thermonuclear reactions in the sun. no need for confinement! the enormous self-gravity of the sun...

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Thermonuclear Reactions in the Sun

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A ‘ Solar Model ’

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Page 1: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

Thermonuclear Reactions in the Sun

Page 2: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

No Need for Confinement!The enormous self-gravity of the sun

holds it together. There is no way the fuel can escape (or the sun can blow itself apart).

So the nuclear reactions just keep ‘ticking away’ in the hot central regions, slowly and steadily releasing the energy that keeps the sun in equilibrium.

Page 3: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

A ‘Solar Model’

Page 4: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

Turning Hydrogen into Helium

Atomic masses: Hydrogen 1, Helium 4

The Hydrogen nucleus is a proton

Helium contains two protons (positively charged) and two neutrons (uncharged)

Page 5: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

The Fundamental Effect 4 H He + energy

(from E = mc2)

Page 6: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

One Obvious ProblemHow can 4 protons (4 H) merge to produce a

Helium with 2 protons and 2 neutrons?

The masses add up pretty well – although a little bit vanishes -- but where do the extra positive charges go?

(Remember that charge is conserved – it cannot simply vanish!)

Page 7: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

A Second Problem

What are the chances of four protons running into each other all at the same time to form a Helium nucleus?

Answer: slim to none.

Page 8: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

A Frequent Occurence

Page 9: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

Much Less Frequent…

Page 10: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

Exploring The AnalogyTwo-car accidents are much more

common than multiple-car collisions.

So too with the atomic nuclei in the stars.

A proton has a good chance of running into another single proton, but not three at once!

Page 11: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

Instead: A Chain of Events

Page 12: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

Another Visualisation

Page 13: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

…and yet again: The Proton-proton (pp) Chain

Page 14: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

Important Things to NoteNet effect: 4 H 1 He + energy

(Note that only a fraction of the original mass is converted to energy via E = mc2. Less than 1% of it vanishes, with a big lump of He being left over.)

Positrons are created

Neutrinos are released (more on this later!)

Page 15: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

Meet The Positron:`Antimatter’

For every type of particle, there is an antiparticle.

When they meet, they annihilate completely and are converted to energy.

They have equal masses. If they are charged, they must have opposite charges (conservation law).

The positron (+) is the anti-electron (-).

Page 16: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

What Use Is a Positron?It can’t be contained: it will annihilate with

an electron the instant they meet. We can’t build vacuum chambers empty enough to prevent this happening quickly!

But we use them every day in hospitals, in PET scans (Positron Emission Tomography)

They meet electrons and create gamma rays.

Page 17: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

PET in DiagnosticsBut how do we get positrons into the body?

Page 18: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

Not Just From Nuclear Reactions!

Positrons are also emitted by some naturally radioactive isotopes. These can be included in organic molecules and ingested, then go to the tumour.

Page 19: Thermonuclear Reactions in the Sun. No Need for Confinement! The enormous self-gravity of the sun holds…

PET ScansRadioactive elementsproduce the positrons right where we needthem!