generation quarks (t and b) are more massive than the second-generation quarks (c and s), which in turn are more massive than the first-generation quarks (u and d). Only upper limits to the masses of neutrinos are known, but tauons are more massive than muons, which in turn are more massive than electrons.

Question 6

Which particles participate in strong interactions, weak interactions and electromagnetic interactions, respectively?

Answer

Only quarks take part in strong interactions. All quarks and leptons participate in weak interactions. All electrically charged particles experience electromagnetic interactions.

Question 7

How do the charge and mass of antimatter particles differ from those of the corresponding matter particles?

Answer

Antimatter particles have the opposite electric charge, but the same mass, as their matter counterparts. Antimatter quarks also have the opposite colour charge to matter quarks.

Let's now consider what the net electric charge of the Universe would have been at this time. When quarks and leptons are spontaneously produced from energy, they appear as matter-antimatter pairs with equal and opposite charge. So the net charge of the Universe remains zero, however many quarks, antiquarks, leptons and antileptons are produced in this way. But there is another way of producing leptons and quarks, namely by the decay of X bosons (Equation 2). The decays of X bosons produce:

  • three quarks for every one lepton (and three antiquarks for every antilepton);

  • quarks with charge +2/3 unit as often as quarks with charge −1/3 unit;

  • charged leptons as often as uncharged leptons.

So, a few X bosons might decay to produce three up quarks, three down quarks, one electron and one electron neutrino, in accord with these rules.

Question 7.1

What is the total electric charge of: three up quarks, three down quarks, one electron and one electron neutrino?

Answer

The electric charge of a single up quark is +2/3 unit, of a single down quark is −1/3 unit, of a single electron is −1 unit, and of a single electron neutrino is 0 units. So the total electric charge of this collection of particles is .

An X boson decay rate with a three to one balance between quarks and leptons therefore ensured that the net charge of the Universe remained zero.

S197_1

Take your learning further

Making the decision to study can be a big step, which is why you'll want a trusted University. The Open University has 50 years’ experience delivering flexible learning and 170,000 students are studying with us right now. Take a look at all Open University courses.

If you are new to university level study, find out more about the types of qualifications we offer, including our entry level Access courses and Certificates.

Not ready for University study then browse over 900 free courses on OpenLearn and sign up to our newsletter to hear about new free courses as they are released.

Every year, thousands of students decide to study with The Open University. With over 120 qualifications, we’ve got the right course for you.

Request an Open University prospectus