M8 Flashcards
What were the two competing theories for the origins of the universe?
Big Bang and Steady state
What was the Big Bang theory?
George Gamow suggested that if the universe was expanding then at some point, it must have occupied a very small place from which the universe expanded and cooled.
i.e. the universe originated from a single point.
What was the steady state theory?
Fred Hoyle suggested that the universe is:
Infinite — the ‘outer’ stars would never reach infinity and so could go on moving away from us forever.
Expanding — Matter is being created all the time at just the right rate to keep the density of the universe constant.
What was the key piece of evidence for the Big Bang theory?
Physicists from Princeton in the 1960s theorised that if the big bang theory were true, then that small condensed spot from which everything expanded, must have been very hot. Any hot object would have created large amounts of electromagnetic radiation. As the universe expanded, the wavelength of this radiation must have also. Over time, it should have also then cooled. Calculations revealed that the wavelength would have stretched to around a millimetre and cooled to a few degrees warmer than absolute zero. Two other scientists discovered that the radiation was close to the expected wavelength and corresponded to heat radiation at 2.7K. The radiation was called “cosmic microwave background”. Whilst the CMB radiation was quite uniform from all directions, it wasn’t perfectly uniform and this is evident in small variations in temperature created by this CMB. This is key as it meant that the early universe was not fully uniform, The small variations meant that matter was slightly clumped together in some places and so its unbalanced gravity could gradually pull it together to form the stars and, on a larger scale, galaxies.
Describe the lifecycle of a star of mass < 8 solar masses
- Protostar (gravity -> accretion of matter until thermal equilibrium)
- Main sequence (fuses hydrogen in core to form helium nuclei)
- Red Giant (fuses helium to carbon in SHELL when h fuel depletes)
- Death - Planetary nebula (clouds of gas that are blown away outer layers of a star)
- White dwarf left behind after nebula (dense stars do not fuse)
Describe the lifecycle of a star of mass 8-20 solar masses
- Protostar (gravity -> accretion of matter until thermal equilibrium)
- Main sequence (fuses hydrogen in core to form helium nuclei)
- Red Giant (fuses helium to carbon in SHELL when h fuel depletes)
- Death - Supernova (violent explosions of uncontrolled nuclear reactions)
- Neutron star - remnants of core after the supernova, electrons and protons forced together to form a sea of neutrons, densest objects, possess intense B fields which emit an intense beam of radio waves.
Describe the lifecycle of a star of mass > 20 solar masses
- Protostar (gravity -> accretion of matter until thermal equilibrium)
- Main sequence (fuses hydrogen in core to form helium nuclei)
- Red Giant (fuses helium to carbon in SHELL when h fuel depletes)
- Death - Supernova (violent explosions of uncontrolled nuclear reactions)
- Black holes - crushed remnants of core after supernova
What are the similarities between CNO and PP reactions in main sequence stars?
Both fuse hydrogen to helium and have the same overall net reaction
Both have a mass defect, indicating energy is released at the completion of the cycles.
What are the differences between CNO and PP reactions in main sequence stars?
CNO is a catalytic cycle while PP is a linear process,
CNO requires the presence of carbon as a catalyst and high temperatures (dominates when T > 1.8 x 10^7 K) & PP dominates in smaller stars with temperature < 1.8 x 10^7 K
Thomson’s charge to mass experiment
The setup consisted of a highly evacuated cathode ray tube, with a pair of charged parallel plates (e-field) and Helmholtz coils (B-field) outside the tube.
The electric and magnetic fields were orientated at right angles to each other such that they exerted opposing vertical forces on the beam of electrons
The experiment was then done in 2 stages:
Balancing E-Field and B-field:
Using the electric and magnetic fields simultaneously, he adjusted the strength of both until the electron beam passed through both fields undeflected. This showed that both fields cancelled each other out, i.e. v = E/B
B-Field only:
At this stage, the Efield was turned off and the beam of electrons was deflected under the influence of the magnetic field ONLY
Causing the beam to undergo circular motion, allowing for the radius of curvature to be measured
FB=FC
qvB=mv2/r
q/m=E/vB^2 (sub v = E/B)
As Thompson, knew the value for E, B and radius, he found the charge-to-mass ratio to be: q/m=1.761011C/kg
Milikan’s oil drop experiment
Millikan devised the following experiment where a spray of oil drops was introduced from above, into an electric field created by two charged parallel plates.
At certain electric field strengths, the oil drop would become suspended between the charged parallel plates. This indicated that the oil drop must be charged (to experience a force in the E-field)
The force by E-Field must balance the weight force i.e. qE=mg. Some of these drops would be charged by either; friction with the atomiser gun or friction with the air. He varied the field and found ultimately, the more charged the oil drop was, the weaker the electric field needed to be, to balance the weight force F=Eq, so increased q meant decreased E-field. Milikan then introduced X-rays to the chamber to cause more ionisation of the oil drops, In altering the E-field, he could estimate what the charges of the various oil drops were at various degrees of ionisation. Regardless of the degree of ionisation, he found that the charge on a drop was always a multiple of: 1.6 x 10-19 C. NOTE: at the time, electrons and protons were considered fundamental particles. Being fundamental meant that these two particles carried the smallest possible quantity of charge (q). All charged bodies must therefore carry an integer multiple of q. Millikan used this concept in determining the charge of a single electron.
Why was the Geiger Marsden experiment undertaken?
The experiment was designed by Rutherford’s associate; Hans Geiger and his student Ernest Marsden to test out the structure of the atom.
They wanted to test out the plum pudding model but later found that the results of the experiment could be explained by Rutherford’s later proposed model of the atom.
Explain how it was conducted and the significance of the Geiger Marsden experiment.
The experiments were performed by firing alpha particles at a thin sheet of metal foil
The source of alpha particles was encased in a lead box with a small hole out of which a focused beam of alpha particles could emerge, Gold foil was used as it could be beaten into a very thin slice whilst still maintaining its shape and integrity. As per the plum pudding model, which depicts the atom as a ‘diffuse ball’ of positive charges with electrons interspersed in it, the expectation was that ALL alpha particles (which are as small as an atom) would not collide with anything and pass straight through, no deflections were expected to occur. However, results showed deflection at large angles in the centre of the ball. Showed that the plum model was incorrect. The results showed that alpha particles got through for the most part except in the central region of the atom. This could only make sense if the central region of the gold atom was small, dense and positively charged and would repel the alpha particles (also, small, dense and positively charged).This led Rutherford to propose an atomic model of a charged nucleus surrounded by electrons that orbited the nucleus
How did Chadwick ultimately discover the neutron?
In 1931, two German scientists Walther Bothe and Herbert Becker bombarded the light elements lithium, beryllium, and boron with alpha particles. From these elements, a new type of radiation was thought to have emerged upon bombardment. This radiation was highly penetrating, hence they assumed it was gamma rays. However, this was proven to be wrong by Frederic Joiliot and Irene Curie, These two were interested in the radiation made in Germany, so they fired alpha particles at a block of paraffin wax, managing to knock some of the protons out of the wax. They were not only able to reproduce Bothe’s radiation but also found that this radiation caused high energy (5MeV) protons to be ejected from other substances. Later, James Chadwick applied the law of conservation of momentum to understand that protons were too heavy to be dislodged by mere gamma rays (have no mass but carry energy). He was able to show that the mass of Bothe’s radiation was very similar to the mass of a proton but just without the charge (as it was un-deflected by electric or magnetic fields). He named this new particle, the neutron.
With this, atomic models featuring a nucleus with both positive protons and neutrally charged neutrons emerged shortly after.
What was Rutherford’s model?
Rutherford put forward the nuclear model of the atom in which a central positive nucleus was orbited by electrons in circular orbits
What were the limitations of Rutherford’s model?
Accelerating charged particles emit EMR and according to the LOCOE electrons would emit energy due to their circular motion (an accelerating charge radiates EMR)
This means net energy would decrease as they would not be able to maintain orbit, the electron spirals until it hits the nucleus
As it does this, it was understood that the electron should be emitting energy in a continuous fashion, producing a continuous spectrum
Instead, the spectra produced by certain species showed discrete wavelengths of light
In direct contradiction with Rutherford’s model. Bohr also couldn’t explain why each element emitted a different set of wavelengths.