Given the data generated in Matlab asn = 100000;x = 10 + 10*rand (n,1);To plot p(x), a histogram can be plotted for the values of x. The histogram can be normalised by multiplying the frequency of each bin with the bin width and dividing by the total number of values of x.
The program to plot p(x) is shown below:```
% define the bin width
binWidth = 0.1;
% compute the histogram
[counts, edges] = histcounts(x, 'BinWidth', binWidth);
% normalise the histogram
p = counts/(n*binWidth);
% plot the histogram
bar(edges(1:end-1), p, 'hist')
xlabel('x')
ylabel('p(x)')
```
The `histcounts` function is used to compute the histogram of `x` with a bin width of `binWidth`. The counts of values in each bin are returned in the vector `counts`, and the edges of the bins are returned in the vector `edges`. The normalised histogram is then computed by dividing the counts with the total number of values of `x` multiplied by the bin width.
Finally, the histogram is plotted using the `bar` function, with the edges of the bins as the x-coordinates and the normalised counts as the y-coordinates. The plot of `p(x)` looks like the following: Histogram plot.
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The pressure gradient at a given moment is 10 mbar per 1000 km.
The air temperature is 7°C, the pressure is 1000 mbar and the
latitude is 30°. Calculate the pressure gradient
Select one:
a. 0.0011 P
The pressure gradient force is -0.0122 N/m³.
Given, The pressure gradient at a given moment is 10 mbar per 1000 km. The air temperature is 7°C, the pressure is 1000 mbar, and the latitude is 30°.
Formula used: Pressure gradient force is given by, Gradient pressure [tex]force = -ρgδh[/tex]
Where,ρ is the density of air,δh is the height difference, g is the acceleration due to gravity
The pressure gradient is given by,[tex]ΔP/Δx = -ρg[/tex]
Here, Δx = 1000 km
= 1000000m
[tex]ΔP = 10 mbar[/tex]
= 1000 N/m²
Temperature = 7°C
Pressure = 1000 mbar
Latitude = 30°
To calculate the pressure gradient force, first we need to calculate the air density.
To calculate the air density, use the formula,
[tex]ρ = P/RT[/tex]
Where, R = 287 J/kg.
KP = pressure = 1000 mbar = 100000 N/m²
T = Temperature = 7°C = 280 K
N = 273 + 7 K
= 280 K
ρ = 100000/(287*280) kg/m³
ρ = 1.247 kg/m³
Now, we can find the gradient force,
[tex]ΔP/Δx = -ρg[/tex]
ΔP = 10 mbar = 1000 N/m²
Δx = 1000 km = 1000000m
ρ = 1.247 kg/m³
g = 9.8 m/s²
ΔP/Δx = -(1.247*9.8)
ΔP/Δx = -0.0122 N/m³
Therefore, the pressure gradient force is -0.0122 N/m³.
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2 4. Solve the equation: (D² - 1)y= = ex +1
The equation to be solved is(D² - 1)y = ex + 1.To solve the given equation, we can follow these steps:Step 1: Write the given equation (D² - 1)y = ex + 1 as(D² - 1)y - ex = 1 .
Using the integrating factor e^(∫-dx), multiply both sides by e^(∫-dx) to obtaine^(∫-dx)(D² - 1)y - e^(∫-dx)ex = e^(∫-dx)Step 3: Recognize that the left side of the equation can be written asd/dx(e^(∫-dx)y') - e^(∫-dx)ex = e^(∫-dx)This simplifies to(e^(-x)y')' - e^(-x)ex = e^(-x).
This simplifies to-e^(-x)y' - e^(-x)ex + C1 = -e^(-x) + C2, where C1 and C2 are constants of integration.Step 5: Solve for y'.e^(-x)y' = -e^(-x) + C3, where C3 = C1 - C2.y' = -1 + Ce^x, where C = C3e^x. Integrate both sides with respect to x.∫y'dx = ∫(-1 + Ce^x)dxy = -x + Ce^x + C4, where C4 is a constant of integration.Therefore, the solution of the equation (D² - 1)y = ex + 1 is y = -x + Ce^x + C4.
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Question 4
a) (3 marks) Define thermal energy.
b) A steel pipe is used to transport water at 75°C. The pipe has an external diameter of 300mm and a wall thickness of 15mm. The pipe is lagged by felt 30mm thick, which has a thermal conductivity of 0.05W/m°C. Given:
• Temperature of the air at the outer surface, Tout = 20°C . Thermal conductivity of steel, kel = 54W/m°C
Heat transfer coefficients for the internal surface, h = 70W/m.°C
Heat transfer coefficients for the external surface, hout 22W/m.°C
• Length of pipe, L, = 1m JANUARY 2022 CONFIDENTIAL
i. Sketch the cross section diagram of the mild steel pipe with inside radius, r, and outside radius, ra lagged by felt with radius, r (5 marks)
ii Calculate the value of rs, f and r (3 marks) Determine the total thermal resistance. iv. Calculate the heat loss per unit length of the pipe. (10 marks) (4 marks) BMB22303 Page 3 of 4
a) Definition of thermal energy Thermal energy is the energy that is created from the motion of particles that exist within matter. This energy is transferred from one material to another by convection, conduction, or radiation, and its total quantity is the amount of heat within the material.
b) Solution i. Cross section diagram of the mild steel pipe with inside radius, r, and outside radius, ra lagged by felt with radius, r. ii. Calculation of the value of rs, f and r. Inside radius, r = ra − 2 × thickness of pipe = 300/2 - 2 × 15 = 135mm = 0.135mRadius of felt, rf = ra + f = 0.300 + 0.030 = 0.330mTotal radius, rs = r + rf = 0.330 + 0.135 = 0.465miii.
Calculation of the total thermal resistance. Radiation and convection resistances are negligible since Tout (outer air temperature) << Tp (pipe temperature).Using a total of six resistances, the thermal resistance per unit length of the pipe can be determined as:
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. as outlined below, a 2-kg bob is compressed 60-cm against a 50 n/m spring while on the other side a 3-kg block is placed 4-m up along a 30 degree incline. both objects are then released from rest. assuming all surfaces are frictionless: a. what will be the velocity of each object before they collide? (10pts) b. if the collision between the objects is elastic, what will be the velocity of each object after the collision? (10pts) c. if either (or both) of the objects moves toward the spring after the collision, determine how much the spring will be compressed by the object(s) (10pts) d. if either (or both) of the objects moves toward the incline after the collision, determine how far up the incline the object(s) will travel (10pts)
a. To determine the velocity of each object before they collide, we can apply conservation of mechanical energy.
For the 2-kg bob compressed against the spring, the potential energy stored in the spring when compressed is given by:
PE_spring = 0.5 * k * x^2,
where k is the spring constant (50 N/m) and x is the compression distance (0.6 m).
PE_spring = 0.5 * 50 N/m * (0.6 m)^2 = 9 J
The potential energy is converted entirely into kinetic energy before the collision:
KE_bob = PE_spring = 9 J
Using the formula for kinetic energy:
KE = 0.5 * m * v^2,
where m is the mass and v is the velocity, we can solve for the velocity of the 2-kg bob:
9 J = 0.5 * 2 kg * v^2
v^2 = 9 J / 1 kg
v = √(9 m^2/s^2) = 3 m/s
Therefore, the velocity of the 2-kg bob before the collision is 3 m/s.
For the 3-kg block on the incline, we can determine its velocity using the conservation of potential and kinetic energy.
The potential energy at the top of the incline is given by:
PE_top = m * g * h,
where m is the mass (3 kg), g is the acceleration due to gravity (9.8 m/s^2), and h is the height (4 m).
PE_top = 3 kg * 9.8 m/s^2 * 4 m = 117.6 J
The potential energy is converted into kinetic energy:
KE_block = PE_top = 117.6 J
Using the formula for kinetic energy, we can solve for the velocity of the 3-kg block:
117.6 J = 0.5 * 3 kg * v^2
v^2 = 117.6 J / 1.5 kg
v = √(78.4 m^2/s^2) ≈ 8.85 m/s
Therefore, the velocity of the 3-kg block before the collision is approximately 8.85 m/s.
b. If the collision between the objects is elastic, the total momentum before the collision is equal to the total momentum after the collision.
Total momentum before the collision:
P_before = m1 * v1 + m2 * v2,
where m1 and m2 are the masses, and v1 and v2 are the velocities.
P_before = (2 kg * 3 m/s) + (3 kg * 8.85 m/s)
P_before ≈ 36.55 kg·m/s
Since the collision is elastic, the total momentum after the collision remains the same.
Total momentum after the collision:
P_after = (2 kg * v1') + (3 kg * v2'),
where v1' and v2' are the velocities after the collision.
We need to solve this equation for v1' and v2'. More information is required about the nature of the collision (head-on or at an angle) to determine the specific velocities after the collision.
c. To determine how much the spring will be compressed by the object(s) after the collision, we need to consider the conservation of mechanical energy.
The total mechanical energy after the collision is equal to the sum of potential and kinetic energy:
Total Energy_after = PE_spring + KE_bob,
where PE_spring is the potential energy stored in the spring and KE_bob is the kinetic energy of the 2-kg
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1. What are the three 'functions' or 'techniques' of
statistics (p. 105, first part of ch. 6)? How do they
differ?
2. What’s the difference between a sample and a
population in statistics?
3. What a
1. The three functions or techniques of statistics are
Descriptive Statistics: This involves collecting, organizing, summarizing, and presenting data in a meaningful way. Descriptive statistics provide a clear and concise summary of the main features of a dataset, such as measures of central tendency (mean, median, mode) and measures of variability (range, standard deviation).
Inferential Statistics: This involves making inferences or drawing conclusions about a population based on a sample. Inferential statistics use probability theory to analyze sample data and make predictions or generalizations about the larger population from which the sample is drawn. It helps in testing hypotheses, estimating parameters, and making predictions.
Hypothesis Testing: This is a specific application of inferential statistics. Hypothesis testing involves formulating a null hypothesis and an alternative hypothesis, collecting sample data, and using statistical tests to determine whether there is enough evidence to reject the null hypothesis in favor of the alternative hypothesis. It helps in making decisions and drawing conclusions based on available evidence.
2. In statistics, a population refers to the entire group or set of individuals, objects, or events that the researcher is interested in studying. It includes every possible member of the group. For example, if we want to study the average height of all adults in a country, the population would consist of every adult in that country
On the other hand, a sample is a subset or a smaller representative group selected from the population. It is used to gather data and make inferences about the population. In the previous example, instead of measuring the height of every adult in the country, we can select a sample of adults, measure their heights, and then generalize the findings to the entire population.
The key difference between a population and a sample is the scope and size of the group being studied. The population includes all individuals or objects of interest, while a sample is a smaller subset selected from the population to represent it.
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(10 marks) Suppose (x.f) = A(x - x³)e-it/h, Find V(x) such that the equation is satisfied.
To find the potential function V(x) such that the equation (x.f) = A(x - x³)e^(-it/h) is satisfied, we can use the relationship between the potential and the wave function. In quantum mechanics, the wave function is related to the potential through the Hamiltonian operator.
Let's start by finding the wave function ψ(x) from the given equation. We have:
(x.f) = A(x - x³)e^(-it/h)
In quantum mechanics, the momentmomentumum operator p is related to the derivative of the wave function with respect to position:
p = -iħ(d/dx)
We can rewrite the equation as:
p(x.f) = -iħ(x - x³)e^(-it/h)
Applying the momentum operator to the wave function:
- iħ(d/dx)(x.f) = -iħ(x - x³)e^(-it/h)
Expanding the left-hand side using the product rule:
- iħ((d/dx)(x.f) + x(d/dx)f) = -iħ(x - x³)e^(-it/h)
Differentiating x.f with respect to x:
- iħ(x + xf' + f) = -iħ(x - x³)e^(-it/h)
Now, let's compare the coefficients of each term:
- iħ(x + xf' + f) = -iħ(x - x³)e^(-it/h)
From this comparison, we can see that:
x + xf' + f = x - x³
Simplifying this equation:
xf' + f = -x³
This is a first-order linear ordinary differential equation. We can solve it by using an integrating factor. Let's multiply the equation by x:
x(xf') + xf = -x⁴
Now, rearrange the terms:
x²f' + xf = -x⁴
This equation is separable, so we can divide both sides by x²:
f' + (1/x)f = -x²
This is a first-order linear homogeneous differential equation. To solve it, we can use an integrating factor μ(x) = e^(∫(1/x)dx).
Integrating (1/x) with respect to x:
∫(1/x)dx = ln|x|
So, the integrating factor becomes μ(x) = e^(ln|x|) = |x|.
Multiply the entire differential equation by |x|:
|xf' + f| = |-x³|
Splitting the absolute value on the left side:
xf' + f = -x³, if x > 0
-(xf' + f) = -x³, if x < 0
Solving the differential equation separately for x > 0 and x < 0:
For x > 0:
xf' + f = -x³
This is a first-order linear homogeneous differential equation. We can solve it by using an integrating factor. Let's multiply the equation by x:
x(xf') + xf = -x⁴
Now, rearrange the terms:
x²f' + xf = -x⁴
This equation is separable, so we can divide both sides by x²:
f' + (1/x)f = -x²
The integrating factor μ(x) = e^(∫(1/x)dx) = |x| = x.
Multiply the entire differential equation by x:
xf' + f = -x³
This equation can be solved using standard methods for first-order linear differential equations. The general solution to this equation is:
f(x) = Ce^(-x²
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Problem 2: Lagrangian Mechanics (50 points) Consider a particle of mass m constrained to move on the surface of a cone of half-angle a as shown in the figure below. (a) Write down all constraint relat
The motion of a particle of mass m constrained to move on the surface of a cone of half-angle a can be represented using the Lagrangian mechanics.
The following constraints relating to the motion of the particle must be taken into account. Let r denote the distance between the particle and the apex of the cone, and let θ denote the angle that r makes with the horizontal plane. Then, the constraints can be written as follows:
[tex]r2 = z2 + h2z[/tex]
= r tan(α)cos(θ)h
= r tan(α)sin(θ)
These equations show the geometrical constraints, which constrain the motion of the particle on the surface of the cone. To formulate the Lagrangian of the particle, we need to consider the kinetic and potential energy of the particle.
The kinetic energy can be written as
[tex]T = ½ m (ṙ2 + r2 ṫheta2)[/tex],
and the potential energy can be written as
V = m g h.
The Lagrangian can be written as L = T - V.
The equations of motion of the particle can be obtained using the Euler-Lagrange equation, which states that
[tex]d/dt(∂L/∂qdot) - ∂L/∂q = 0,[/tex]
where q represents the generalized coordinates. For the particle moving on the surface of the cone, the generalized coordinates are r and θ.
By applying the Euler-Lagrange equation, we can obtain the following equations of motion:
[tex]r d/dt(rdot) - r theta2 = 0[/tex]
[tex]r2 theta dot + 2 rdot r theta = 0[/tex]
These equations describe the motion of the particle on the surface of the cone, subject to the geometrical constraints.
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Prepare a diagonal scale of RF=1/6250 to read up to 1 kilometer and to read meters on it. Also show a length of 666 meters on it.
Prepare a diagonal scale of RF=1/6250 to read up to 1 kilometer and meters, marking a length of 666 meters on it.
To prepare a diagonal scale of RF=1/6250 to read up to 1 kilometer and to read meters on it, follow these steps:
1. Determine the total length of the scale: Since the RF is 1/6250, 1 kilometer (1000 meters) on the scale should correspond to 6250 units. Therefore, the total length of the scale will be 6250 units.
2. Divide the total length of the scale into equal parts: Divide the total length (6250 units) into convenient equal parts. For example, you can divide it into 25 parts, making each part 250 units long.
3. Mark the main divisions: Mark the main divisions on the scale at intervals of 250 units. Start from 0 and label each main division as 250, 500, 750, and so on, until 6250.
4. Determine the length for 1 kilometer: Since 1 kilometer should correspond to the entire scale length (6250 units), mark the endpoint of the scale as 1 kilometer.
5. Divide each main division into smaller divisions: Divide each main division (250 units) into 10 equal parts to represent meters. This means each smaller division will correspond to 25 units.
6. Mark the length of 666 meters: Locate the point on the scale that represents 666 meters and mark it accordingly. It should fall between the main divisions, approximately at the 2665 mark (2500 + 165).
By following these steps, you will have prepared a diagonal scale of RF=1/6250 that can read up to 1 kilometer and represent meters on it, with the length of 666 meters marked.
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i.
°F
warms up to
46°F
in
2
min while sitting in a room of temperature
72°F.
How warm will the drink be if left out for
15
min?
ii
An object of mass
20
kg is released from rest
3000
m above the
the drink will warm up to 58°F if left out for 15 minutes.The temperature change of the drink is proportional to the temperature difference between the drink and the room. Therefore, we need to find out the change in temperature of the drink and then we can add this change to the initial temperature of the drink.i. Change in temperature of drink in 2 min, ΔT = (46-30) = 16°F.
It means the temperature of the drink has increased by 16°F in 2 min.Time taken to increase the temperature by 1°F is, t = 2/16 = 0.125 min or 7.5 seconds. (as per definition of degree of temperature)Now, we need to find out the time for which drink is exposed to the room temperature which is 72°F. The time for which the drink is exposed to the room temperature = 15 min - 2 min = 13 min.Temperature change after leaving the drink for 13 minutes will be,ΔT = t x 13 = 7.5 x 13 = 97.5 seconds. (Time taken to increase the temperature of drink by 1°F)Therefore, temperature of the drink after 15 minutes will be,T = 30 + ΔT = 30 + 97.5 = 127.5°F ≈ 128°F.
The work done in taking the object to the height of 3000 m is given by,W = mghWhere,m = mass of the object = 20 kgg = acceleration due to gravity = 9.8 ms-2h = height = 3000 mNow,Work done, W = mgh= 20 × 9.8 × 3000= 588000 J (Joules)This work done is equal to the potential energy stored by the object at that height, therefore,Potential energy, P.E = mgh= 20 × 9.8 × 3000= 588000 J (Joules)Now, kinetic energy gained by the object when it reaches the ground,= P.E.= 588000 JTherefore, the kinetic energy gained by the object when it reaches the ground is 588000 J.
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Quantum mechanics:
Explain the concept of Ehrenfest’s Theorem and give the proofs
for the Ehrenfest equations.
Ehrenfest’s Theorem is a fundamental theorem in quantum mechanics that describes the behavior of expectation values for a time-dependent quantum system. It states that the time derivative of the expectation value of any observable Q in a system is given by the commutator of the observable with the Hamiltonian of the system, while the expectation value of the momentum changes in the same way as the time derivative of the position expectation value.
The theorem is of great significance in quantum mechanics, as it provides a way to relate the behavior of macroscopic systems to the underlying quantum mechanics.
Proofs for the Ehrenfest equations:
The Ehrenfest equations can be derived using the Heisenberg picture, which describes the time evolution of operators rather than the wavefunction of a system. The Heisenberg picture is related to the Schrodinger picture through the relation:
A(t) = e^(iHt/hbar) A e^(-iHt/hbar)
where A is an operator, H is the Hamiltonian, hbar is the reduced Planck constant.
To derive the Ehrenfest equations, we start by differentiating the Heisenberg equation of motion for the position operator x(t):
d/dt x(t) = i/hbar [H,x(t)]
where [H,x(t)] is the commutator of the Hamiltonian and the position operator. Using the chain rule, we can write:
d/dt x(t) = (dx/dt)(dt/dt) + (dx/dH) (dH/dt)
where the first term is the velocity of the particle and the second term is the force acting on the particle. Since the Hamiltonian is the total energy of the system, the force term is just the gradient of the potential energy:
F = - d/dx U(x)
where U(x) is the potential energy. We can write this as:
F = - d/dx
where is the expectation value of the Hamiltonian.
Thus, we have shown that the time derivative of the position expectation value is given by the expectation value of the momentum operator:
d/dt =
/m
where m is the mass of the particle. Similarly, we can show that the time derivative of the momentum expectation value is given by the expectation value of the force operator:
d/dt
= -
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Its four parts but one question please solve them all
Y Part A Find the magnitude of the net electric force exerted on a charge +Q, located at the center of the square, for the following arrangement of charge: the charges alternate in sign (+9,-9, +9,-g)
The magnitude of the net electric force exerted on the charge +Q at the center of the square is |k * Q² / r²| * 18.
To find the magnitude of the net electric force exerted on the charge +Q at the center of the square, we need to consider the individual electric forces between the charges and the charge +Q and then add them up vectorially.
Given:
Charge +Q at the center of the square.
Charges on the corners of the square: +9, -9, +9, -Q.
Let's label the charges on the corners as follows:
Top-left corner: Charge A = +9
Top-right corner: Charge B = -9
Bottom-right corner: Charge C = +9
Bottom-left corner: Charge D = -Q
The electric force between two charges is given by Coulomb's Law:
F = k * (|q₁| * |q₂|) / r²
where F is the electric force, k is the Coulomb's constant, q₁ and q₂ are the magnitudes of the charges, and r is the distance between them.
Now, let's calculate the net electric force exerted on the charge +Q:
1. The force exerted by Charge A on +Q:
F₁ = k * (|A| * |Q|) / r₁²
2. The force exerted by Charge B on +Q:
F₂ = k * (|B| * |Q|) / r₂²
3. The force exerted by Charge C on +Q:
F₃ = k * (|C| * |Q|) / r₃²
4. The force exerted by Charge D on +Q:
F₄ = k * (|D| * |Q|) / r₄²
Note: The distances r₁, r₂, r₃, and r₄ are all the same since the charges are located on the corners of the square.
The net electric force is the vector sum of these individual forces:
Net force = F₁ + F₂ + F₃ + F₄
Substituting the values and simplifying, we have:
Net force = (k * Q² / r²) * (|A| - |B| + |C| - |D|)
Since A = C = +9 and
B = D = -9, we can simplify further:
Net force = (k * Q² / r²) * (9 + 9 - 9 - (-9))
Net force = (k * Q² / r²) * (18)
The magnitude of the net electric force is given by:
|Net force| = |k * Q² / r²| * |18|
So, the magnitude of the net electric force exerted on the charge +Q at the center of the square is |k * Q² / r²| * 18.
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Match the material with its property. Metals
Ceramics
Composites
Polymers Semiconductors - Good electrical and thermal insulators
- Conductivity and weight can be tailored
- Poor electrical and thermal conductivity - The level of conductivity or resistivity can be controlled - low compressive strength
Metals - Conductivity and weight can be tailored, Ceramics - Good electrical and thermal insulators, Composites - The level of conductivity or resistivity can be controlled, Polymers - Poor electrical and thermal conductivity, Semiconductors - low compressive strength.
Metals: Metals are known for their good electrical and thermal conductivity. They are excellent conductors of electricity and heat, allowing for efficient transfer of these forms of energy.
Ceramics: Ceramics, on the other hand, are good electrical and thermal insulators. They possess high resistivity to the flow of electricity and heat, making them suitable for applications where insulation is required.
Composites: Composites are materials that consist of two or more different constituents, typically combining the properties of both. The conductivity and weight of composites can be tailored based on the specific composition.
Polymers: Polymers are characterized by their low conductivity, both electrical and thermal. They are poor electrical and thermal conductors.
Semiconductors: Semiconductors possess unique properties where their electrical conductivity can be controlled. They have an intermediate level of conductivity between conductors (metals) and insulators (ceramics).
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(b) A satellite is launched into an equatorial orbit such that it orbits the Earth exactly 8 times per day. If the orbit perigee height is 800 km, what is the value of apogee height? [Assume the radiu
The apogee height of the satellite's orbit is 41200 km. This is the value of the apogee height when the perigee height is 800 km and the satellite orbits the Earth eight times per day.
A satellite is placed in an equatorial orbit such that it revolves around the Earth eight times each day. The perigee height of the orbit is 800 km, and we have to determine the apogee height of the orbit. We'll use the fact that the time period of an object in an orbit can be calculated using Kepler's third law.
Kepler's third law is given as
T² = (4π²/GM) × a³,
where T is the time period of the object in orbit, G is the gravitational constant, M is the mass of the planet, and a is the semi-major axis of the orbit.
We know that the satellite completes one orbit in 1/8th of a day since it revolves around the Earth eight times each day. Therefore, its time period is given as
T = 1/8 days = 0.125 days.
We can plug in these values into Kepler's third law to find the semi-major axis of the orbit.
0.125² = (4π²/GM) × [(800 km + apogee height)/2]³
Simplifying this equation, we obtain:
apogee height + 800 km
= 42000 km
Therefore, the apogee height of the satellite's orbit is 41200 km. This is the value of the apogee height when the perigee height is 800 km and the satellite orbits the Earth eight times per day.
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Q30 (1 point) Which of the following releases the least energy? A main-sequence star. A spaceship entering Earth's atmosphere. A quasar.
Of the options provided, a main-sequence star releases the least energy. Main-sequence stars, including our Sun, undergo nuclear fusion in their cores, converting hydrogen into helium and releasing a substantial amount of energy in the process.
Main-sequence stars, including our Sun, undergo nuclear fusion in their cores, converting hydrogen into helium and releasing a substantial amount of energy in the process. While main-sequence stars emit a considerable amount of energy, their energy output is much lower compared to other celestial objects such as quasars or intense events like a spaceship entering Earth's atmosphere.
A spaceship entering Earth's atmosphere experiences intense friction and atmospheric resistance, generating a significant amount of heat energy. Quasars, on the other hand, are incredibly luminous objects powered by supermassive black holes at the centers of galaxies, releasing tremendous amounts of energy.
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A string oscillates according to the equation: y(x, t) (0.50 cm) sin)] cos (40ms ¹)t). What are the amplitude and speed of the wave?
The amplitude and speed of the wave are 0.50 cm and 40 m/s, respectively.
The equation for a string oscillating is given as:
y(x, t) = Asin(kx - ωt)
where
A is the amplitude
k is the wave number
x is the position along the string
t is the time
ω is the angular frequency.
Using this, we can find the amplitude and speed of the wave given by the equation
y(x, t) = (0.50 cm) sin(kx - ωt) cos (40ms-1 t).
Comparing this equation with the standard equation, we get:
Amplitude = A = 0.50 cm
Wave number, k = 1
Speed of the wave,
v = ω/kwhereω
= 40 ms-1v
= 40 ms-1/ 1
= 40 m/s
Therefore, the amplitude and speed of the wave are 0.50 cm and 40 m/s, respectively.
Note: In the given equation, the wave number, k = 1.
This is because the equation does not contain any information about the length of the string, or the distance between the oscillating points.
If we had more information about the string, we could have found the value of k.
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if an RER of 1.0 means that we are relying 100% on carbohydrate
oxidation, how it is that we end up measuring RERs above 1.0?
RER is known as Respiratory exchange ratio. if an RER of 1.0 means that we are relying 100% on carbohydrate oxidation, then we can't measure RERs above 1.0 for the whole body because it is not possible.
RER is known as Respiratory exchange ratio. It is the ratio of carbon dioxide produced by the body to the amount of oxygen consumed by the body. RER helps to determine the macronutrient mixture that the body is oxidizing. The RER for carbohydrates is 1.0, for fat is 0.7, and for protein, it is 0.8.
An RER above 1.0 means that the body is oxidizing more carbon dioxide and producing more oxygen. Therefore, it is not possible to measure an RER of more than 1.0.There are two possible reasons why we may measure RERs above 1.0.
Firstly, there may be an error in the measurement. Secondly, we may be measuring the RER of a very specific part of the body rather than the whole body. The respiratory quotient (RQ) for a particular organ can exceed 1.0, even though the RER of the whole body is not possible to exceed 1.0.
So, if an RER of 1.0 means that we are relying 100% on carbohydrate oxidation, then we can't measure RERs above 1.0 for the whole body because it is not possible.
Therefore, this statement is invalid.
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4. In the common collector amplifier circuit, which of the following options is the relationship between the input voltage and the output voltage? (10points) A. The output voltage > The input voltage
In the common collector amplifier circuit, the input voltage and output voltage are in-phase, and the output voltage is slightly less than the input voltage.
Explanation:
The relationship between the input voltage and the output voltage in the common collector amplifier circuit is that the input voltage and output voltage are in-phase, and the output voltage is slightly less than the input voltage.
This circuit is also known as the emitter-follower circuit because the emitter terminal follows the base input voltage.
This circuit provides a voltage gain that is less than one, but it provides a high current gain.
The output voltage is in phase with the input voltage, and the voltage gain of the circuit is less than one.
The output voltage is slightly less than the input voltage, which is why the common collector amplifier is also called an emitter follower circuit.
The emitter follower circuit provides high current gain, low output impedance, and high input impedance.
One of the significant advantages of the common collector amplifier is that it acts as a buffer for driving other circuits.
In conclusion, the relationship between the input voltage and output voltage in the common collector amplifier circuit is that the input voltage and output voltage are in-phase, and the output voltage is slightly less than the input voltage.
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Given that the resultant force of the three forces on the wheel borrow shown is zero, calculate the following knowing that W=300N. 450 mm J. [Select] [Select] [Select] [Select] 900 mm W 28⁰ 450 mm (
To calculate the given question, we have to use trigonometry as the weight is at an angle. Here are the steps to solve this problem:
Step 1: Find the horizontal component of the 450 mm force; it is given as 450 cos(28)
Step 2: Find the vertical component of the 450 mm force; it is given as 450 sin(28).
Step 3: As the resultant force is zero, the sum of horizontal components of the three forces should also be zero. Thus:450 cos(28) + T cos(20) - R = 0Step 4:
The sum of vertical components of the three forces should also be zero. Thus:3[tex]00 + 450 sin(28) - T sin(20) = 0[/tex]
Step 5: Calculate the distance D, which is equal to 900 mm - J
Step 6:
The moment of force of 450 N force, taking the pivot as the wheel axle, will be:450 sin(28) × 450/1000
Step 7: The moment of force of T, taking the pivot as the wheel axle, will be: T sin(20) × D/1000
Step 8: The moment of force of R, taking the pivot as the wheel axle, will be:
R × 300/1000Step 9: As the moment of force is balanced, then the sum of moments should be zero, which means[tex]450 sin(28) × 450/1000 + T sin(20) × D/1000 - R × 300/1000 = 0[/tex]
Step 10:Finally, we can solve the equations to find the unknowns. From equation (3):R = 450 cos(28) + T cos(20)and from equation (4):T sin(20) = 300 - 450 sin(28)Substitute this into equation (3):
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2. If A is hermitian, show that (A²) ≥ 0. To do show, consider an arbitrary quantum state |ø). Then, (A²) = (q|A²|4). Also use the fact that (A|q))* = (q|A† = (Aq]. If necessary, use the fact
Consider an arbitrary quantum state |ø) . A Hermitian operator is a linear operator that satisfies the Hermitian conjugate property, i.e., A†=A. In other words, the Hermitian conjugate of the operator A is the same as the original operator A.
The operator A² is also Hermitian. A Hermitian operator has real eigenvalues, and its eigenvectors form an orthonormal basis.
For any Hermitian operator A, (A²) ≥ 0.
Let us consider an arbitrary quantum state |ø).Therefore,(A²)=|q|A²|ø>²=q*A²|ø>Using the fact that (A|q))*=(q|A†)
= (Aq), we can write q*A²|ø> as (A†q)*Aq*|ø>.
Since A is Hermitian,
A = A†. Thus, we can replace A† with A. Hence, q*A²|ø>=(Aq)*Aq|ø>
Since the operator A is Hermitian, it has real eigenvalues.
Therefore, the matrix representation of A can be diagonalized by a unitary matrix U such that U†AU=D, where D is a diagonal matrix with the eigenvalues on the diagonal.
Then, we can write q*A²|ø> as q*U†D U q*|ø>.Since U is unitary, U†U=UU†=I.
Therefore, q*A²|ø> can be rewritten as (Uq)* D(Uq)*|ø>.
Since Uq is just another quantum state, we can replace it with |q).
Therefore, q*A²|ø>
=(q|D|q)|ø>.
Since D is diagonal, its diagonal entries are just the eigenvalues of A.
Since A is Hermitian, its eigenvalues are real.
Therefore, (q|D|q) ≥ 0. Thus, (A²) ≥ 0.
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Suppose you are interested in the causal relationship between x and y, and you are aware that z might be related to both x and y. What should you do to obtain the best estimate of the x-->y causal eff
To obtain the best estimate of the x-->y causal effect, you should first adjust for z. Adjustment for z will decrease the bias in the estimate of the effect of x on y. You should also be certain that z is measured accurately.
This is because any inaccuracies in the measurement of z may result in an inaccurate adjustment. Furthermore, if there are any unmeasured confounders, the estimates of the effect of x on y will be biased. Therefore, you should make every effort to obtain accurate and complete data on all relevant variables when conducting causal research. When you're interested in the causal relationship between x and y, and you know that z may be related to both x and y, you should adjust for z to obtain the best estimate of the x-->y causal effect. Adjustment for z will minimize bias in the estimate of the effect of x on y. You should also ensure that z is measured accurately, as any inaccuracies in the measurement of z may result in an incorrect adjustment.
It's critical to obtain accurate and complete data on all relevant variables when conducting causal research because if there are any unmeasured confounders, the estimates of the effect of x on y will be biased. Unmeasured confounders are variables that influence both the independent and dependent variables, and they're unknown or unmeasured. It's challenging to control for confounding when unmeasured confounders are present, which may lead to biased causal effect estimates. Adjustment for confounding variables is an important aspect of causal inference, and it is frequently necessary when studying causal effects. When it comes to causal inferences, identifying confounding variables is critical to ensure accurate conclusions. Researchers should strive to recognize and account for potential confounders when conducting causal research.
To obtain the best estimate of the x-->y causal effect, you should adjust for z, which will reduce bias in the estimate of the effect of x on y. If there are any unmeasured confounders, the estimates of the effect of x on y will be biased. Therefore, it's critical to obtain accurate and complete data on all relevant variables when conducting causal research. Adjustment for confounding variables is a crucial aspect of causal inference, and identifying confounding variables is crucial to ensure accurate conclusions.
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17. Consider a thin, isolated, conducting, spherical shell that is uniformly charged to a constant charge density o. How much work does it take to move a small positive test charge qo (a) from the sur
The work done to move a small positive test charge qo from the surface of a charged spherical shell with charge density o to a distance r away is qo * kQ(1/R - 1/r). The work is positive, indicating that we need to do work to move the test charge against the electric field.
To move a small positive test charge qo from the surface of the sphere to a distance r away from the sphere, we need to do work against the electric field created by the charged sphere. The work done is equal to the change in potential energy of the test charge as it is moved against the electric field.
The potential energy of a charge in an electric field is given by:
U = qV
where U is the potential energy, q is the charge, and V is the electric potential (also known as voltage).
The electric potential at a distance r away from a charged sphere of radius R and charge Q is given by:
V = kQ*(1/r - 1/R)
where k is Coulomb's constant.
At the surface of the sphere, r = R, so the electric potential is:
V = kQ/R
Therefore, the potential energy of the test charge at the surface of the sphere is:
U_i = qo * (kQ/R)
At a distance r away from the sphere, the electric potential is:
V = kQ*(1/r - 1/R)
Therefore, the potential energy of the test charge at a distance r away from the sphere is:
U_f = qo * (kQ/R - kQ/r)
The work done to move the test charge from the surface of the sphere to a distance r away is equal to the difference in potential energy:
W = U_f - U_i
Substituting the expressions for U_i and U_f, we get:
W = qo * (kQ/R - kQ/r - kQ/R)
Simplifying, we get:
W = qo * kQ(1/R - 1/r)
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Light of frequency fis incident on a metal surface. The work function of the metal is p. Which of the following is the maximum kinetic energy of the electrons emitted from the surface? Select one: O a. hf-p O b. (h/e)(p-1)- OC None of them. O d. (h/e)(f-p) O e. p-hf
The maximum kinetic energy of the electrons emitted from the surface is given by (hf − p), where h is Planck's constant, f is the frequency of the light, and p is the work function of the metal.
When light of frequency f is incident on a metal surface, the energy of the incident photon is given by E = hf, where h is Planck's constant. If this energy is greater than the work function of the metal, p, then electrons will be emitted from the surface with a kinetic energy given by
KE = E − p = hf − p.
The maximum kinetic energy of the electrons emitted from the surface is obtained when the incident light has the highest possible frequency, which is given by
fmax = c/λmin,
where c is the speed of light and λmin is the minimum wavelength of light that can eject electrons from the surface, given by λmin = h/p. The maximum kinetic energy of the electrons emitted from the surface is thus given by
KEmax = hfmax − p = hc/λmin − p = hc(p/h) − p = (h/e)(p − 1),
where e is the elementary charge of an electron. Therefore, the correct option is (h/e)(p − 1).Main answer: The maximum kinetic energy of the electrons emitted from the surface is given by (hf − p), where h is Planck's constant, f is the frequency of the light, and p is the work function of the metal. The maximum kinetic energy of the electrons emitted from the surface is obtained when the incident light has the highest possible frequency, which is given by fmax = c/λmin, where c is the speed of light and λmin is the minimum wavelength of light that can eject electrons from the surface, given by λmin = h/p.The maximum kinetic energy of the electrons emitted from the surface is thus given by KEmax = hfmax − p = hc/λmin − p = hc(p/h) − p = (h/e)(p − 1),
where e is the elementary charge of an electron. The maximum kinetic energy of the electrons emitted from the surface is (h/e)(p − 1).
When a metal is illuminated with light of a certain frequency, it emits electrons. The energy required to eject an electron from a metal surface, known as the work function, is determined by the metal's composition. Planck's constant, h, and the frequency of the incoming light, f, are used to calculate the energy of individual photons in the light incident on the metal surface, E = hf.If the energy of a single photon is less than the work function, p, no electrons are emitted because the photons do not have sufficient energy to overcome the work function's barrier. Photons with energies greater than the work function, on the other hand, will eject electrons from the surface of the metal. The ejected electrons will have kinetic energy equal to the energy of the incoming photon minus the work function of the metal,
KE = hf - p.
The maximum kinetic energy of the emitted electrons is achieved when the incoming photons have the highest possible frequency, which corresponds to the minimum wavelength, λmin, of photons that can eject electrons from the metal surface.
KEmax = hfmax - p = hc/λmin - p = hc(p/h) - p = (h/e)(p - 1), where e is the elementary charge of an electron. This equation shows that the maximum kinetic energy of the ejected electrons is determined by the work function and Planck's constant, with higher work functions requiring more energy to eject an electron and resulting in lower maximum kinetic energies. The maximum kinetic energy of the electrons emitted from the surface is (h/e)(p - 1). The energy required to eject an electron from a metal surface, known as the work function, is determined by the metal's composition. Photons with energies greater than the work function, on the other hand, will eject electrons from the surface of the metal.
The maximum kinetic energy of the emitted electrons is achieved when the incoming photons have the highest possible frequency, which corresponds to the minimum wavelength, λmin, of photons that can eject electrons from the metal surface.
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Determine the difference equation for generating the process
when the excitation is white noise. Determine the system function
for the whitening filter.
2. The power density spectrum of a process {x(n)} is given as 25 Ixx (w) = = |A(w)|² 2 |1 - e-jw + + 12/2e-1²w0 1² where is the variance of the input sequence. a) Determine the difference equation
To determine the difference equation for generating the process when the excitation is white noise, we need to use the power density spectrum given and the properties of white noise.
1. Difference Equation:
The power density spectrum of the process {x(n)} is given as:
Ixx(w) =[tex]|A(w)|²/(2\pi)[/tex]
= [tex]|1 - e^{(-jw)} + (1/2)e^{(-j2w0)}|²,[/tex]
where σ² is the variance of the input sequence.
To obtain the difference equation, we can take the inverse Fourier transform of the power density spectrum. However, since the given power density spectrum has a complicated form, the resulting difference equation may not have a simple form.
2. System Function:
The system function, H(w), represents the transfer function of the system and can be obtained by taking the square root of the power density spectrum:
H(w) = √[Ixx(w)].
Substituting the given power density spectrum into the above equation, we have:
H(w) = √[|1 - e^(-jw) + (1/2)e^(-j2w0)|²/(2π)].
The system function, H(w), describes the frequency response of the system and can be used to analyze the filtering properties of the system.
It's important to note that without further information or constraints on the system, the exact form of the difference equation and the system function cannot be determined. Additional information or constraints on the system would be required to derive a more specific expression for the difference equation and system function.
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Limits to Measurement /6 Explain the difference between accuracy and precision; giving an example to support your answer. (2 marks) When I created the playhouse I had to haul many loads of material fr
The differences between accuracy and precision Accuracy: Accuracy is defined as how close a measurement is to the correct or accepted value. It measures the degree of closeness between the actual value and the measured value. It's a measurement of correctness.
Precision refers to the degree of closeness between two or more measurements of the same quantity. It refers to the consistency, repeatability, or reproducibility of the measurement. Precision has nothing to do with correctness, but rather with the consistency of the measurement . Let's say a person throws darts at a dartboard and their results are as follows:
In the first scenario, the person throws darts randomly and misses the bullseye in both accuracy and precision.In the second scenario, the person throws the darts close to one another, but they are all off-target, indicating precision but not accuracy.In the third scenario, the person throws the darts close to the bullseye, indicating accuracy and precision.
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you are using a 50-mm-focal-length lens to photograph a tree. if you change to a 100-mm-focal-length lens and refocus, the image height on the detector changes by a factor of
The image height on the detector will change by a factor of 2 if you change from a 50-mm-focal-length lens to a 100-mm-focal-length lens and refocus.
The magnification of a lens is given by the ratio of the image height to the object height. Since the object height remains the same, the change in magnification is solely determined by the change in focal length.
The magnification of a lens is given by the formula:
Magnification = - (image distance / object distance).
Since we are only interested in the ratio of image heights, we can ignore the negative sign.
For the 50-mm lens, the magnification is:
Magnification1 = 50 mm / object distance.
For the 100-mm lens, the magnification is:
Magnification2 = 100 mm / object distance.
Taking the ratio of the two magnifications:
Magnification2 / Magnification1 = (100 mm / object distance) / (50 mm / object distance) = 100 mm / 50 mm = 2.
Therefore, the image height on the detector changes by a factor of 2 when switching from a 50-mm-focal-length lens to a 100-mm-focal-length lens and refocusing.
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1. explain the graph in detail !
2. why is the cosmic ray flux inversely proportional to the energy
(when the energy is large then the cosmic ray flux is small)?
3. where do you get the graphics from?
the graphThe graph shows that cosmic ray flux decreases as the energy of cosmic rays increases. The decrease in cosmic ray flux at high energy levels is the consequence of the process known as cosmic ray energy spectrum hardening.
The cosmic ray spectrum is observed to become steeper as energy increases, and the primary reason for this phenomenon is that as the energy of cosmic rays increases, they encounter a more complex and turbid interstellar magnetic field that allows less of them to penetrate into the inner solar system. As a result, the cosmic ray spectrum hardens, with the flux of higher energy cosmic rays decreasing more quickly than that of lower-energy cosmic rays.
The inverse proportionality between cosmic ray flux and energy is due to the way that cosmic rays are produced. High-energy cosmic rays are created by extremely violent astrophysical events such as supernovae, which can accelerate particles to energies of up to 10^20 electron volts (eV). Because these cosmic rays are produced in violent explosions and other energetic events, they have a highly variable and uncertain origin.
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please solve the question related to optics.
3. Explain briefly the principle of constructing achromatic doublets. Con- sider a crown glass with Abbe number 60 and a flint glass with Abbe number 40, assuming that na = 1.5 for both glasses. Deter
An achromatic doublet is made of two optical glasses with varying dispersion, which functions to correct the chromatic aberration of a system. Chromatic aberration arises in optical systems that have lenses, prisms, and diffraction gratings, among other components.
Chromatic aberration causes the colored fringes to appear around the edges of an object in focus. Chromatic aberration arises due to the fact that different wavelengths of light refract to differing degrees.
Achromatic doublets can be made by fusing a lens made of a crown glass, which is a low-dispersion glass, with a lens made of flint glass, which is a high-dispersion glass.
To construct an achromatic doublet, a low-dispersion crown glass and a high-dispersion flint glass are used. An achromatic doublet is made up of two lenses with varying dispersion. By selecting two optical glasses with a sufficient difference in Abbe number, an achromatic doublet can be produced.
A chromatic error-free doublet will have a minimum level of chromatic error when the Abbe numbers of the two components are selected accordingly. An achromatic doublet is made up of two lenses with different dispersions, which serve to eliminate chromatic aberrations from a system.
The refractive index of the crown glass is chosen to be nA = 1.5, while that of the flint glass is chosen to be n B = 1.5. The Abbe numbers for the crown glass and flint glass are 60 and 40, respectively.
The refractive index of the flint glass is greater than that of the crown glass, and it has a higher dispersion.
The two lenses are chosen to be such that their focal lengths are equal and that the chromatic aberration they produce cancels each other out.
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Four people work inside a walk-in cooler for a period of 6 hours per day. The walk-in cooler is maintained at a temperature of 15°F. Calculate the heat load component of the persons working inside the cooler, in Btu/day.
T = 6 hours per day. Temperature = 15 F. The heat load component of the persons working inside the cooler is 190.
Thus, The capacity needed from a cooling system to keep the temperature of a building or space below a desired level is also referred to as the "heat load."
All potential heat-producing activities (heat sources) must be considered in this. This includes indoor heat sources like people, lighting, kitchens, computers, and other equipment, as well as external heat sources like people and sun radiation.
a data centre that houses computers and servers will generate a certain amount of heat load as a result of an electrical load. The building's cooling system will need to take in this heat load and transfer it outside.
Thus, T = 6 hours per day. Temperature = 15 F. The heat load component of the persons working inside the cooler is 190.
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A tank in an elevator with water at a depth of 0.40 m is accelerated at 2 mimWhat is the pressure at the bottom of the tank if the elevator moves downward a. 3.57 kPa c. 4.36 kPa b. 5.78 kPa d. 3.12 kPa 4. A rectangular gate has a base width of 1 m and altitude of 2.4 m. The short side of the gate is flushed with the water surface. Obtain the location of the total force of water on the gate measured from its centroid a. 0.6 m C 0.3 m b. 0.8 m d. 0.4 m 5. A rectangular plate is submerged vertically in two layers of liquids Half of the plate is submerged in water and the other half is in oil (sg = 084). The top of the gate is flushed with liquid surface Obtain the ratio of the force of water to the force of oil a 3.25 c. 3 19 b. 375 d. 3.52
The pressure at the bottom of the tank is 5.78 kPa.
The location of the total force of water on the gate measured from its centroid is 0.6 m.
The ratio of the force of water to the force of oil is 3.75.
The pressure at a point in a fluid is equal to the weight of the fluid above that point divided by the area of the surface.
In this case, the elevator is accelerating downward, so the weight of the fluid above the bottom of the tank is increased by the acceleration due to gravity.
The pressure at the bottom of the tank is therefore:
P = ρgh + ρa
where ρ is the density of the fluid, g is the acceleration due to gravity, h is the depth of the fluid, and a is the acceleration of the elevator.
P = 1000 kg/m^3 * 9.8 m/s^2 * 0.40 m + 1000 kg/m^3 * 2 m/s^2
P = 5.78 kPa
The location of the total force of water on the gate measured from its centroid is equal to the distance from the centroid to the bottom of the gate.
The centroid of the gate is located at 0.6 m from the short side of the gate, so the location of the total force of water on the gate is also 0.6 m from the short side.
The force of water on the plate is equal to the weight of the water that is displaced by the plate. The force of oil on the plate is equal to the weight of the oil that is displaced by the plate.
The ratio of the force of water to the force of oil is therefore equal to the ratio of the densities of water and oil.
ρ_w / ρ_o = 1000 kg/m^3 / 840 kg/m^3 = 1.19
F-w / Fo = ρ_w / ρ_o = 1.19
Therefore, the ratio of the force of water to the force of oil is 1.19.
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2. Consider a silicon crystal at 300K, with the Fermi level 0.2 eV below the conduction band. CB What type is the material? 021 EF E₁ 0 36 FF £9-112 50-56 (2.5) ZF VB 0.56 ev. On e. VE 2. Eg 1-12 E
The given silicon crystal is an n-type semiconductor.What is a semiconductor?
Semiconductor materials are neither excellent conductors nor good insulators. However, their electrical conductivity can be altered and modified by adding specific impurities to the base material through a process known as doping. Doping a semiconductor material generates an extra electron or hole into the crystal lattice, giving it the characteristics of a negatively charged (n-type) or positively charged (p-type) material.
What are n-type and p-type semiconductors?Silicon (Si) and Germanium (Ge) are the two most common materials used as semiconductors. Semiconductors are divided into two types:N-type semiconductors: When some specific impurities such as Arsenic (As), Antimony (Sb), and Phosphorus (P) are added to Silicon, it becomes an n-type semiconductor. N-type semiconductors have a surplus of electrons (which are negative in charge) that can move through the crystal when an electric field is applied.
They also have empty spaces known as holes where electrons can move to.P-type semiconductors: When impurities such as Aluminum (Al), Gallium (Ga), Boron (B), and Indium (In) are added to Silicon, it becomes a p-type semiconductor. P-type semiconductors contain holes (or empty spaces) that can accept electrons and are therefore positively charged.Material type of the given crystalAccording to the question, the Fermi level is 0.2 eV below the conduction band. This shows that the crystal is an n-type semiconductor. Hence, the material type of the given silicon crystal is n-type.Main answerA silicon crystal at 300K, with the Fermi level 0.2 eV below the conduction band, is an n-type semiconductor.
The given silicon crystal is an n-type semiconductor because the Fermi level is 0.2 eV below the conduction band. Semiconductors can be categorized into two types: n-type and p-type. When impurities like Phosphorus, Antimony, and Arsenic are added to Silicon, it becomes an n-type semiconductor.
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