Class 12th

Get insights from 11.9k questions on Class 12th, answered by students, alumni, and experts. You may also ask and answer any question you like about Class 12th

Follow Ask Question
11.9k

Questions

0

Discussions

44

Active Users

0

Followers

New answer posted

a year ago

0 Follower 1 View

N
Nishtha Datta

Beginner-Level 5

As per NCERT Textbboks"If forward current is too large, it can produce large heating and damage the junction. So, a resistor is used in series with the diode to limit the current in the circuit.

It means when a semiconductor diode is connected to a source under high current it causes excess heat due to more electrical energy. This excess heat is responsible to damage the junction in semiconductor diode permanently. Student can check out NCERT Solutions for Semicondutor Electronics of class 12 physics.  

 

New answer posted

a year ago

0 Follower 15 Views

A
alok kumar singh

Contributor-Level 10

1.34 Velocity of the particle, vx = 2.0 *106m/s

Separation of the two plates, d = 0.5 cm = 0.005 m

Electric field between two plates, E = 9.1 *102 N/C

Charge of an electron, q = 1.6 *10-19 C

Mass of an electron, me = 9.1 *10-31 kg

Let the electron strike the upper plate at the end of the plate L, when deflection is s. Therefore

s = qeL22mvx2

L = 2smvx2qE = 2*0.005*9.1*10-31*(2.0*106)21.6*10-19*9.1*102 = 3.64*10-201.456*10-16

= 0.0158 m = 1.58 cm

Therefore, the electron will strike the upper plate after travelling 1.58 cm.

New answer posted

a year ago

0 Follower 2 Views

P
Payal Gupta

Contributor-Level 10

8.15 Long distance radio broadcasts use shortwave bands because only these bands can be refracted by ionosphere.

It is necessary to use satellites for long distance TV transmissions because television signals are of high frequencies and high energies. Thus these signals are not reflected by ionosphere. Hence, satellites are helpful in reflecting TV signals. Also they help in long distance TV transmissions.

With reference to X-ray astronomy, X-rays are absorbed by the atmosphere. However, visible and radio waves can penetrate. Hence, optical and radio telescopes are built on the ground, while X-ray astronomy is possible only with the help

...more

New answer posted

a year ago

0 Follower 3 Views

P
Payal Gupta

Contributor-Level 10

8.13 A body at a particular temperature produces a continuous spectrum of wavelengths. In case of a black body, the wavelength corresponding to maximum intensity of radiation is given according to Plank's law. It can be given by the relation,

T = 0.29 cmK

λ m = 0.29 T cm K, where λ m

= maximum wavelength and T = temperature

Thus, the temperature for different wavelengths can be obtained as:

For λ m  = 10 - 4 cm, T = 2900 ° K

For λ m  = 5 * 10 - 5 cm, T = 5800 ° K

For λ m  = 10 - 6  cm, T = 290 * 10 3 ° K and so on

The numbers obtained tell us that temperature ranges are required for obtaining radiations in different parts of an electromagnetic spectrum. As the wavelength d

...more

New answer posted

a year ago

0 Follower 66 Views

A
alok kumar singh

Contributor-Level 10

1.32 (a) Let the equilibrium of the test charge be stable. If a test charge is in equilibrium and displaced from its position in any direction, then it experiences a restoring force towards a null point, where the electric field is zero. All the field lines near the null point are directed inwards towards the null point. There is a net inward flux of electric field through a closed surface around the null point. According to Gauss's law, the flux of electric field through a surface, which is not enclosing any charge, is zero. Hence, the equilibrium of the test charge can be stable.

 

(b) Two charges of same magnitude and same sign a

...more

New answer posted

a year ago

0 Follower 3 Views

P
Payal Gupta

Contributor-Level 10

8.12 Power rating of the bulb, P = 100 W

Power of visible radiation, P v = 5% of 100 W = 5 W

Distance from the bulb, d = 1 m

Intensity of radiation at that point is given as:

I = P v 4 π d 2 = 5 4 π * 1 2 = 0.398 W/ m 2

Distance from the bulb, d = 10 m

Intensity of radiation at that point is given as:

I = P v 4 π d 2 = 5 4 π * 10 2 = 3.978 * 10 - 3  W/ m 2

New answer posted

a year ago

0 Follower 1 View

A
alok kumar singh

Contributor-Level 10

1.31 A proton has 3 quarks. Let there be n 'up quarks', then number of 'down quarks' = 3-n

Charge due to n 'up quarks' = (23 e) n

Charge due to (3-n) 'down quarks' =-13e)(3-n) 

Total charge on a proton = +e = (23 e) n +  ( -13e)(3-n) 

e =  2ne3 +ne3-e

2e = 3ne3

n = 2

Number of 'up quark' = 2 and number of 'down quark' = 1. Therefore a proton can be represented as 'uud'.

A neutron has 3 quarks. Let there be n 'up quark' in a neutron and (3-n) 'down quark'

Charge due to n 'up quark' = +(23 e)n

Charge due to (3-n) 'down quark' = 
- ( 13e)(3-n)

Since total charge of a neutron is zero, we get

+ (23e)n -(13e)(3-n) = 0


(23 e)n = ( 13e)(3-n)

2en3=e-en3

en = e or n = 1

Hence number of 'up quark' in neu

...more

New answer posted

a year ago

0 Follower 3 Views

P
Payal Gupta

Contributor-Level 10

8.10 Frequency of the electromagnetic wave, ν  = 2.0 * 10 10  Hz

Electric field amplitude, E 0  = 48 V/m

Speed of light, c = 3 * 10 8 m/s

Wavelength of a wave is given by,

λ = c ν = 3 * 10 8 2.0 * 10 10 = 0.015 m

Magnetic field strength is given by

B 0 = E 0 c = 48 3 * 10 8 = 1.6 10-12 T

Energy density of the electric field is given as,

U E 1 2 ? 0 E 2 and energy density of magnetic field is given by,

U B = 1 2 B 2 μ 0

w h e r e

E 0  = Permittivity of free space

μ 0 =  Permeability of free space

We have the relation connecting E and B as:

E = cB, where c = 1 ? 0 μ 0

Hence E = B ? 0 μ 0 i ?

E 2  = B 2 ? 0 μ 0

? 0 E 2 = B 2 μ 0

2 U E = 2 U B  or U E = U B

New answer posted

a year ago

0 Follower 4 Views

P
Payal Gupta

Contributor-Level 10

8.9 Energy of a photon is given as:

E = h ν = hcλ , where

h = Planck's constant = 6.6 *10-34 Js

c = Speed of light = 3 *108 m/s

λ = wavelength of radiation

Hence, E = 6.6*10-34*3*108λ J = 1.98*10-25λ J = 1.98*10-25λ*1.602*10-19 eV = 1.236*10-6λ eV

The following table lists the photon energies for different parts of an electromagnetic spectrum for different λ

New answer posted

a year ago

0 Follower 69 Views

A
alok kumar singh

Contributor-Level 10

1.30 

Take a long thin wire XY of uniform linear charge density λ. Consider a point A at a perpendicular distance l from the midpoint O of the wire. Let E be the electric field at point A due to the wire XY. Consider a small length element dx on the wire section with OZ = x. Let q be the charge on this piece.

Q = λdx

Electric field due to the piece,

dE =  = 14πε0*λdx(AZ)2  = 14πε0*λdx(l2+x2)since AZ =l2+x2

The electric field is resolved into two rectangular components. dE cos?θ is the perpendicular component and dEsin?θ  When the whole wire is considered, the component dE sin?θistheparallelcomponent. is cancelled. Only the perpendicular component dE cos?θ affects point A.

Hence

...more

Get authentic answers from experts, students and alumni that you won't find anywhere else

Sign Up on Shiksha

On Shiksha, get access to

  • 66k Colleges
  • 1.2k Exams
  • 705k Reviews
  • 1850k Answers

Share Your College Life Experience

×
×

This website uses Cookies and related technologies for the site to function correctly and securely, improve & personalise your browsing experience, analyse traffic, and support our marketing efforts and serve the Core Purpose. By continuing to browse the site, you agree to Privacy Policy and Cookie Policy.