The frequency of the most intense radiation emitted by the planet into outer space is 1.148 x 10^12 Hz
The answer to the first part of the question "The average surface temperature of a planet is 292 K" is given, and we need to determine the frequency of the most intense radiation emitted by the planet into outer space.
Frequency can be calculated using Wien's displacement law.
According to Wien's law, the frequency of the radiation emitted by a body is proportional to the temperature of the body.
The frequency of the most intense radiation emitted by the planet into outer space can be found using Wien's law.
The formula for Wien's law is:
λ_maxT = 2.898 x 10^-3,
whereλ_max is the wavelength of the peak frequency,T is the temperature of the planet in kelvin, and, 2.898 x 10^-3 is a constant.
The frequency of the most intense radiation emitted by the planet into outer space can be found using the relation:
c = fλ
c is the speed of light (3 x 10^8 m/s), f is the frequency of the radiation emitted by the planet, λ is the wavelength of the peak frequency
We can rearrange Wien's law to solve for the peak frequency:
f = c/λ_maxT
= c/(λ_max * 292)
Substitute the values and calculate:
f = (3 x 10^8 m/s)/(9.93 x 10^-7 m * 292)
= 1.148 x 10^12 Hz
Therefore, the frequency of the most intense radiation emitted by the planet into outer space is 1.148 x 10^12 Hz.
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Compare and contrast prototype theory and theory-based view of category representation, Explain which one better explains how knowledge is represented.
Prototype theory and the theory-based view of category representation are two different approaches to understanding how knowledge is represented in categories. While both theories provide insights into categorization, they differ in their underlying assumptions and emphasis on different aspects of category representation.
Prototype theory suggests that categories are represented by a central prototype or a typical example that captures the most characteristic features of the category.
According to this view, category membership is determined by comparing objects or concepts to the prototype and assessing their similarity. Prototype theory emphasizes the role of similarity and graded membership, allowing for flexibility and variability in category boundaries. It acknowledges that categories can have fuzzy boundaries and that members can differ in terms of typicality.
In contrast, the theory-based view of category representation posits that categories are defined by a set of defining features or rules. According to this view, category membership is determined by the presence or absence of these defining features. The theory-based view emphasizes the role of explicit rules and criteria for categorization. It assumes that categories have clear-cut boundaries and that membership is based on meeting specific criteria.
Both prototype theory and the theory-based view have strengths and weaknesses in explaining category representation. Prototype theory provides a more flexible and dynamic account of categorization, capturing the variation and context-dependency often observed in real-world categories. It accounts for typicality effects and the graded structure of categories. On the other hand, the theory-based view offers a more precise and rule-based approach to categorization, emphasizing the importance of defining features and criteria for membership.
The question of which theory better explains how knowledge is represented depends on the context and nature of the categories being considered. Prototype theory is often favored for capturing everyday categorization and capturing the cognitive flexibility involved in category formation. However, the theory-based view may be more suitable when dealing with categories that have clear criteria and strict boundaries, such as scientific categories.
In summary, both prototype theory and the theory-based view provide valuable insights into category representation. The choice of which theory better explains knowledge representation depends on the specific context and nature of the categories being studied, as both approaches have their strengths and limitations.
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Two point charges produce an electrostatic force of 6.87 × 10-3 N Determine the electrostatic force produced if charge 1 is doubled, charge 2 is tripled and the distance between them is
alf.
elect one:
) a. 1.65 x 10-1 N • b. 6.87 × 10-3 N ) c. 4.12 × 10-2.N
) d. 2.06 x 10-2 N
The electrostatic force produced when charge 1 is doubled, charge 2 is tripled, and the distance between them is halved is approximately 1.48 N. None of the provided answer choices (a), (b), (c), or (d) match this value.
To determine the electrostatic force produced when charge 1 is doubled, charge 2 is tripled, and the distance between them is halved, we can use Coulomb's Law.
Coulomb's Law states that the electrostatic force (F) between two point charges is given by the equation:
F = k * (|q1| * |q2|) / r^2
where k is the electrostatic constant (k ≈ 8.99 × 10^9 Nm^2/C^2), |q1| and |q2| are the magnitudes of the charges, and r is the distance between them.
Let's denote the original values of charge 1, charge 2, and the distance as q1, q2, and r, respectively. Then the modified values can be represented as 2q1, 3q2, and r/2.
According to the problem, the electrostatic force is 6.87 × 10^(-3) N for the original configuration. Let's denote this force as F_original.
Now, let's calculate the modified electrostatic force using the modified values:
F_modified = k * (|(2q1)| * |(3q2)|) / ((r/2)^2)
= k * (6q1 * 9q2) / (r^2/4)
= k * 54q1 * q2 / (r^2/4)
= 216 * (k * q1 * q2) / r^2
Since k * q1 * q2 / r^2 is the original electrostatic force (F_original), we have:
F_modified = 216 * F_original
Substituting the given value of F_original = 6.87 × 10^(-3) N into the equation, we get:
F_modified = 216 * (6.87 × 10^(-3) N)
= 1.48 N
Therefore, the electrostatic force produced when charge 1 is doubled, charge 2 is tripled, and the distance between them is halved is approximately 1.48 N.
None of the provided answer choices matches this value, so none of the options (a), (b), (c), or (d) are correct.
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Question 21 () a) wider fringes will be formed by decreasing the width of the slits. increasing the distance between the slits. increasing the width of the slits. decreasing the distance between the slits. Question 22 () b) changing the color of the light from red to violet will make the pattern smaller and the fringes thinner. make the pattern larger and the fringes thicker. make the pattern larger and the fringes thinner. make the pattern smaller and the fringes thicker.
1) Wider fringes can be achieved by decreasing the width of the slits and increasing the distance between them, while narrower fringes are obtained by increasing the slit width and decreasing the slit distance.
2) Changing the color of the light from red to violet leads to smaller pattern size and thinner fringes, while switching from violet to red creates a larger pattern with thicker fringes.
1) When observing interference fringes produced by a double-slit setup, the width of the fringes can be affected by adjusting the parameters. The width of the fringes will increase by decreasing the width of the slits and increasing the distance between the slits. Conversely, the width of the fringes will decrease by increasing the width of the slits and decreasing the distance between the slits.
2) Changing the color of the light from red to violet in an interference pattern will influence the size and thickness of the fringes. Switching from red to violet light will make the pattern smaller and the fringes thinner. Conversely, changing the color from violet to red will result in a larger pattern with thicker fringes.
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Abusive behavior inventory total scale (abi) 36. 05 07. 49 psychological abuse 25. 40 6. 35 physical abuse 10. 66 1. 74
The total scale score of the Abusive Behavior Inventory (ABI) is 36.05, indicating the overall level of abusive behavior measured by the inventory. This score represents a combination of psychological abuse and physical abuse.
The psychological abuse score on the ABI is 25.40, suggesting the extent of psychological mistreatment or harm inflicted upon individuals. This score is based on responses to items related to psychological abuse within the inventory. A higher score indicates a higher level of psychological abuse experienced.
The physical abuse score on the ABI is 10.66, indicating the degree of physical harm or violence experienced by individuals. This score is derived from responses to items specifically related to physical abuse within the inventory. A higher score reflects a higher level of physical abuse endured.
These scores provide quantitative measures of abusive behavior, allowing for assessment and evaluation of individuals' experiences. It is important to interpret these scores within the context of the ABI and consider other relevant factors when assessing abusive behavior in individuals or populations.
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What is the net change in energy of a system over a period of 1.5 hours if the system has a power output of 140W? O A. 70.0 kJ O B. 756.0 kJ C. 93.3 kJ O D. 1.6 kJ
The net change in energy of the system over a period of 1.5 hours, with a power output of 140W, is 756.0 kJ. Option B is correct.
To determine the net change in energy of a system over a period of time, we need to calculate the energy using the formula:
Energy = Power × Time
Power output = 140 W
Time = 1.5 hours
However, we need to convert the time from hours to seconds to be consistent with the unit of power (Watt).
1.5 hours = 1.5 × 60 × 60 seconds
= 5400 seconds
Now we can calculate the energy:
Energy = Power × Time
Energy = 140 W × 5400 s
Energy = 756,000 J
Converting the energy from joules (J) to kilojoules (kJ):
756,000 J = 756 kJ
The correct answer is option B.
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Part A What is the approximate radius of an a particle (He)? Express your answer to two significant figures and include the appropriate units. ? HA Value Units The Submit Request Answer
As per the details, the approximate radius of an alpha particle (He) is 1.2 fm.
The Rutherford scattering formula, which connects the scattering angle to the impact parameter and the particle radius, can be used to estimate the approximate radius of an alpha particle (He). The formula is as follows:
θ = 2 * arctan ( R / b )
Here,
θ = scattering angle
R = radius of the particle
b = impact parameter
An alpha particle (He) is made up of two protons and two neutrons that combine to produce a helium nucleus. A helium nucleus has a radius of about 1.2 femtometers (fm) or [tex]1.2* 10^{(-15)[/tex] metres.
Therefore, the approximate radius of an alpha particle (He) is 1.2 fm.
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What is the frequency of a sound wave with a wavelength of 2.81 m
traveling in room-temperature air (v
= 340 m/s)?
The speed of sound in air is approximately 340 m/s, which represents the rate at which sound waves travel through the medium of air. So, the frequency of the sound wave is approximately 121.00 Hz. It is commonly measured in hertz (Hz), where 1 Hz represents one cycle per second.
The speed of sound in air is approximately 340 m/s. The formula to calculate the frequency of a wave is given by:
frequency = speed / wavelength
Substituting the given values:
frequency = 340 m/s / 2.81 m
frequency ≈ 121.00 Hz
Therefore, the frequency of the sound wave is approximately 121.00 Hz. It is commonly measured in hertz (Hz), where 1 Hz represents one cycle per second.
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An RL circuit is composed of a 12 V battery, a 6.0 H inductor and a 0.050 Ohm resistor.
The switch is closed at t = 0
An RL circuit is composed of a 12 V battery, a 6.0 H inductor and a 0.050 Ohm resistor.
The switch is closed at t = 0
These are the options:
The time constant is 1.2 minutes and after the switch has been closed a long time the voltage across the inductor is zero.
The time constant is 2.0 minutes and after the switch has been closed a long time the voltage across the inductor is 12 V.
The time constant is 1.2 minutes and after the switch has been closed a long time the voltage across the inductor is 12 V.
The time constant is 2.0 minutes an
The correct option is : The time constant is 2.0 minutes, and after the switch has been closed for a long time, the voltage across the inductor is zero.
To determine the time constant and the voltage across the inductor after a long time, we can use the formula for the time constant of an RL circuit:
τ = L/R
where τ is the time constant, L is the inductance, and R is the resistance.
In this case, the inductance (L) is given as 6.0 H and the resistance (R) is given as 0.050 Ω.
Using the formula, we can calculate the time constant:
τ = 6.0 H / 0.050 Ω = 120 seconds
Since the time constant is given in seconds, we need to convert it to minutes:
τ = 120 seconds * (1 minute / 60 seconds) = 2.0 minutes
So, the correct option is:
The time constant is 2.0 minutes, and after the switch has been closed for a long time, the voltage across the inductor is zero.
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The figure below shows a ball of mass m=1.9 kg which is connected to a string of length L=1.9 m and moves in a vertical circle. Only gravity and the tension in the string act on the ball. If the velocity of the ball at point A is v0=4.2 m/s, what is the tension T in the string when the ball reaches the point B?
The tension in the string at point B is approximately 29.24 N.
To find the tension in the string at point B, we need to consider the forces acting on the ball at that point. At point B, the ball is at the lowest position in the vertical circle.
The forces acting on the ball at point B are gravity (mg) and tension in the string (T). The tension in the string provides the centripetal force necessary to keep the ball moving in a circle.
At point B, the tension (T) and gravity (mg) add up to provide the net centripetal force. The net centripetal force is given by:
T + mg = mv^2 / R
Where m is the mass of the ball, g is the acceleration due to gravity, v is the velocity of the ball, and R is the radius of the circular path.
The radius of the circular path is equal to the length of the string (L) since the ball moves in a vertical circle. Therefore, R = L = 1.9 m.
The velocity of the ball at point B is not given directly, but we can use the conservation of mechanical energy to find it. At point A, the ball has gravitational potential energy (mgh) and kinetic energy (1/2 mv0^2), where h is the height from the lowest point of the circle to point A.
At point B, all the gravitational potential energy is converted into kinetic energy, so we have:
mgh = 1/2 mv^2
Solving for v, we find:
v = sqrt(2gh)
Substituting the given values of g (9.8 m/s^2) and h (L = 1.9 m), we can calculate the velocity at point B:
v = sqrt(2 * 9.8 * 1.9) ≈ 7.104 m/s
Now we can substitute the values into the equation for net centripetal force:
T + mg = mv^2 / R
T + (1.9 kg)(9.8 m/s^2) = (1.9 kg)(7.104 m/s)^2 / 1.9 m
Simplifying and solving for T, we get:
T ≈ 29.24 N
Therefore, the tension in the string at point B is approximately 29.24 N.
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A quantity is calculated bases on (20 + 1) + [(50 + 1)/(5.0+ 0.2)] value of the quantity is 30, but what is the uncertainty in this?
Thus, the uncertainty in the calculated quantity is approximately 0.10. The formula to calculate the uncertainty of a quantity is given by δQ=√(δA²+δB²)
Given (20 + 1) + [(50 + 1)/(5.0+ 0.2)] = 30. (20 + 1) + [(50 + 1)/(5.0+ 0.2)] is the quantity whose uncertainty we want to calculate.
We know that: δA = uncertainty in 20.1 = ±0.1δ
B = uncertainty in (50 + 1)/(5.0+ 0.2) = uncertainty in (51/5.2)
We have to calculate δB:δB = uncertainty in (51/5.2) = δ[(50 + 1)/(5.0+ 0.2)] = δ(51/5.2) = [(1/5.2)² + (0.2*51)/(5.2²)]½= (0.00641 + 0.00293)½= 0.0083
∴δQ = √(δA² + δB²) = √(0.1² + 0.0083²) = √(0.01009) = 0.1005 ≈ 0.10
Thus, the uncertainty in the calculated quantity is approximately 0.10.
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quick answer
please
QUESTION 17 An observatory uses a large refracting telescope that has an objective lens of diameter, 1.00 m. The telescope resolves images with green light of wavelength 550 nm. If the telescope can b
The telescope can resolve objects with an angular size greater than or equal to 1.21 arcseconds.
The resolving power of a telescope determines its ability to distinguish fine details in an observed object. It is determined by the diameter of the objective lens or mirror and the wavelength of the light being observed. The formula for resolving power is given by:
R = 1.22 * (λ / D)
Where R is the resolving power, λ is the wavelength of light, and D is the diameter of the objective lens or mirror.
In this case, the diameter of the objective lens is given as 1.00 m, and the wavelength of green light is 550 nm (or 550 x 10^-9 m). Plugging in these values into the formula, we can calculate the resolving power:
R = 1.22 * (550 x 10^-9 m / 1.00 m)
R ≈ 1.21 x 10^-3 radians
To convert the resolving power to angular size, we can use the fact that there are approximately 206,265 arcseconds in a radian:
Angular size = R * (206,265 arcseconds/radian)
Angular size ≈ 1.21 x 10^-3 radians * 206,265 arcseconds/radian
The result is approximately 1.21 arcseconds. Therefore, the telescope can resolve objects with an angular size greater than or equal to 1.21 arcseconds.
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QUESTION 3 What is the mutual inductance in nk of these two loops of wire? Loop 1 Leop 44 20 Both loops are rectangles, but the length of the horizontal components of loop 1 are infinite compared to the size of loop 2 The distance d-5 cm and the system is in vacuum
Mutual inductance is an electromagnetic quantity that describes the induction of one coil in response to a variation of current in another nearby coil.
Mutual inductance is denoted by M and is measured in units of Henrys (H).Given that both loops are rectangles, the length of the horizontal components of loop 1 are infinite compared to the size of loop 2. The distance d-5 cm and the system is in vacuum, we are to calculate the mutual inductance of both loops.
The formula for calculating mutual inductance is given as:
[tex]M = (µ₀ N₁N₂A)/L, whereµ₀ = 4π × 10−7 H/m[/tex] (permeability of vacuum)
N₁ = number of turns of coil
1N₂ = number of turns of coil 2A = area of overlap between the two coilsL = length of the coilLoop 1,Leop 44,20 has a rectangular shape with dimensions 44 cm and 20 cm, thus its area
[tex]A1 is: A1 = 44 x 20 = 880 cm² = 0.088 m²[/tex].
Loop 2, on the other hand, has a rectangular shape with dimensions 5 cm and 20 cm, thus its area A2 is:
[tex]A2 = 5 x 20 = 100 cm² = 0.01 m².[/tex]
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What is the electrostatic force of attraction between 2 positively charged particles separated by 0.30 meter distance and with a charge of 8.0x10-6 C and 5.0x10-6 C respectively? A
8.0×10^5 N 1.2 N
2.4×10^5 N 4.0 N
The electrostatic force of attraction between the two positively charged particles is approximately 4.4 × 10^-9 N.
The electrostatic force of attraction between two charged particles can be calculated using Coulomb's law, which states that the force is directly proportional to the product of the charges and inversely proportional to the square of the distance between them. Mathematically, it can be expressed as:
F = (k * q1 * q2) / r^2
Where: F is the electrostatic force of attraction, k is the electrostatic constant (approximately 9 × 10^9 Nm^2/C^2), q1 and q2 are the charges of the particles, and r is the distance between the particles.
Plugging in the given values: q1 = 8.0 × 10^-6 C q2 = 5.0 × 10^-6 C r = 0.30 m
F = (9 × 10^9 Nm^2/C^2) * (8.0 × 10^-6 C) * (5.0 × 10^-6 C) / (0.30 m)^2
Simplifying the equation: F = (9 × 8.0 × 5.0 × 10^-6 × 10^-6) / (0.09) F = 36 × 10^-12 / 0.09 F = 4 × 10^-10 / 0.09 F ≈ 4.4 × 10^-9 N
Therefore, the electrostatic force of attraction between the two positively charged particles is approximately 4.4 × 10^-9 N.
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A block, W 180 lbs rests on a rough level plane. The coefficient of friction is 0.42, what horizontal push will cause the block to move? What inclined push making 45° with the horizontal will cause the block to move?
The inclined push making a 45° angle with the horizontal should satisfy the equation: Horizontal component = inclined push × cos(45°) ≥ Frictional force
To determine the horizontal push required to make the block move, we need to consider the force of friction acting on the block. The force of friction can be calculated using the formula:
Frictional force = coefficient of friction × normal force
The normal force is equal to the weight of the block, which is 180 lbs. Therefore, the normal force is 180 lbs × acceleration due to gravity.
To find the horizontal push, we need to overcome the force of friction. The force of friction is given by the equation:
Frictional force = coefficient of friction × normal force
Let's calculate the force of friction:
Frictional force = 0.42 × (180 lbs × acceleration due to gravity)
Now we can calculate the horizontal push:
Horizontal push = Frictional force
To Know the inclined push making a 45° angle with the horizontal, we need to consider the force components acting on the block. The horizontal component of the inclined push will contribute to overcoming the force of friction, while the vertical component will assist in counteracting the weight of the block.
Since the inclined push makes a 45° angle with the horizontal, the horizontal component can be calculated using the formula:
Horizontal component = inclined push × cos(45°)
To make the block move, the horizontal component of the inclined push should be equal to or greater than the force of friction calculated previously.
Therefore, the inclined push making a 45° angle with the horizontal should satisfy the equation:
Horizontal component = inclined push × cos(45°) ≥ Frictional force
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A cylinder of radius 10 cm has a thread wrapped around its edge. If the cylinder is initially at rest and begins to rotate with an angular acceleration of 1 rad/s2, determine the length of thread that unwinds in 10 seconds.
Given
,Radius of cylinder
= r = 10 cm = 0.1 mAngular acceleration of cylinder = α = 1 rad/s²Time = t = 10s
Let’s find the angle covered by the cylinder in 10 seconds using the formula:θ = ωit + 1/2 αt²whereωi = initial angular velocity = 0 rad/st = time = 10 sα = angular acceleration = 1 rad/s²θ = 0 + 1/2 × 1 × (10)² = 50 rad
Now, let's find the length of the
thread
that unwinds using the formula:L = θrL = 50 × 0.1 = 5 mTherefore, the length of the thread that unwinds in 10 seconds is 5 meters.
Here, we used the formula for the arc
length of a circle
, which states that the length of an arc (in this case, the thread) is equal to the angle it subtends (in radians) times the radius.
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Determine the number of electrons, protons, and neutrons in
argon
3818Ar
.
HINT
(a)
electrons
(b)
protons
(c)
neutrons
The number of electrons in Argon is 18, the number of protons is 18, and the number of neutrons is 20.
Now, let's proceed to the second part of the question. Here's how to determine the number of electrons, protons, and neutrons in Argon 38 :18 Ar :Since the atomic number of Argon is 18, it has 18 protons in its nucleus, which is also equal to its atomic number.
Since Argon is neutral, it has 18 electrons orbiting around its nucleus.In order to determine the number of neutrons, we have to subtract the number of protons from the atomic mass. In this case, the atomic mass of Argon is 38.
Therefore: Number of neutrons = Atomic mass - Number of protons Number of neutrons = 38 - 18 Number of neutrons = 20 Therefore, the number of electrons in Argon is 18, the number of protons is 18, and the number of neutrons is 20
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Three negative charged particles of equal charge, -15x10^-6, are located at the corners of an equilateral triangle of side 25.0cm. Determine the magnitude and direction of the net electric force on each particle.
The magnitude of the net electric force on each particle is 2.025 N directed away from the triangle.
Charge on each particle, q1 = q2 = q3 = -15 × 10⁻⁶C
∴ Net force on particle 1 = F1
Net force on particle 2 = F2
Net force on particle 3 = F3
The magnitude of the net electric force on each particle:
It can be determined by using Coulomb's Law:
F = kqq / r²
where
k = Coulomb's constant = 9 × 10⁹ Nm²/C²
q = charge on each particle
r = distance between the particles
We know that all three charges are negative, so they will repel each other. Therefore, the direction of net force on each particle will be away from the triangle.
From the given data,
Side of equilateral triangle, a = 25cm = 0.25m
∴ Distance between each corner of the triangle = r = a = 0.25m
∴ Net force on particle 1 = F1
F1 = kq² / r² = 9 × 10⁹ × (-15 × 10⁻⁶)² / (0.25)²= -2.025 N
∴ Net force on particle 2 = F2
F2 = kq² / r² = 9 × 10⁹ × (-15 × 10⁻⁶)² / (0.25)²= -2.025 N
∴ Net force on particle 3 = F3
F3 = kq² / r² = 9 × 10⁹ × (-15 × 10⁻⁶)² / (0.25)²= -2.025 N
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Part A Monochromatic light passes through two slits separated by a distance of 0.0344 mm. If the angle to the third maximum above the central fringe is 3.61 °, what is the wavelength of the light? Express your answer to three significant figures. VI AEQ ? l= nm Submit Request Answer
A Monochromatic light passes through two slits separated by a distance of 0.0344 mm. If the angle to the third maximum above the central fringe is 3.61 °, the wavelength of the light is 634.62 nm.
To solve this problem, we can use the following equation:
sin(theta) = n * lambda / d
Where:
theta is the angle to the nth maximum above the central fringe in degrees
n is the order of the maximum (in this case, n = 3)
lambda is the wavelength of the light in meters
d is the distance between the slits in meters
Plugging in the values, we get:
sin(3.61°) = 3 * lambda / 0.0344 mm
lambda = (0.0344 mm) * sin(3.61°) / 3
lambda = 634.62 nm
Therefore, the wavelength of the light is 634.62 nm.
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In solving problems in which two objects are joined by rope, what assumptions do we make about the mass of the rope and the forces the rope exerts on each end?
When two objects are connected by a rope, it is assumed that the mass of the rope is negligible compared to the mass of the objects, and that the forces the rope exerts on each end are equal and opposite.
When solving problems where two objects are connected by a rope, it is assumed that the mass of the rope is negligible compared to the mass of the objects, and that the forces the rope exerts on each end are equal and opposite. This is known as the assumption of massless, frictionless ropes.
In other words, the rope's mass is usually assumed to be zero because the mass of the rope is very less compared to the mass of the two objects that are connected by the rope. It is also assumed that the rope is frictionless, which means that no friction acts between the rope and the objects connected by the rope. Furthermore, it is assumed that the tension in the rope is constant throughout the rope. The forces that the rope exerts on each end of the object are equal in magnitude but opposite in direction, which is the reason why they balance each other.
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beginning with h=4.136x10-15 eV.s and c = 2.998x108 m/s , show that hc =1240 eV-nm.
Beginning with h=4.136x10-15 eV.s and c = 2.998x108 m/s , we have shown that hc is approximately equal to 1240 eV·nm
We'll start with the given values:
h =Planck's constant= 4.136 x 10^(-15) eV·s
c = speed of light= 2.998 x 10^8 m/s
We want to show that hc = 1240 eV·nm.
We know that the energy of a photon (E) can be calculated using the formula:
E = hc/λ
where
h is Planck's constant
c is the speed of light
λ is the wavelength
E is the energy of the photon.
To prove hc = 1240 eV·nm, we'll substitute the given values into the equation:
hc = (4.136 x 10^(-15) eV·s) ×(2.998 x 10^8 m/s)
Let's multiply these values:
hc ≈ 1.241 x 10^(-6) eV·m
Now, we want to convert this value from eV·m to eV·nm. Since 1 meter (m) is equal to 10^9 nanometers (nm), we can multiply the value by 10^9:
hc ≈ 1.241 x 10^(-6) eV·m × (10^9 nm/1 m)
hc ≈ 1.241 x 10^3 eV·nm
Therefore, we have shown that hc is approximately equal to 1240 eV·nm
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How much heat in joules is required to convery 1.00 kg of ice at 0 deg C into steam at 100 deg C? (Lice = 333 J/g; Lsteam= 2.26 x 103 J/g.)
The heat required to convert 1.00 kg of ice at 0°C to steam at 100°C is 1.17 x 10⁶ J.
To calculate the heat required to convert 1.00 kg of ice at 0°C to steam at 100°C, we need to consider three different processes: heating the ice to 0°C, melting the ice into water at 0°C, and heating the water to 100°C and converting it into steam.
1. Heating the ice to 0°C:
The heat required is given by Q1 = m × Cice × ∆T, where m is the mass of ice, Cice is the heat capacity of ice, and ∆T is the temperature change.
Q1 = 1.00 kg × (333 J/g) × (0 - (-273.15)°C) = 3.99 x 10⁵ J
2. Melting the ice into water at 0°C:
The heat required is given by Q2 = m × L_ice, where Lice is the heat of fusion of ice.
Q2 = 1.00 kg × (333 J/g) = 3.33 x 10⁵ J
3. Heating the water to 100°C and converting it into steam:
The heat required is given by Q3 = m × Cwater × ∆T + m × Lsteam, where Cwater is the heat capacity of water, Lsteam is the heat of vaporization of water, and ∆T is the temperature change.
Q3 = 1.00 kg × (4.18 J/g°C) × (100 - 0)°C + 1.00 kg × (2.26 x 10³ J/g) = 4.44 x 10⁵ J
The total heat required is the sum of the three processes:
Total heat = Q1 + Q2 + Q3 = 3.99 x 10⁵ J + 3.33 x 10⁵ J + 4.44 x 10⁵ J = 1.17 x 10⁶ J
Therefore, the heat required to convert 1.00 kg of ice at 0°C to steam at 100°C is 1.17 x 10⁶ J.
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If you are using a motion encodr receiver to find the veloicty of a cart, how would you find the uncertainty in veloicty?
To find the uncertainty in velocity using a motion encoder receiver, you need to consider the uncertainties in the measurements, collect multiple measurements, calculate the standard deviation, and report the uncertainty as a range around the measured velocity.
To find the uncertainty in velocity when using a motion encoder receiver, you would need to consider the uncertainties associated with the measurements taken by the receiver. Here's how you can do it:
Determine the uncertainties in the measurements: This involves identifying the sources of uncertainty in the motion encoder receiver. It could be due to factors like resolution limitations, noise in the signal, or calibration errors. Consult the manufacturer's specifications or conduct experiments to determine these uncertainties.
Collect multiple measurements: Take several velocity measurements using the motion encoder receiver. It is important to take multiple readings to account for any random variations or errors.
Calculate the standard deviation: Calculate the standard deviation of the collected measurements. This statistical measure quantifies the spread of the data points around the mean. It provides an estimation of the uncertainty in the velocity measurements.
Report the uncertainty: Express the uncertainty as a range around the measured velocity. Typically, uncertainties are reported as a range of values, such as ± standard deviation or ± percentage. This range represents the potential variation in the velocity measurements due to the associated uncertainties.
To find the uncertainty in velocity using a motion encoder receiver, you need to consider the uncertainties in the measurements, collect multiple measurements, calculate the standard deviation, and report the uncertainty as a range around the measured velocity.
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Two objects of mass 7.20 kg and 6.90 kg collide head-on in a perfectly elastic collision. If the initial velocities of the objects are respectively 3.60 m/s [N] and 13.0 m/s [S], what is the velocity of both objects after the collision? 8.20 m/s [S]; 0.353 m/s [N] 0.30 m/s [S]; 17.0 m/s [N] 12.6 m/s [S]; 3.95 m/s [N] 16 m/s [N]; 0 m/s
Two objects of mass 7.20 kg and 6.90 kg collide head-on in a perfectly elastic collision. If the initial velocities of the objects are respectively 3.60 m/s [N] and 13.0 m/s [S], the velocity of both objects after the collision is 0.30 m/s [S]; 17.0 m/s [N] .
The correct answer would be 0.30 m/s [S]; 17.0 m/s [N] .
In a perfectly elastic collision, both momentum and kinetic energy are conserved. To determine the velocities of the objects after the collision, we can apply the principles of conservation of momentum.
Let's denote the initial velocity of the 7.20 kg object as v1i = 3.60 m/s [N] and the initial velocity of the 6.90 kg object as v2i = 13.0 m/s [S]. After the collision, let's denote their velocities as v1f and v2f.
Using the conservation of momentum, we have:
m1v1i + m2v2i = m1v1f + m2v2f
Substituting the given values:
(7.20 kg)(3.60 m/s) + (6.90 kg)(-13.0 m/s) = (7.20 kg)(v1f) + (6.90 kg)(v2f)
25.92 kg·m/s - 89.70 kg·m/s = 7.20 kg·v1f + 6.90 kg·v2f
-63.78 kg·m/s = 7.20 kg·v1f + 6.90 kg·v2f
We also know that the relative velocity of the objects before the collision is equal to the relative velocity after the collision due to the conservation of kinetic energy. In this case, the relative velocity is the difference between their velocities:
[tex]v_r_e_l_i[/tex]= v1i - v2i
[tex]v_r_e_l_f[/tex] = v1f - v2f
Since the collision is head-on, the relative velocity before the collision is (3.60 m/s) - (-13.0 m/s) = 16.6 m/s [N]. Therefore, the relative velocity after the collision is also 16.6 m/s [N]:
v_rel_f = 16.6 m/s [N]
Now we can solve the system of equations:
v1f - v2f = 16.6 m/s [N] (1)
7.20 kg·v1f + 6.90 kg·v2f = -63.78 kg·m/s (2)
Solving equations (1) and (2) simultaneously will give us the velocities of the objects after the collision.
After solving the system of equations, we find that the velocity of the 7.20 kg object (v1f) is approximately 0.30 m/s [S], and the velocity of the 6.90 kg object (v2f) is approximately 17.0 m/s [N].
Therefore, after the head-on collision between the objects of masses 7.20 kg and 6.90 kg, the 7.20 kg object moves with a velocity of approximately 0.30 m/s in the south direction [S], while the 6.90 kg object moves with a velocity of approximately 17.0 m/s in the north direction [N].
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Askater extends her arms horizontally, holding a 5-kg mass in each hand. She is rotating about a vertical axis with an angular velocity of one revolution per second. If she drops her hands to her sides, what will the final angular velocity (in rev/s) be if her moment of inertia remains approximately constant at 5 kg m and the distance of the masses from the axis changes from 1 m to 0.1 m? 6 4 19 7
Initial moment of inertia, I = 5 kg m. The distance of the masses from the axis changes from 1 m to 0.1 m.
Using the conservation of angular momentum, Initial angular momentum = Final angular momentum
⇒I₁ω₁ = I₂ω₂ Where, I₁ and ω₁ are initial moment of inertia and angular velocity, respectively I₂ and ω₂ are final moment of inertia and angular velocity, respectively
The final moment of inertia is given by I₂ = I₁r₁²/r₂²
Where, r₁ and r₂ are the initial and final distances of the masses from the axis respectively.
I₂ = I₁r₁²/r₂²= 5 kg m (1m)²/(0.1m)²= 5000 kg m
Now, ω₂ = I₁ω₁/I₂ω₂ = I₁ω₁/I₂= 5 kg m × (2π rad)/(1 s) / 5000 kg m= 6.28/5000 rad/s= 1.256 × 10⁻³ rad/s
Therefore, the final angular velocity is 1.256 × 10⁻³ rad/s, which is equal to 0.0002 rev/s (approximately).
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How far apart are an object and an image formed by a 75 -cm-focal-length converging lens if the image is 2.25× larger than the object and is real? Express your answer using two significant figures.
The magnification (M) of the image formed by a lens can be calculated using the formula:
M = -di/do
where di is the image distance and do is the object distance.
Given:
Focal length (f) = 75 cm
Magnification (M) = 2.25
Since the image is real and the magnification is positive, we can conclude that the lens forms an enlarged, upright image.
To find the object distance, we can rearrange the magnification formula as follows:
M = -di/do
2.25 = -di/do
do = -di/2.25
Now, we can use the lens formula to find the image distance:
1/f = 1/do + 1/di
Substituting the value of do obtained from the magnification formula:
1/75 = 1/(-di/2.25) + 1/di
Simplifying the equation:
1/75 = 2.25/di - 1/di
1/75 = 1.25/di
di = 75/1.25
di = 60 cm
Since the object and image are on the same side of the lens, the object distance (do) is positive and equal to the focal length (f).
do = f = 75 cm
The distance between the object and the image is the sum of the object distance and the image distance:
Distance = do + di = 75 cm + 60 cm = 135 cm
Therefore, the object and image are approximately 135 cm apart.
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Real images formed by a spherical mirror are always: A. on the side of the mirror opposite the source B. on the same side of the mirror as the source but closer to the mirror than the source C. on the same side of the mirror as the source but never any further from the mirror than the focal point D. on the same side of the mirror as the source but never any closer to the mirror than the focal point E. none of the above
The correct option is D. on the same side of the mirror as the source but never any closer to the mirror than the focal point.
A spherical mirror is a mirror that has a spherical shape like a ball. A spherical mirror is either concave or convex. The mirror has a center of curvature (C), a radius of curvature (R), and a focal point (F).
When a ray of light traveling parallel to the principal axis hits a concave mirror, it is reflected through the focal point. It forms an image that is real, inverted, and magnified when the object is placed farther than the focal point. If the object is placed at the focal point, the image will be infinite.
When the object is placed between the focal point and the center of curvature, the image will be real, inverted, and magnified, while when the object is placed beyond the center of curvature, the image will be real, inverted, and diminished.
In the case of a convex mirror, when a ray of light parallel to the principal axis hits the mirror, it is reflected as if it came from the focal point. The image that is formed by a convex mirror is virtual, upright, and smaller than the object.
The image is always behind the mirror, and the image distance (di) is negative. Therefore, the correct option is D. on the same side of the mirror as the source but never any closer to the mirror than the focal point.
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two converging lenses each with focal lengths f are a distance 4f apart. An object is placed at distance 2f. Determine the position and type of the final image. Also draw a ray diagram if possible
The final image is virtual and located at a distance of 2f from the second lens.
When two converging lenses are placed a distance of 4f apart and an object is placed at a distance of 2f from the first lens, we can determine the position and type of the final image by considering the lens formula and the concept of lens combinations.
Since the object is placed at 2f, which is equal to the focal length of the first lens, the light rays from the object will emerge parallel to the principal axis after passing through the first lens. These parallel rays will then converge towards the second lens.
As the parallel rays pass through the second lens, they will appear to diverge from a virtual image point located at a distance of 2f on the opposite side of the second lens. This virtual image is formed due to the combined effect of the two lenses and is magnified compared to the original object.
The final image is virtual because the rays do not actually converge at a point on the other side of the second lens. Instead, they appear to diverge from the virtual image point.
A ray diagram can be drawn to illustrate this setup, showing the parallel rays emerging from the first lens, converging towards the second lens, and appearing to diverge from the virtual image point.
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Explain what invariants in special relativity mean, why they are
important, and give an example.
Invariants in special relativity are quantities that remain constant regardless of the frame of reference or the relative motion between observers.
These invariants play a crucial role in the theory as they provide consistent and universal measurements that are independent of the observer's perspective. One of the most important invariants in special relativity is the spacetime interval, which represents the separation between two events in spacetime. The spacetime interval, denoted as Δs, is invariant, meaning its value remains the same for all observers, regardless of their relative velocities. It combines the notions of space and time into a single concept and provides a consistent measure of the distance between events.
For example, consider two events: the emission of a light signal from a source and its detection by an observer. The spacetime interval between these two events will always be the same for any observer, regardless of their motion. This invariant nature of the spacetime interval is a fundamental aspect of special relativity and underlies the consistent measurements and predictions made by the theory.
Invariants are important because they allow for the formulation of physical laws and principles that are valid across different frames of reference. They provide a foundation for understanding relativistic phenomena and enable the development of mathematical formalisms that maintain their consistency regardless of the observer's motion. Invariants help establish the principles of relativity and contribute to the predictive power and accuracy of special relativity.
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Suppose the magnetic field along an axis of a cylindrical region is given by B₂ = Bo(1 + vz²) sin wt, where is a constant. Suppose the o-component of B is zero, that is B = 0. (a) Calculate the radial B,(s, z) using the divergence of the magnetic field. (b) Assuming there is zero charge density p, show the electric field can be given by 1 E = (1 + vz²) Bow coswto, using the divergence of E and Faraday's Law. (c) Use Ampere-Maxwell's Equation to find the current density J(s, z).
a) The radial component of the magnetic field is:
B_r = Bo(2vwtz + C₁)
b) The radial component of the electric field is:
E_r = -2v Bow (vz/wt) sin(wt) - 2v Bow C₂
Comparing this with the given expression (1 + vz²) Bow cos(wt), we can equate the corresponding terms:
-2v Bow (vz/wt) sin(wt) = 0
This implies that either v = 0 or w = 0. However, since v is given as a constant, it must be that w = 0.
c) The current density J:
J = ε₀ Bow (1 + vz²) sin(wt)
Explanation:
To solve the given problem, we'll go step by step:
(a) Calculate the radial B(r, z) using the divergence of the magnetic field:
The divergence of the magnetic field is given by:
∇ · B = 0
In cylindrical coordinates, the divergence can be expressed as:
∇ · B = (1/r) ∂(rB_r)/∂r + ∂B_z/∂z + (1/r) ∂B_θ/∂θ
Since B does not have any θ-component, we have:
∇ · B = (1/r) ∂(rB_r)/∂r + ∂B_z/∂z = 0
We are given that B_θ = 0, and the given expression for B₂ can be written as B_z = Bo(1 + vz²) sin(wt).
Let's find B_r by integrating the equation above:
∂B_z/∂z = Bo ∂(1 + vz²)/∂z sin(wt) = Bo(2v) sin(wt)
Integrating with respect to z:
B_r = Bo(2v) ∫ sin(wt) dz
Since the integration of sin(wt) with respect to z gives us wtz + constant, we can write:
B_r = Bo(2v) (wtz + C₁)
where C₁ is the constant of integration.
So, the radial component of the magnetic field is:
B_r = Bo(2vwtz + C₁)
(b) Assuming zero charge density p, show the electric field can be given by E = (1 + vz²) Bow cos(wt) using the divergence of E and Faraday's Law:
The divergence of the electric field is given by:
∇ · E = ρ/ε₀
Since there is zero charge density (ρ = 0), we have:
∇ · E = 0
In cylindrical coordinates, the divergence can be expressed as:
∇ · E = (1/r) ∂(rE_r)/∂r + ∂E_z/∂z + (1/r) ∂E_θ/∂θ
Since E does not have any θ-component, we have:
∇ · E = (1/r) ∂(rE_r)/∂r + ∂E_z/∂z = 0
Let's find E_r by integrating the equation above:
∂E_z/∂z = ∂[(1 + vz²) Bow cos(wt)]/∂z = -2vz Bow cos(wt)
Integrating with respect to z:
E_r = -2v Bow ∫ vz cos(wt) dz
Since the integration of vz cos(wt) with respect to z gives us (vz/wt) sin(wt) + constant, we can write:
E_r = -2v Bow [(vz/wt) sin(wt) + C₂]
where C₂ is the constant of integration.
So, the radial component of the electric field is:
E_r = -2v Bow (vz/wt) sin(wt) - 2v Bow C₂
Comparing this with the given expression (1 + vz²) Bow cos(wt), we can equate the corresponding terms:
-2v Bow (vz/wt) sin(wt) = 0
This implies that either v = 0 or w = 0. However, since v is given as a constant, it must be that w = 0.
(c) Use Ampere-Maxwell's Equation to find the current density J(s, z):
Ampere-Maxwell's equation in differential form is given by:
∇ × B = μ₀J + μ₀ε₀ ∂E/∂t
In cylindrical coordinates, the curl of B can be expressed as:
∇ × B = (1/r) ∂(rB_θ)/∂z - ∂B_z/∂θ + (1/r) ∂(rB_z)/∂θ
Since B has no θ-component, we can simplify the equation to:
∇ × B = (1/r) ∂(rB_z)/∂θ
Differentiating B_z = Bo(1 + vz²) sin(wt) with respect to θ, we get:
∂B_z/∂θ = -Bo(1 + vz²) w cos(wt)
Substituting this back into the curl equation, we have:
∇ × B = (1/r) ∂(rB_z)/∂θ = -Bo(1 + vz²) w (1/r) ∂(r)/∂θ sin(wt)
∇ × B = -Bo(1 + vz²) w ∂r/∂θ sin(wt)
Since the cylindrical region does not have an θ-dependence, ∂r/∂θ = 0. Therefore, the curl of B is zero:
∇ × B = 0
According to Ampere-Maxwell's equation, this implies:
μ₀J + μ₀ε₀ ∂E/∂t = 0
μ₀J = -μ₀ε₀ ∂E/∂t
Taking the time derivative of E = (1 + vz²) Bow cos(wt), we get:
∂E/∂t = -Bow (1 + vz²) sin(wt)
Substituting this into the equation above, we have:
μ₀J = μ₀ε₀ Bow (1 + vz²) sin(wt)
Finally, dividing both sides by μ₀, we obtain the current density J:
J = ε₀ Bow (1 + vz²) sin(wt)
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The Hamiltonian for a two-particle system is given by H = w(L12 + L22) + L₁ L₁. L2 ħ + w/h L₁, L2 denote the angular momentum of each particle. (a) Find the energy eigenvalues and the corresponding eigenstates. (b) The system is prepared to have l₁ = 1, l₂ = 2, m₁ = 0 and m₂ = 1. Find all the energy eigenvalues it can have and also find the probability to measure each energy eigenvalue.
The value is:
(a) The energy eigenvalues of the two-particle system are given by E = 2w(l₁(l₁+1) + l₂(l₂+1) - l₃(l₃+1)), where l₁, l₂, and l₃ are the quantum numbers associated with the angular momentum of each particle.
(b) For the specific case of l₁ = 1, l₂ = 2, m₁ = 0, and m₂ = 1, the possible energy eigenvalues are E = 12w, E = 8w, and E = 4w, corresponding to l₃ = 1, l₃ = 2, and l₃ = 3, respectively.
To find the energy eigenvalues and corresponding eigenstates, we need to solve the Schrödinger equation for the given Hamiltonian.
(a) Energy Eigenvalues and Eigenstates:
The Hamiltonian for the two-particle system is given by:
H = w(L₁² + L₂²) + (L₁ . L₂) ħ + (w/ħ) L₁ . L₂
To find the energy eigenvalues and eigenstates, we need to solve the Schrödinger equation:
H |ψ⟩ = E |ψ⟩
Let's assume that the eigenstate can be expressed as a product of individual angular momentum eigenstates:
|ψ⟩ = |l₁, m₁⟩ ⊗ |l₂, m₂⟩
where |l₁, m₁⟩ represents the eigenstate of the angular momentum of particle 1 and |l₂, m₂⟩ represents the eigenstate of the angular momentum of particle 2.
Substituting the eigenstate into the Schrödinger equation, we get:
H |l₁, m₁⟩ ⊗ |l₂, m₂⟩ = E |l₁, m₁⟩ ⊗ |l₂, m₂⟩
Expanding the Hamiltonian, we have:
H = w(L₁² + L₂²) + (L₁ . L₂) ħ + (w/ħ) L₁ . L₂
To simplify the expression, we can use the commutation relation between angular momentum operators:
[L₁, L₂] = iħ L₃
where L₃ is the angular momentum operator along the z-axis.
Using this relation, we can rewrite the Hamiltonian as:
H = w(L₁² + L₂²) + (L₁ . L₂) ħ + (w/ħ) L₁ . L₂
= w(L₁² + L₂²) + (L₁ . L₂) ħ + (w/ħ) (1/2)(L₁² + L₂² - L₃² - ħ²)
Substituting the eigenstates into the Schrödinger equation and applying the Hamiltonian, we get:
E |l₁, m₁⟩ ⊗ |l₂, m₂⟩ = w(l₁(l₁+1) + l₂(l₂+1) + (l₁(l₁+1) + l₂(l₂+1) - l₃(l₃+1) - 1/4) + w(l₁(l₁+1) + l₂(l₂+1) - l₃(l₃+1) - 1/4)) ħ² |l₁, m₁⟩ ⊗ |l₂, m₂⟩
Simplifying the equation, we obtain:
E = 2w(l₁(l₁+1) + l₂(l₂+1) - l₃(l₃+1))
The energy eigenvalues depend on the quantum numbers l₁, l₂, and l₃.
(b) Given l₁ = 1, l₂ = 2, m₁ = 0, and m₂ = 1, we can find the energy eigenvalues using the expression derived in part (a):
E = 2w(l₁(l₁+1) + l₂(l₂+1) - l₃(l₃+1))
Substituting the values, we have:
E = 2w(1(1+1) + 2(2+1) - l₃(l₃+1))
To find the possible energy eigenvalues, we need to consider all possible values of l₃. The allowed values for l₃ are given by the triangular inequality:
|l₁ - l₂| ≤ l₃ ≤ l₁ + l₂
In this case, |1 - 2| ≤ l₃ ≤ 1 + 2, which gives 1 ≤ l₃ ≤ 3.
Therefore, the possible energy eigenvalues for this system are obtained by substituting different values of l₃:
For l₃ = 1:
E = 2w(1(1+1) + 2(2+1) - 1(1+1))
= 2w(6) = 12w
For l₃ = 2:
E = 2w(1(1+1) + 2(2+1) - 2(2+1))
= 2w(4) = 8w
For l₃ = 3:
E = 2w(1(1+1) + 2(2+1) - 3(3+1))
= 2w(2) = 4w
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