6. Unlimited DOUBT solving on doubt
App 8 AM- 11 PM
Regular Mock Tests and Practice
Papers
20 All India Level tests
7.
8. ₹10,000
How to Avail Discount ?
Apply Coupon Code: SMCC
Visit: https://vdnt.in/JEECCE
Special Discount for this class
Link in Description
₹4,000/-
(incl. of all taxes)
17. NLM
Linear Momentum :
Newton’s first law : inertial frame.
Newton’s second law :
Newton’s third law :
Frictional Force : fstatic, max
= 𝜇s
N, f kinetic
=𝜇k
N
Banking angle :
20. Work:
Kinetic energy :
Potential energy : for conservative F
Work done by conservative force is path
independent and depends only on initial
and final points :
WPE
21. Work - energy theorem : W = ∆ K
Mechanical energy : E = U + K
Conserved if forces are conservative in nature.
Power :
WPE
35. Variation of g with depth:
Variation of g with height:
Effect of non-spherical earth shape on g:
g at pole > g at equator (∵ Re
- Rp
≈ 21 km)
Effect of earth rotation on apparent weight:
Mg𝜃
’ = mg - m𝜔2
Rcos2
𝜃
Gravitation
36. Orbital velocity of satellite :
Escape velocity :
Kepler’s laws :
First: Elliptical orbit with sun at one of the focus.
Second : areal velocity is constant .
Third : T2
𝛼 a3
. In circular orbit
Gravitation
44. Notation : Amplitude A, Frequency v, Wavelength 𝜆,
period T, Angular Frequency 𝜔, Wave number k,
Progressive wave travelling with speed v:
Y = f(t - x/v), ⇝ + x, y = f(t + x/v), ⇝ - x
Progressive sine wave:
y = A sin(kx -𝜔t) = A sin(2𝜋(x/𝜆 - t/T))
Wave Motion
47. String fixed at both ends:
1. Boundary conditions y = 0 at x = 0 and at x = L
2. Allowed freq:
3. Fundamental/1st
harmonics :
4. 1st
overtone/2nd
harmonics:
5. 2nd
overtone/3rd
harmonics :
6. All harmonics are present.
Waves On String
48. String fixed at one end:
1. Boundary conditions: y = a at x = L
2. Allowed freq:
3. Fundamental/1st
harmonics :
4. 1st
overtone/3rd
harmonics :
5. 2nd
overtone/5th
harmonics:
6. Only odd harmonics are present.
Waves On String
50. Displacement wave : s = s0
sin 𝜔 (t - x/v)
Pressure wave : p = p0
cos 𝜔(t-x/v), p0
= (B𝜔/v) s0
Speed of sound waves :
Sound Waves
51. Closed organ pipe:
1. Boundary condition: x = 0 at y = 0
2. Allowed freq:
3. Fundamental/1st
harmonics :
4. 1st
overtone/3rd
harmonics:
5. 2nd
overtone/5th
harmonics:
6. Only odd harmonics are present.
Sound Waves
52. Open organ pipe:
1. Boundary condition ; x = 0 at y = 0
Allowed freq:
2. Fundamental/1st
harmonics:
3.1st
overtone/2nd
harmonics:
4. 2nd
overtone/3rd
harmonics:
5. All harmonics are present.
Sound Waves
53. Beats: two waves of almost equal frequencies 𝜔1
≈ 𝜔2
P1
= P0
sin 𝜔1
(t - x/v), P2
= sin 𝜔2
(t - x/v)
P = P1
+ P2
= 2P0
cos ∆𝜔(t - x/v) sin 𝜔(t - x/v)
𝜔= (𝜔1
+ 𝜔2
)/2, ∆𝜔 = 𝜔1
- 𝜔2
(beats freq.)
Doppler Effect:
Where, v is the speed of sound in the medium, u0
is the
speed of the observer w.r.t. the medium, considered positive
when it moves towards the source and negative when it
moves away from the source, and us
is the speed of the
source w.r.t. the medium, considered positive when it moves
towards the observer and negative when it moves away
from the observer.
Sound Waves
59. Temperature And Thermal
Expansion
Temp. scales:
Ideal gas equation: pV = nRT, n : number of moles
Thermal expansion:
L = L0
(1 + 𝛼∆T), A = A0
(1 + 𝛽∆T) , = V0
(1 + 𝛾∆T)
𝛼 = 𝛽/2 = 𝛾/3
Thermal stress of a material :
62. Kirchhoff’s law:
Wien’s displacement law: 𝜆m
T = b
( b = 3 × 10-3
m-k)
Stefan-Boltzmann law: (σ=5.6704×10−8
W/m2
·K)
Newton’s law of cooling :
Heat Transfer
64. KTG
General : M = mNA
, k = R/NA
RMS Speed :
Average speed :
Most probable speed :
Pressure :
Equipartition of energy: K = kT for each
degree of freedom. Thus, K = kT for molecule
having f degrees of freedom.
Internal energy of n moles of an ideal gas is
U = nRT.
65. Specific heat :
Latent heat : L = Q/m
Specific heat at constant volume:
Specific heat at constant pressure:
Relation between Cp
and Cv
: Cp
- Cv
= R
Ratio of specific heats : 𝛾 = Cp
/Cv
KTG
66. Relation between U and Cv
: ∆U = nCv
∆T
Specific heat of gas mixture:
Molar internal energy of an ideal gas U = RT,
f = 3 for monatomic and f = 5 for diatomic gas.
KTG
79. Force between plates of a parallel plate
capacitor :
Energy stored in capacitor :
Energy density in electric field:
Capacitor with dielectric : C=KC0
Capacitance
C0
= ∊0
A/d
81. Current Electricity
Current density : j = i/A = 𝜎E
Drift speed :
Resistance of a wire : R = pl/A, where p = 1/𝜎
Temp. dependence of resistance : R = R0
(1 + 𝛼∆T)
Ohm’s law : V = iR
82. Kirchhoff’s Laws :
(i) The junction law: The algebraic sum of all the
currents directed towards a node is zero i.e., ∑node
Ii
= 0.
(ii) The Loop Law: The algebraic sum of all the
potential differences along a closed loop in a circuit is
zero i.e. ∑loop
∆ Vi
= 0.
Resistors in parallel :
Resistors in series : Req
R1
+ R2
Current Electricity
94. EMI
Magnetic flux :
Faraday’s law :
Lenz’s Law : Induced current create a B-field
that opposes the change in magnetic flux.
Motional emf : e = Blv
95. Self inductance :
Self inductance of a solenoid : L = 𝜇0
n2
(𝜋r2
l)
Energy stored in an inductor :
Energy density of B field :
Mutual inductance :
EMI
96. Growth of current in LR circuit :
Decay of current in LR circuit :
Time constant of LR circuit : 𝜏 = L/R
EMI
98. EMF induced in a rotating coil : e = NAB 𝜔 sin 𝜔t
Alternating current :
i = i0
sin(𝜔t + 𝜙), T = 2𝜋/𝜔
Average current in AC :
RMS current :
Energy : E = irms
2
RT
AC
103. Laws of reflection :
(i) Incident ray, reflected ray,
and normal lie in the same plane
(ii) ∠i = ∠r
Plane mirror :
(i) the image and the object are
equidistant from mirror
(ii) virtual image of real object
Ray optics
104. Spherical mirror :
1. Focal length: f = R/2
2. Mirror equation :
3. Magnification :
Ray optics
108. Ray Optics
Lens formula :
Power of the lens : P in diopter if f in metre.
Two thin lenses separated by distance d :
109. Simple microscope : m = D/f in normal adjustment.
Compound microscope :
1. Magnification in normal adjustment :
2. Resolving power :
Ray Optics- Optical
Instruments
111. Dispersion by prism with small A and i :
1. Mean deviation : 𝛿y
= (𝜇y
- 1) A
2. Angular dispersion: 𝛳 = (𝜇v
- 𝜇r
)A
Dispersive power : (if A and i small)
Dispersion without deviation :
(𝜇y
- 1) A +(𝜇y
’ - 1)A’ = 0
Deviation without dispersion :
(𝜇v
- 𝜇r
)A = (𝜇v
’ - 𝜇r
’)A’
Ray Optics- Dispersion
122. Radioactivity
Nuclear radius : R = R0
A1/3
, R0
≈ 1.1 × 10-15
m
Decay rate :
Population at time t : N = N0
e-𝜆t
Half life : t1/2
= 0.693/𝜆
Average life : tav
= 1/𝜆
Population after n half lives : N = N0
/2n
124. Nuclei
Mass defect : ∆m = [Zmp
+ (A - Z)mn
] - M
Binding energy : B = [Zmp
+ (A -Z)mn
- M]c2
Energy released in nuclear reaction : ∆E = ∆mc2
Where ∆m = mreactants
- mproducts
.
132. Unlimited DOUBT solving on doubt
App 8 AM- 11 PM
Regular Mock Tests and Practice
Papers
20 All India Level tests
133.
134. ₹10,000
How to Avail Discount ?
Apply Coupon Code: SMCC
Visit: https://vdnt.in/JEECCE
Special Discount for this class
Link in Description
₹4,000/-
(incl. of all taxes)