Physics Common Response Flashcards

1
Q

Explain the formation of interference patterns

A
  • laser light made up of electromagnetic waves
  • as the waves pass through mesh > diffract
  • when light reaches screen > interference pattern
  • when light from different waves meet the screen in phase with one another > constructive interference (resulting in maxima)
  • light arrives in phase with path difference n(wavelength), where n = 1,2 etc
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2
Q

Assess the evidence for Newton’s theory of light

A
  • very little evidence to support
  • newton’s theory state that light consists of small solid particles with intrinsic properties such as shape and sides
  • could accurately predict reflection and refraction of light, and dispersion into the colours
  • no empirical evidence that supported the wave model, and he was contradicted through Young’s double slit
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3
Q

Assess the evidence for Huygen’s theory of light

A
  • consisted of wave model of light (where wavelets propagate from individual spreading out centres along the wavefront)
  • Huygen’s theory was clearly supported through empirical evidence
  • Young’s double slit experiment, demonstrating diffraction and interference patterns provided strong evidence
  • Foucault verified Huygen model by showing that light travels slower in denser material
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4
Q

Assess Maxwell’s contribution to the classical theory of electromagnetism

A
  • vitally important to classical theory (3 predictions)
  • light is an em wave, with self-propagating electric and magnetic fields
  • light is only one part of spectrum
  • the speed of electromagnetic waves is c
  • Maxwell was the foundation of electromagnetism
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5
Q

Explain how the spectra of a star is produced, and how it can be used to show the star’s composition

A
  • continuous spectrum is emitted from the core of the star
  • travels outwards through the photosphere
  • photons with energies that correspond to the atomic energy level transitions of the gases that make up the photosphere are absorbed
  • photons of these energies are missing from the emission spectra of the star on earth
  • each element in the star will give rise to a unique series of lines which enables elements present in the star to be determined (chem comp)
  • the abundance of these elements are measured through the intensities of the spectral lines
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6
Q

characteristics of stars found from its spectra

A

surface temp
- determined through Wein’s Law, where wavelength max is determined from the stars spectrum.
- longer wavelengths > cooler temp
- shorter wavelengths > warmer temp

chemical comp
- found by comparing the emission spectra of known elements, with the absorption spectra of a star
- the absorption levels ate present due to the atomic energy level transitions of the atoms in the photosphere
- shared bonds indicate the elements presence

translational velocity
- obtained through red or blue shift
- red-shifted (longer wavelength) it is moving away
- blue-shifted (shorter wavelength) it is moving towards
- the larger the shift, the faster it’s moving

rotational velocity
- determined through the width of the absorption bands
- faster it is rotating, the wider the absorption bands are

density layers
- obtained through the spectra
- wider absorption pattern for more dense (as a more dense star has more collisions)
- this is called collisional broadening

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7
Q

Explain strategies to improve transformer efficiency

A
  • Eddy currents (resistive heating effects)
    laminate to have smaller or prevent eddy currents
  • Incomplete flux linkage between primary and secondary
    solid iron core
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