NPTEL – Physics – Mathematical Physics - 1
Lecture 29
Metric Tensor
The rotation of distance is fundamental in all areas of physics and mathematics.
The arc length in different coordinate system is represented as,
𝑑𝑠2 = (𝑑𝑥1)2 + (𝑑𝑥2)2 + (𝑑𝑥3)2 = 𝛿𝑖𝑗 𝑑𝑥𝑖𝑑𝑥𝑗
More generally, this can be written as,
𝑑𝑠2 = gij𝑑𝑥𝑖 𝑑𝑥𝑗
In polar coordinates : (𝑥1, 𝑥2) = (𝑟, 𝜃)
𝑑𝑠2 = (𝑑𝑥1)2 + (𝑥1)2(𝑑𝑥2)2
in spherical polar coordinates :
(𝑥1, 𝑥2, 𝑥3) = (𝑟, 𝜃, 𝛷)
𝑑𝑠2 = (𝑑𝑥1)2 + (𝑥1)2(𝑑𝑥2)2 + (𝑥1𝑠𝑖𝑛𝑥2)2(𝑑𝑥3)2 etc. thus in
general notation, let {𝑥1𝑗} denote a set of Cartesian
coordinates and
{𝑥𝑗} denote some other coordinates of which {𝑥1𝑗} are
functions. Then we have,
𝑑𝑥1𝑖
(1)
𝑑𝑥1𝑖 = 𝑑𝑥𝑗 (sum over j is
implicit)
thus the element of length (squared) in a 𝑉
𝑛 space is,
𝑑𝑠2 = ∑𝑛 (𝑑𝑥1𝑖)2
= ∑𝑛
𝑖=1 𝑖=1 𝑑𝑥1𝑖 𝑑𝑥1𝑖
= ∑𝑛
(𝜕𝑥
1𝑖
𝜕𝑥
𝑗
𝑑𝑥𝑗 ) (𝜕𝑥
𝑑𝑥𝑘
)
𝑖=1
1𝑖
𝜕𝑥
𝑘
= (∑𝑛 𝜕𝑥 𝜕
𝑥
1𝑖
𝜕𝑥 𝜕
𝑥
𝑗
𝑖=1
1𝑖
𝑘 ) 𝑑𝑥 𝑑𝑥
𝑗 𝑘
(2)
Compose Eq. (1) and (2)
𝑛
𝑔 = ∑
𝑗 𝑘 𝑖=1
𝜕𝑥1𝑖 𝜕𝑥1
𝑖
𝜕𝑥𝑗 𝜕𝑥
𝑘
𝑔𝑗 𝑘 is called the metric tenk of order (0, 2) which can be proved as
follows,
𝑛
Page 15 of 20
Joint initiative of IITs and IISc – Funded by MHRD
𝑔𝑗𝑘 = ∑
𝜕𝑥̅ 𝑗 𝜕𝑥̅𝑘
𝑖=1
𝜕𝑥1𝑖 𝜕𝑥1𝑖
Using a chain rule,
NPTEL – Physics – Mathematical Physics - 1
𝑔𝑗𝑘 = ∑
𝜕𝑥𝑝 𝜕𝑥̅ 𝑗 𝜕𝑥𝑞 𝜕𝑥̅𝑘
𝑖=1
𝜕𝑥1𝑗 𝜕𝑥𝑝 𝜕𝑥1𝑗 𝜕𝑥
𝑞
𝑛
= (∑𝑛 𝜕𝑥 𝜕𝑥 𝜕𝑥 𝜕𝑥
1
𝑗
𝜕𝑥 𝜕𝑥 𝜕𝑥̅ 𝜕𝑥̅ 𝜕𝑥̅ 𝜕𝑥̅
𝑝 𝑞 𝑗 𝑘 𝑗 𝑘
𝑖=1
1𝑗 𝑝 𝑞
) = 𝑔𝑝𝑞
𝜕𝑥 𝜕𝑥
𝑝 𝑞
𝑔𝑝𝑞
The elements of the metric tensor are invertible which can be extended
as,
𝑔𝑗𝑘ℎ𝑘𝑚 = 𝛿𝑗
𝑚
Example
Metric tensor in spherical polar coordinates We
have,
x = rsin𝜃𝑐𝑜𝑠, 𝑦 = 𝑟𝑠𝑖𝑛𝜃𝑠𝑖𝑛,
metric tensors are
𝑧 = 𝑟𝑐𝑜𝑠𝜃. The components of the
𝑔𝑟𝑟 (𝑟, 𝜃, ) = (𝜕𝑟
) + (𝜕𝑟
) + ( )
𝜕𝑥 𝜕𝑦 𝜕𝑧
2 2 2
𝜕𝑟
= (sin 𝑐𝑜𝑠)2 + (𝑠𝑖𝑛𝜃𝑠𝑖𝑛)2 + (𝑐𝑜𝑠𝜃)2
= 1
𝑔𝑟𝑟 (𝑟, 𝜃, ) =
𝜕𝑥 𝜕𝑥 𝜕𝑦 𝜕𝑦 𝜕𝑧 𝜕
𝑧
+ +
𝜕𝑟 𝜕𝜃 𝜕𝑟 𝜕𝜃 𝜕𝑟 𝜕𝜃
= 0 (check !!)
𝜕𝑥 2
𝜕𝑦 2
𝜕𝑧 2
𝑔𝜃𝜃 = (
𝜕𝑟
) + (
𝜕𝑟
) + (
𝜕𝑟
)
= 𝑟2
𝑔 = (
𝜕
𝜕𝑥 2
𝜕𝑦 2
𝜕𝑧 2
) + ( ) + ( )
𝜕 𝜕
𝑑𝑠2 = (𝑑𝑟)2 + 𝑟2(𝑑𝜃)2 + 𝑟2𝑠𝑖𝑛2𝜃(𝑑)2
-a known result
Page 16 of 20
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lec29.ppt

  • 1. NPTEL – Physics – Mathematical Physics - 1 Lecture 29 Metric Tensor The rotation of distance is fundamental in all areas of physics and mathematics. The arc length in different coordinate system is represented as, 𝑑𝑠2 = (𝑑𝑥1)2 + (𝑑𝑥2)2 + (𝑑𝑥3)2 = 𝛿𝑖𝑗 𝑑𝑥𝑖𝑑𝑥𝑗 More generally, this can be written as, 𝑑𝑠2 = gij𝑑𝑥𝑖 𝑑𝑥𝑗 In polar coordinates : (𝑥1, 𝑥2) = (𝑟, 𝜃) 𝑑𝑠2 = (𝑑𝑥1)2 + (𝑥1)2(𝑑𝑥2)2 in spherical polar coordinates : (𝑥1, 𝑥2, 𝑥3) = (𝑟, 𝜃, 𝛷) 𝑑𝑠2 = (𝑑𝑥1)2 + (𝑥1)2(𝑑𝑥2)2 + (𝑥1𝑠𝑖𝑛𝑥2)2(𝑑𝑥3)2 etc. thus in general notation, let {𝑥1𝑗} denote a set of Cartesian coordinates and {𝑥𝑗} denote some other coordinates of which {𝑥1𝑗} are functions. Then we have, 𝑑𝑥1𝑖 (1) 𝑑𝑥1𝑖 = 𝑑𝑥𝑗 (sum over j is implicit) thus the element of length (squared) in a 𝑉 𝑛 space is, 𝑑𝑠2 = ∑𝑛 (𝑑𝑥1𝑖)2 = ∑𝑛 𝑖=1 𝑖=1 𝑑𝑥1𝑖 𝑑𝑥1𝑖 = ∑𝑛 (𝜕𝑥 1𝑖 𝜕𝑥 𝑗 𝑑𝑥𝑗 ) (𝜕𝑥 𝑑𝑥𝑘 ) 𝑖=1 1𝑖 𝜕𝑥 𝑘 = (∑𝑛 𝜕𝑥 𝜕 𝑥 1𝑖 𝜕𝑥 𝜕 𝑥 𝑗 𝑖=1 1𝑖 𝑘 ) 𝑑𝑥 𝑑𝑥 𝑗 𝑘 (2) Compose Eq. (1) and (2) 𝑛 𝑔 = ∑ 𝑗 𝑘 𝑖=1 𝜕𝑥1𝑖 𝜕𝑥1 𝑖 𝜕𝑥𝑗 𝜕𝑥 𝑘 𝑔𝑗 𝑘 is called the metric tenk of order (0, 2) which can be proved as follows, 𝑛 Page 15 of 20 Joint initiative of IITs and IISc – Funded by MHRD 𝑔𝑗𝑘 = ∑ 𝜕𝑥̅ 𝑗 𝜕𝑥̅𝑘 𝑖=1 𝜕𝑥1𝑖 𝜕𝑥1𝑖 Using a chain rule,
  • 2. NPTEL – Physics – Mathematical Physics - 1 𝑔𝑗𝑘 = ∑ 𝜕𝑥𝑝 𝜕𝑥̅ 𝑗 𝜕𝑥𝑞 𝜕𝑥̅𝑘 𝑖=1 𝜕𝑥1𝑗 𝜕𝑥𝑝 𝜕𝑥1𝑗 𝜕𝑥 𝑞 𝑛 = (∑𝑛 𝜕𝑥 𝜕𝑥 𝜕𝑥 𝜕𝑥 1 𝑗 𝜕𝑥 𝜕𝑥 𝜕𝑥̅ 𝜕𝑥̅ 𝜕𝑥̅ 𝜕𝑥̅ 𝑝 𝑞 𝑗 𝑘 𝑗 𝑘 𝑖=1 1𝑗 𝑝 𝑞 ) = 𝑔𝑝𝑞 𝜕𝑥 𝜕𝑥 𝑝 𝑞 𝑔𝑝𝑞 The elements of the metric tensor are invertible which can be extended as, 𝑔𝑗𝑘ℎ𝑘𝑚 = 𝛿𝑗 𝑚 Example Metric tensor in spherical polar coordinates We have, x = rsin𝜃𝑐𝑜𝑠, 𝑦 = 𝑟𝑠𝑖𝑛𝜃𝑠𝑖𝑛, metric tensors are 𝑧 = 𝑟𝑐𝑜𝑠𝜃. The components of the 𝑔𝑟𝑟 (𝑟, 𝜃, ) = (𝜕𝑟 ) + (𝜕𝑟 ) + ( ) 𝜕𝑥 𝜕𝑦 𝜕𝑧 2 2 2 𝜕𝑟 = (sin 𝑐𝑜𝑠)2 + (𝑠𝑖𝑛𝜃𝑠𝑖𝑛)2 + (𝑐𝑜𝑠𝜃)2 = 1 𝑔𝑟𝑟 (𝑟, 𝜃, ) = 𝜕𝑥 𝜕𝑥 𝜕𝑦 𝜕𝑦 𝜕𝑧 𝜕 𝑧 + + 𝜕𝑟 𝜕𝜃 𝜕𝑟 𝜕𝜃 𝜕𝑟 𝜕𝜃 = 0 (check !!) 𝜕𝑥 2 𝜕𝑦 2 𝜕𝑧 2 𝑔𝜃𝜃 = ( 𝜕𝑟 ) + ( 𝜕𝑟 ) + ( 𝜕𝑟 ) = 𝑟2 𝑔 = ( 𝜕 𝜕𝑥 2 𝜕𝑦 2 𝜕𝑧 2 ) + ( ) + ( ) 𝜕 𝜕 𝑑𝑠2 = (𝑑𝑟)2 + 𝑟2(𝑑𝜃)2 + 𝑟2𝑠𝑖𝑛2𝜃(𝑑)2 -a known result Page 16 of 20 Joint initiative of IITs and IISc – Funded by MHRD