1. Creation the Element Carbon for BI105 or how the elemental composition of the Universe got to be By Dr. Harold Williams of Montgomery College Planetarium http://montgomerycollege.edu/Departments/planet/

2. Some Physics First There are four fundamental forces in the universe 1GRAVITY 2ELECTROMAGNETISM 3WEAK NUCLEAR FORCE 4STRONG NUCLEAR FORCE

3. Gravity Gravity which is the weakest and acts on all mass and energy It acts on everything and is always attractive, it sucks never pushes always pulls things together. The largest structures from mountains to planets to stars to galaxies to clusters of galaxies to super clusters of galaxies are formed by gravity. Gravitational forces fall off inversely proportional to the distance squared. Gravitational forces are proportional to mass energy.

4. Gravity It has not been made into a good quantum theory yet. Newton’s Universal theory of gravity works well, but has been superseded by the General Theory of Relativity. General Relativity is the theory of gravity discovered or invented by Albert Einstein in 1915. Its details are much more complicated than electromagnetism.

5. Electromagnetism Electromagnetism is much stronger than gravity, but only effects charges. Benjamin Franklin discovered that like charges, q, repel each other and unlike charges attract. This is the most important fact of electromagnetism. When charges accelerate or decelerate photons are emitted or absorbed. Photons can be radio waves, TV waves, microwaves, infrared, visible light, ultraviolet, x-rays, or gamma rays. The only difference is frequency of the wave and energy per photon.

6. All Photons travel at the speed of light, c! The speed of light is finite and it is the fastest speed in the universe. Therefore the speed of light is the same relative to all reference frames. Space and time are different; just as where and when are different, but they are intimately linked. Different observers will not agree on lengths of objects and time intervals between events. Simultaneity is very tricky!

7. Electromagnetism Charges create electrical fields, E Moving charges, q, traveling at velocity, v, create a magnetic field, B, and moving charges are effected by magnetic fields. Magnetism is weaker than Electric and is caused by the finite nature of the speed of light. The speed of light has to be finite or we would not live in a causal universe. There would be not cause and effect!!!!!

8. Electromagnetism Causes chemistry, holds negatively charged electrons, e -, around around positively charged nuclei. Positively charge nuclei contains protons, p +. Atoms, molecules, material strength, and you are held together by electrical forces. Electrical forces fall off inversely proportional to the distance squared.

9. Weak Nuclear Force Very short range, not long range like gravity and electromagnetism. Causes nuclear decay, a neutrino, is emitted. This causes the core of the earth to be hot and only up and down quarks to be stable.

10. Strong Nuclear Force Also a short range force, not long range like gravity and electromagenistm. It is a much stronger force and its range while short is longer than the weak nuclear force. It hold protons and neutrons together in the nucleus of an atom. It operates over nuclear distances.

11. Four known forces in universe: Strong Force Electromagnetism Weak Force Gravity

12. Four known forces in universe: Strong Force Electromagnetism Weak Force Gravity Do forces unify at high temperatures?

13. Four known forces in universe: Strong Force Electromagnetism Weak Force Gravity Do forces unify at high temperatures? Yes! (Electroweak)

14. Four known forces in universe: Strong Force Electromagnetism Weak Force Gravity Do forces unify at high temperatures? Yes! (Electroweak) Maybe (GUT)

15. Four known forces in universe: Strong Force Electromagnetism Weak Force Gravity Do forces unify at high temperatures? Yes! (Electroweak) Maybe (GUT) Who knows? (String Theory)

16. What is the history of the universe according to the Big Bang theory?

18. Planck Era Before Planck time (~10 -43 sec) No theory of quantum gravity, yet!

19. GUT Era Lasts from Planck time (~10 -43 sec) to end of GUT force (~10 -38 sec)

20. Electroweak Era Lasts from end of GUT force (~10 -38 sec) to end of electroweak force (~10 -10 sec)

21. Particle Era Amounts of matter and antimatter nearly equal (Roughly 1 extra proton for every 10 9 proton- antiproton pairs!)

22. Era of Nucleo- synthesis Begins when matter annihilates remaining antimatter at ~ 0.001 sec Nuclei begin to fuse

23. Era of Nuclei Helium nuclei form at age ~ 3 minutes Universe has become too cool to blast helium apart

24. Protons and neutrons combined to make long-lasting helium nuclei when universe was ~ 3 minutes old

25. Big Bang theory prediction: 75% H, 25% He (by mass) Matches observations of nearly primordial gases

26. Abundances of other light elements agree with Big Bang model having 4.4% normal matter – more evidence for WIMPS!

27. Era of Atoms Atoms form at age ~ 380,000 years Background radiation released

28. The cosmic microwave background – the radiation left over from the Big Bang – was detected by Penzias & Wilson in 1965

29. Background radiation from Big Bang has been freely streaming across universe since atoms formed at temperature ~ 3,000 K: visible/IR

30. Expansion of universe has redshifted thermal radiation from that time to ~1000 times longer wavelength: microwaves Background has perfect thermal radiation spectrum at temperature 2.73 K

31. Around 380,000 years after the Beginning of Time

32. Era of Galaxies Galaxies form at age ~ 1 billion years Star form earlier ending the dark ages ~200 million years.

33. So after the Big Bang the Universe is Composed Of 75% by weight Hydrogen, 1 H 25% by weight Helium, 4 He A small amount of Deuterium, 2 H An even smaller amount of Lithium and Beryllium, Li and Be and some 3 He. No Carbon, C, no Nitrogen, N, no Oxygen, O, no heavy elements like Iron, Fe, or Magnesium, Mg, Sulfur, S, or Potassium, K, or Phosphorus, P.

34. Elemental Composition of the Universe the song lyrics by Harold and Barbara Williams Twinkle, Twinkle, little star. Yes I know just what you are. You’re three quarters hydrogen, and one quarter helium with trace amounts of other things from pink sea shells, to diamond rings.

35. How do high-mass stars make the elements necessary for life? http://en.wikipedia.org/wiki/Triple-alpha_process http://en.wikipedia.org/wiki/Neon_burning_process http://en.wikipedia.org/wiki/Silicon_burning_process

36. CNO Cycle http://en.wikipedia.org/wiki/CNO_cycle http://en.wikipedia.org/wiki/CNO_cycle High-mass main sequence stars fuse H to He at a higher rate using carbon, nitrogen, and oxygen as catalysts Greater core temperature enables H nuclei to overcome greater repulsion

37. Big Bang made 75% H, 25% He – stars make everything else

38. Helium fusion can make carbon in low-mass stars

39. CNO cycle can change C into N and O

40. Helium Capture High core temperatures allow helium to fuse with heavier elements

41. Helium capture builds C into O, Ne, Mg, …

42. Advanced Nuclear Burning Core temperatures in stars with >8M Sun allow fusion of elements as heavy as iron

43. Advanced reactions in stars make elements like Si, S, Ca, Fe

44. Multiple Shell Burning Advanced nuclear burning proceeds in a series of nested shells

45. Iron is dead end for fusion because nuclear reactions involving iron do not release energy (Fe has lowest mass per nuclear particle)

46. Evidence for helium capture: Higher abundances of elements with even numbers of protons

47. Iron builds up in core until degeneracy pressure can no longer resist gravity Core then suddenly collapses, creating supernova explosion

48. How does a high-mass star die?

49. Supernova Explosion http://en.wikipedia.org/wiki/Supernova http://en.wikipedia.org/wiki/Supernova Core degeneracy pressure goes away because electrons combine with protons, making neutrons and neutrinos Neutrons collapse to the center, forming a neutron star http://en.wikipedia.org/wiki /Neutron_starhttp://en.wikipedia.org/wiki /Neutron_star

50. Energy and neutrons released in supernova explosion enable elements heavier than iron to form, including Au and U

51. Supernova Remnant http://en.wikipedia.org/wiki/Crab_nebula http://en.wikipedia.org/wiki/Crab_nebula Energy released by collapse of core drives outer layers into space The Crab Nebula is the remnant of the supernova seen in A.D. 1054, M1, NGC 1952, Taurus A, ~6,300LY away, 3LY radius, optical and radio pulsar

52. Supernova 1987A http://en.wikipedia.org/wiki/Supernova_1987a http://en.wikipedia.org/wiki/Supernova_1987a The closest supernova in the last four centuries was seen in 1987

53. Rings around Supernova 1987A The supernova’s flash of light caused rings of gas around the supernova to glow

54. Impact of Debris with Rings More recent observations are showing the inner ring light up as debris crashes into it