1. Coherent beams with wavelengths of 400 nm intersect at points on the screen. What will be observed at these points interference maximum or minimum, if the optical path difference of the beam is in the 1st case A1=20 um and in the 2nd - A2=15 um? Find the order of minimum and maximum. 2. An installation for observing Newton's rings in reflected light is illuminated by monochromatic light incident normally to the plate surface. The distance between the second and fourth dark rings is 5 mm. Find the distance between the eighth and sixteenth light rings. 3. Find the angle between the main planes of the polarizer and the analyzer if the intensity of the natural light passing through the polarizer and the analyzer decreased by 5 times.

Answers

Answer 1
Answer:
  • 1. The observed interference at points will be maximum for \(A_1 = 20 \, \mu m\) and minimum for \(A_2 = 15 \, \mu m\), with orders 12th maximum and 12th minimum.
  • 2. The distance between the eighth and sixteenth light rings is approximately 2.583 mm.
  • 3. The angle between the main planes of the polarizer and the analyzer is approximately \(63.43^\circ\) when the intensity decreases by 5 times.

1. For coherentbeams with wavelengths of 400 nm, the interference observed at points on the screen will be maximum when the optical path difference (OPD) is a whole number of wavelengths (\(m \lambda\)), and minimum when the OPD is a half-integer number of wavelengths (\((m + 0.5) \lambda\)).

Given

\(A_1 = 20 \, \mu m\)

\(A_2 = 15 \, \mu m\), the difference in optical path between the two cases is \(\Delta A = A_1 - A_2 = 5 \, \mu m\).

The number of wavelengths difference can be calculated as \((\Delta A)/(\lambda)\), which is approximately 12.5 wavelengths.

2. In Newton's ringspattern, the radius of the m dark ring is given by \(r_m = √(m \lambda R)\), where R is the radius of curvature of the lens.

Given the distance between the second and fourth darkrings (\(m = 2\) to \(m = 4\)) as 5 mm, we can set up an equation:

\(√(4 \lambda R) - √(2 \lambda R) = 5 \, \text{mm}\).

Solving for R gives \(R \approx 1.904 * 10^(-2) \, \text{m}\).

Now, the radius of the 16th light ring can be calculated as \(r_(16) = √(16 \lambda R)\), and the radius of the 8th light ring is \(r_(8) = √(8 \lambda R)\). The distance between these two light rings is then given by:

\(d = r_(16) - r_(8) \n\n= √(16 \lambda R) - √(8 \lambda R)\).

Plugging in the values, we get \(d \approx 2.583 \, \text{mm}\).

3. When the intensity decreases by a factor of 5, the transmission of the polarizer and analyzer combination becomes \((1)/(√(5))\) times the original transmission, as intensity is proportional to the square of the transmission.

The relationship between the intensity and the angle \(\theta\) between the main planes of the polarizer and the analyzer is given by Malus's law: \(I = I_0 \cos^2 \theta\), where \(I_0\) is the initial intensity.

Given that \(I_0\) decreases by a factor of 5, we have:

\((I)/(I_0) = (1)/(√(5)) \n\n= \cos^2 \theta\)

Solving for \(\theta\), we get:

\(\theta = \arccos \left( (1)/(√(5)) \right)\n\n \approx 63.43^\circ\)

Thus, the angle is \(63.43^\circ\).

For more details regarding wavelength, visit:

brainly.com/question/31143857

#SPJ4

Answer 2
Answer:

Answer:

a=3....................................


Related Questions

What is the energy of a photon whose frequency is 6.0x10^20 hz?
If a bar magnet is cut 3 times resulting in 4 smaller magnet pieces, then each new magnet will have *A.only a N poleB. only a S poleC. both a N and S poleD.neither a N nor a S pole
Convert 93 nanometer to meters.
Which term refers to the phenomenon of light shining on a metal and causing electrons to break free from their atoms?A. Blackbody radiationB.Ultraviolet catastropheC. Emission spectraD. Photoelectric effect
you kick a soccer ball straight up into the air with a speed of 21.2 m/s. How long does it take he soccer ball to reach its highest point?.

Which of the following sensory receptors would lead you to squint in bright light?. A. thermoreceptors B. mechanoreceptors C. photoreceptors D. chemoreceptors

Answers

If my memory serves me well, sensory receptors which would lead you to squint in bright light are called C. photoreceptors

A planet moves fastest when it is ___________________ to the Sun and slowest when it is ___________________ from the Sun. Choose one: A. farthest; closest B. at the nearest focus; at the farthest focus C. closest; farthest

Answers

Answer:

option (c) is correct

Explanation:

A planet moves fastest when it is closest to the Sun and slowest when it is farthest from the Sun.

Answer:

fastest when closest to the Sun, slowest when it is farthest

Explanation:

Plato/Edmentum

the maximum characteristic x-ray photon energy comes from the capture of a free electron into a k shell vacancy. what is this photon energy in kev for polonium assuming the free electron has no initial kinetic energy?

Answers

The photon energy is 75 keV (kilo-electron volts) for polonium, assuming the free electron has no initial kinetic energy.

The maximum characteristic x-ray photon energy from the capture of a free electron into a K-shell vacancy is equal to the difference in binding energies between the K-shell and L-shell in the atom.

For polonium (Po), the atomic number is 84, which means it has 84 electrons. The K-shell of polonium is filled with 2 electrons, and the L-shell is filled with 8 electrons.

The K-shell binding energy for polonium can be found in a table of atomic data to be around 88 keV. The L-shell binding energy can also be found in the same table to be around 13 keV.

Therefore, the maximum characteristic x-ray photon energy from the capture of a free electron into a K-shell vacancy in polonium is:

E = (K-shell binding energy) - (L-shell binding energy)

= 88 keV - 13 keV

= 75 keV

To know more about binding energies refer here

brainly.com/question/30073915#

#SPJ11

Which extremely flammable gas is most commonly burned for fuel in a home? A) Hydrogen B) Methane C) Propane D) Butane

Answers

Answer:

B ) Methane

Explanation:

Methane is known as a natural gas and is the most commonly used sources of fuel amongst businesses and homes to power water heaters and stoves.

Bode's Law: correctly predicted the location of Jupiter, uses a number sequence to determine planetary distances, incorrectly predicted the location of Uranus and Neptune, all of the above

Answers

The correct answer for the question that is being presented above is this one: "correctly predicted the location of Jupiter, uses a number sequence to determine planetary distances." Bode's law correctly predicted the location of Jupiter, uses a number sequence to determine planetary distances.

Final answer:

Bode's Law, also known as Titius-Bode law, provides a numerical pattern that predicts the position of most planets in our Solar System, including Jupiter. It, however, fails to accurately predict the location of Uranus and Neptune. The fundamental principles of planetary motion were established by Kepler's laws and later consolidated by Newton in his Universal Law of Gravitation.

Explanation:

This question pertains to Bode's Law, a rule of planetary distances at times referred to as the Titius-Bode Law. The rule indicates a pattern of increasing distances of the planets from the sun, which interestingly correlates to the position of most planets in our Solar System, including Jupiter. However, exceptions, particularly Uranus and Neptune, don't fit precisely into this pattern.

The origins of planetary motions can be traced back to the work of scientists like Herr Tycho Brahe, Johannes Kepler, and Sir Isaac Newton. Kepler's work in particular developed three fundamental laws of planetary motion using Brahe's meticulously collected data. These laws describe the behavior of planets in their orbits and together provide the foundation of the Universal Law of Gravitation as later synthesized by Newton.

Learn more about Bode's Law here:

brainly.com/question/35159500

#SPJ3

Radio telescopes measure the galaxy’s distribution of

Answers

Radio Telescopes measures the galaxy's distribution of stars, galaxies, blackholes and other astronomical objects. It is used to study naturally -occuring radio light which is emitted by these astronomical bodies. Radio observatories are located far away from major cities to avoid electromagnetic interference from radio, televisions and radar.

hydrogen from which stars are formed