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NPTEL – Physics – Mathematical Physics - 1
Lecture 30
Dynamics of particle : usage of tensors
Let us start by giving a simple example of calculating moment of inertia
of a cylinder of radius R and height H.
The components of the inertia tensor are calculated as,
𝐼𝑥𝑥 = ∑ 𝑚𝑖 (𝑦𝑖 + 𝑧𝑖 )
𝑖
2 2
= ∫ 𝑑𝑥𝑑𝑦𝑑𝑧(𝑦2 + 𝑧2)
Where : density of the
cylinder
= 𝑅2 𝐻
𝑀
Using Cylindrical Co-ordinates, 𝑟⃗ = (𝑟𝑐𝑜𝑠, 𝑟𝑠𝑖𝑛, 𝑧
)
𝑑𝑣 = 𝑑𝑥 𝑑𝑦 𝑑𝑧 = 𝑟 𝑑𝑟 𝑑 𝑑𝑧
So,
𝐼𝑥𝑥 =  ∫ 𝑑𝑧 ∫ 𝑑 ∫ 𝑑𝑟 𝑟 (𝑟2𝑠𝑖𝑛2 + 𝑧2)
𝐻⁄2
−𝐻⁄2
2 𝑅
0 0
=  [𝐻 𝑅4
4 12
+ 𝐻
3
𝑅2]
Using  as in above,
𝐼𝑥𝑥 =
3
𝑀𝐻 +
4
𝑀𝑅
Similarly,
1 1
2 2
𝐼𝑦𝑦 = ∑ 𝑀𝑖 (𝑥𝑖 + 𝑦𝑖 ) = 𝐼𝑥𝑥
𝑖
2 2
Joint initiative of IITs and IISc – Funded by MHRD Page 17 of 20
NPTEL – Physics – Mathematical Physics - 1
𝐼 = ∑ 𝑚 (𝑥 + 𝑦 ) =
𝑧𝑧 𝑖 𝑖 𝑖
𝑖
2 2 𝑀
𝑅 ℎ
2
∫ 𝑑𝑧 ∫ 𝑑 ∫ 𝑑𝑟 (𝑟2𝑐𝑜𝑠2 + 𝑟2𝑠𝑖𝑛2 )
𝐻⁄2
−𝐻⁄2
2 𝑅
0 0
= 𝑀𝑅2
1
2
For the off diagonal elements
𝐼𝑥𝑦 = 𝐼𝑥𝑦 = − ∑ 𝑚𝑖 𝑥𝑖𝑦𝑖 = − ∫ 𝑑𝑧 ∫ 𝑑 ∫ 𝑑𝑟 𝑟3𝑠𝑖𝑛 𝑐𝑜𝑠 = 0
𝑖 −𝐻
𝐻⁄2
⁄2
2 𝑅
0 0
2
(because of ∫ 𝑠𝑖𝑛 𝑐𝑜𝑠 = 0 )
0
Similarly,
𝐼𝑥𝑧 = 𝐼𝑧𝑥 = 𝐼𝑦𝑧 = 𝐼𝑧𝑦 = 0
Thus the only non-zero components are along the diagonal owing to the
symmetry of the object under consideration. Thus the moment of inertia tensor
takes a form,
Velocity and Acceleration- Application in Mechanics
The portion of a particle in 𝑉3 is represented by 𝑥⃑ = (𝑥𝑖(𝑡)), while the
velocity is given by,
𝑣⃑ = 𝑑𝑥⃑
= (𝑥̇ 1, 𝑥̇ 2, 𝑥̇ 3) and the acceleration is given
by, 𝑑𝑡
𝑎⃑ = 𝑑𝑣⃗⃑
= (𝑥̈ 1, 𝑥̈ 2, 𝑥̈ 3) where the number of dots indicate
the 𝑑𝑡
number of time derivatives taken.
In an arbitrary coordinate system, with 𝑔𝑖𝑗 representing the metric tensor, we
have, by definition,
𝑣𝑖 =
𝑑𝑥𝑖
𝑑𝑡
;
Joint initiative of IITs and IISc – Funded by MHRD Page 18 of 20
𝐼𝑥𝑥 0 0
⃡𝐼 = ( 0
0
𝐼𝑦𝑦
0
0 )
𝐼𝑧𝑧
NPTEL – Physics – Mathematical Physics - 1
𝑎𝑖 = + {
𝑖
}
𝑑𝑣𝑖
𝑑𝑡 𝑗𝑘
𝑑𝑥𝑗 𝑑𝑥
𝑘
𝑑𝑡 𝑑𝑡
𝑑𝑡
Where 𝑑𝑣
is the intrisic derivative and {
𝑖
} are the Christoffel symbols
𝑖
𝑗𝑘
calculated from the metric tensor 𝑔𝑖𝑗 associated with the reference system X. If
is also written as
𝑎𝑖 = + 𝛤
𝑟𝑠𝑣 𝑣
𝑑𝑣𝑖
𝑑𝑡
𝑖 𝑟
𝑠
=
𝑑2𝑥𝑖
𝑑𝑡2 𝑑𝑡 𝑑𝑡
+ 𝛤
𝑟𝑠
𝑖 𝑑𝑥 𝑑
𝑥
𝑟 𝑠
Where the speed and acceleration are invariant,
v = √𝑔𝑖𝑗𝑣𝑖𝑣𝑗 a = √𝑔𝑖𝑗𝑎𝑖𝑎𝑗
yielding the contravariant components of velocity and acceleration. Also 𝛤𝑟𝑠 are
defined as,
𝑖
𝛤
𝑟𝑠
𝑖
= 𝜕 𝑥̅
2 𝑗 𝑖
𝜕2𝑥𝑟𝜕𝑥5 𝜕𝑥̅𝑗
𝜕𝑥
If the mass of the particle m, the Newton’s equation of motion yields,
𝐹 𝑖 = 𝑚 = 𝑚𝑎𝑖
Joint initiative of IITs and IISc – Funded by MHRD Page 19 of 20
𝑑𝑣𝑖
𝑑𝑡
The element of work done by the force 𝐹⃗ in producing a displacement
d𝑟⃑ is given by,
dw =𝐹⃗. 𝑑𝑟⃑
since the components of 𝑟⃑ and 𝑑𝑟⃑ are respectively, 𝐹𝑖 and 𝑑𝑥𝑖 , their
scalar product is equal to,
dw = 𝑔𝑖𝑗𝐹𝑖𝑑𝑥𝑗
= 𝐹𝑗 𝐹𝑑𝑥𝑖
NPTEL – Physics – Mathematical Physics - 1
Where 𝐹𝑗 =𝑔𝑖𝑗𝐹𝑖 are the covariant components of the vector 𝐹
⃗. The kinetic energy is written as,
𝑇 = 𝑔𝑖 𝑗 𝑣𝑖 𝑣
𝑗
𝑚
2
Suppose you are given the task of computing the components of
the acceleration in cylindrical coordinates. Here (𝑥1, 𝑥2, 𝑥3) = (𝑟, 𝜃, 𝑧).
The components of the metric tensor as computed from the discussion made
earlier,
𝑔11 = 1, 𝑔22 = (𝑥1)2 = 𝑟2, 𝑔33 = 1
𝑔12 = 𝑔13 = 0 = 𝑔23
Also the components of 𝛤 are computed as,
𝛤
22
1
= −𝑥 = −𝑟 𝛤 = =
1 2
12
𝑥1
1 1
𝑟
Thus, 𝑎1 = − 𝑟 ( )
𝑑2𝑟
𝑑𝑡2
𝑑𝜃 2
𝑑𝑡
𝑎2 =
𝑑2𝜃
𝑑𝑡2 𝑟 𝑑𝑡 𝑑𝑡
𝑑2𝑧
𝑑𝑡2
+
2 𝑑𝑟 𝑑𝜃
𝑎3 =
Joint initiative of IITs and IISc – Funded by MHRD Page 20 of 20

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lec30.ppt

  • 1. NPTEL – Physics – Mathematical Physics - 1 Lecture 30 Dynamics of particle : usage of tensors Let us start by giving a simple example of calculating moment of inertia of a cylinder of radius R and height H. The components of the inertia tensor are calculated as, 𝐼𝑥𝑥 = ∑ 𝑚𝑖 (𝑦𝑖 + 𝑧𝑖 ) 𝑖 2 2 = ∫ 𝑑𝑥𝑑𝑦𝑑𝑧(𝑦2 + 𝑧2) Where : density of the cylinder = 𝑅2 𝐻 𝑀 Using Cylindrical Co-ordinates, 𝑟⃗ = (𝑟𝑐𝑜𝑠, 𝑟𝑠𝑖𝑛, 𝑧 ) 𝑑𝑣 = 𝑑𝑥 𝑑𝑦 𝑑𝑧 = 𝑟 𝑑𝑟 𝑑 𝑑𝑧 So, 𝐼𝑥𝑥 =  ∫ 𝑑𝑧 ∫ 𝑑 ∫ 𝑑𝑟 𝑟 (𝑟2𝑠𝑖𝑛2 + 𝑧2) 𝐻⁄2 −𝐻⁄2 2 𝑅 0 0 =  [𝐻 𝑅4 4 12 + 𝐻 3 𝑅2] Using  as in above, 𝐼𝑥𝑥 = 3 𝑀𝐻 + 4 𝑀𝑅 Similarly, 1 1 2 2 𝐼𝑦𝑦 = ∑ 𝑀𝑖 (𝑥𝑖 + 𝑦𝑖 ) = 𝐼𝑥𝑥 𝑖 2 2 Joint initiative of IITs and IISc – Funded by MHRD Page 17 of 20
  • 2. NPTEL – Physics – Mathematical Physics - 1 𝐼 = ∑ 𝑚 (𝑥 + 𝑦 ) = 𝑧𝑧 𝑖 𝑖 𝑖 𝑖 2 2 𝑀 𝑅 ℎ 2 ∫ 𝑑𝑧 ∫ 𝑑 ∫ 𝑑𝑟 (𝑟2𝑐𝑜𝑠2 + 𝑟2𝑠𝑖𝑛2 ) 𝐻⁄2 −𝐻⁄2 2 𝑅 0 0 = 𝑀𝑅2 1 2 For the off diagonal elements 𝐼𝑥𝑦 = 𝐼𝑥𝑦 = − ∑ 𝑚𝑖 𝑥𝑖𝑦𝑖 = − ∫ 𝑑𝑧 ∫ 𝑑 ∫ 𝑑𝑟 𝑟3𝑠𝑖𝑛 𝑐𝑜𝑠 = 0 𝑖 −𝐻 𝐻⁄2 ⁄2 2 𝑅 0 0 2 (because of ∫ 𝑠𝑖𝑛 𝑐𝑜𝑠 = 0 ) 0 Similarly, 𝐼𝑥𝑧 = 𝐼𝑧𝑥 = 𝐼𝑦𝑧 = 𝐼𝑧𝑦 = 0 Thus the only non-zero components are along the diagonal owing to the symmetry of the object under consideration. Thus the moment of inertia tensor takes a form, Velocity and Acceleration- Application in Mechanics The portion of a particle in 𝑉3 is represented by 𝑥⃑ = (𝑥𝑖(𝑡)), while the velocity is given by, 𝑣⃑ = 𝑑𝑥⃑ = (𝑥̇ 1, 𝑥̇ 2, 𝑥̇ 3) and the acceleration is given by, 𝑑𝑡 𝑎⃑ = 𝑑𝑣⃗⃑ = (𝑥̈ 1, 𝑥̈ 2, 𝑥̈ 3) where the number of dots indicate the 𝑑𝑡 number of time derivatives taken. In an arbitrary coordinate system, with 𝑔𝑖𝑗 representing the metric tensor, we have, by definition, 𝑣𝑖 = 𝑑𝑥𝑖 𝑑𝑡 ; Joint initiative of IITs and IISc – Funded by MHRD Page 18 of 20 𝐼𝑥𝑥 0 0 ⃡𝐼 = ( 0 0 𝐼𝑦𝑦 0 0 ) 𝐼𝑧𝑧
  • 3. NPTEL – Physics – Mathematical Physics - 1 𝑎𝑖 = + { 𝑖 } 𝑑𝑣𝑖 𝑑𝑡 𝑗𝑘 𝑑𝑥𝑗 𝑑𝑥 𝑘 𝑑𝑡 𝑑𝑡 𝑑𝑡 Where 𝑑𝑣 is the intrisic derivative and { 𝑖 } are the Christoffel symbols 𝑖 𝑗𝑘 calculated from the metric tensor 𝑔𝑖𝑗 associated with the reference system X. If is also written as 𝑎𝑖 = + 𝛤 𝑟𝑠𝑣 𝑣 𝑑𝑣𝑖 𝑑𝑡 𝑖 𝑟 𝑠 = 𝑑2𝑥𝑖 𝑑𝑡2 𝑑𝑡 𝑑𝑡 + 𝛤 𝑟𝑠 𝑖 𝑑𝑥 𝑑 𝑥 𝑟 𝑠 Where the speed and acceleration are invariant, v = √𝑔𝑖𝑗𝑣𝑖𝑣𝑗 a = √𝑔𝑖𝑗𝑎𝑖𝑎𝑗 yielding the contravariant components of velocity and acceleration. Also 𝛤𝑟𝑠 are defined as, 𝑖 𝛤 𝑟𝑠 𝑖 = 𝜕 𝑥̅ 2 𝑗 𝑖 𝜕2𝑥𝑟𝜕𝑥5 𝜕𝑥̅𝑗 𝜕𝑥 If the mass of the particle m, the Newton’s equation of motion yields, 𝐹 𝑖 = 𝑚 = 𝑚𝑎𝑖 Joint initiative of IITs and IISc – Funded by MHRD Page 19 of 20 𝑑𝑣𝑖 𝑑𝑡 The element of work done by the force 𝐹⃗ in producing a displacement d𝑟⃑ is given by, dw =𝐹⃗. 𝑑𝑟⃑ since the components of 𝑟⃑ and 𝑑𝑟⃑ are respectively, 𝐹𝑖 and 𝑑𝑥𝑖 , their scalar product is equal to, dw = 𝑔𝑖𝑗𝐹𝑖𝑑𝑥𝑗 = 𝐹𝑗 𝐹𝑑𝑥𝑖
  • 4. NPTEL – Physics – Mathematical Physics - 1 Where 𝐹𝑗 =𝑔𝑖𝑗𝐹𝑖 are the covariant components of the vector 𝐹 ⃗. The kinetic energy is written as, 𝑇 = 𝑔𝑖 𝑗 𝑣𝑖 𝑣 𝑗 𝑚 2 Suppose you are given the task of computing the components of the acceleration in cylindrical coordinates. Here (𝑥1, 𝑥2, 𝑥3) = (𝑟, 𝜃, 𝑧). The components of the metric tensor as computed from the discussion made earlier, 𝑔11 = 1, 𝑔22 = (𝑥1)2 = 𝑟2, 𝑔33 = 1 𝑔12 = 𝑔13 = 0 = 𝑔23 Also the components of 𝛤 are computed as, 𝛤 22 1 = −𝑥 = −𝑟 𝛤 = = 1 2 12 𝑥1 1 1 𝑟 Thus, 𝑎1 = − 𝑟 ( ) 𝑑2𝑟 𝑑𝑡2 𝑑𝜃 2 𝑑𝑡 𝑎2 = 𝑑2𝜃 𝑑𝑡2 𝑟 𝑑𝑡 𝑑𝑡 𝑑2𝑧 𝑑𝑡2 + 2 𝑑𝑟 𝑑𝜃 𝑎3 = Joint initiative of IITs and IISc – Funded by MHRD Page 20 of 20