Spinorial Field Representation

In summary: So the coefficients a_{ A } are given bya_{ A } = \frac{1}{4}\Gamma^{ A }^{*}\left( \begin{array} {c} -1 & -2 & -3 \\ 0 & 1 & 2 \\ 3 & 4 & 5 \end{array} \right).
  • #1
Breo
177
0
What does mean the next (why we write it like this, why is a sum, why first a 0 and secondly a 1/2 and viceversa):

$$ (\frac{1}{2} , 0 ) \oplus (0, \frac{1}{2}) $$

?
 
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  • #2
Do you know how the representations of the Lorentz group are classified? The (1/2, 0) and (0, 1/2) are two irreducible representations of the Lorentz group. These representations are also called the "left-handed Weyl spinor" and the "right-handed Weyl spinor." The ##\oplus## is the symbol for a direct sum of group representations.
 
  • #3
I asked this to eventually understand the next decomposition. If we take the tensor product of 2 spinors ## \Psi\Psi* ##:

$$[(\frac{1}{2}, 0 ) \oplus (0, \frac{1}{2})] \otimes [(\frac{1}{2}, 0 ) \oplus (0, \frac{1}{2})] = 2(\frac{1}{2},\frac{1}{2}) \oplus (1,0) \oplus 2(0, 0 ) \oplus (0, 1)$$

Why we say these are 16 terms and how to descompose ##2(\frac{1}{2},\frac{1}{2})## in the vector ## \bar{\Psi}\gamma^{\mu}\Psi ## and pseudovector ## \bar{\Psi}\gamma^5 \gamma^{\mu}\Psi ## ?
 
  • #4
May I suggest supplimenting whatever you're reading with Wu Ki Tung's group theory for physicists book? It explains things nicely. Miller's book is more detailed (especially on the Clebsch-Gordan theorem), but more intricate. Why are there 16 terms in a basis ? The representation space of the product representation is the tensor product of the 2 spaces. How do you compute dimensions?
 
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  • #5
## dim ( D \otimes D) = dim (D) .dim (D) ## ?
 
  • #6
Bingo, so if the direct sum of 2 elementary Weyl spinors has dimension 4, what's the dimension of the product of 2 such direct sums?
 
  • #7
16. I missunderstood the dimensions and terms... Thank you for clarification.

Do you know how to descompose the ##2(1/2, 1/2)## as I stated in the official post?
 
  • #9
Breo said:
I asked this to eventually understand the next decomposition. If we take the tensor product of 2 spinors ## \Psi\Psi* ##:

$$[(\frac{1}{2}, 0 ) \oplus (0, \frac{1}{2})] \otimes [(\frac{1}{2}, 0 ) \oplus (0, \frac{1}{2})] = 2(\frac{1}{2},\frac{1}{2}) \oplus (1,0) \oplus 2(0, 0 ) \oplus (0, 1)$$
The LHS of this equation is the vector space [itex]S \otimes \bar{ S }[/itex] of all 16-component vectors of the form [itex]\psi \otimes \bar{ \psi }[/itex]. We can also take this “vector” to be the [itex]4 \times 4[/itex] matrix (of fields on [itex]M^{ ( 1 , 3 ) }[/itex]) [itex]\psi_{ a } \bar{ \psi }_{ b }[/itex] formed by the following direct product
[tex]
\psi \otimes \bar{ \psi } = \left( \begin{array} {c} \psi_{1} \\ \psi_{2} \\ \psi_{3} \\ \psi_{4} \end{array} \right) \otimes \left( \psi_{ 1 }^{ * } , \ \psi_{ 2 }^{ * } , \ - \psi_{ 3 }^{ * } , \ - \psi_{ 4 }^{ * } \right) .
[/tex]
Or
[tex]
\psi \otimes \bar{ \psi } = \left( \begin {array} {c c c c}
( \psi_{ 1 } \psi_{ 1 }^{ * } ) & ( \psi_{ 1 } \psi_{ 2 }^{ * } ) & ( - \psi_{ 1 } \psi_{ 3 }^{ * } ) & ( - \psi_{ 1 } \psi_{ 4 }^{ * } ) \\
( \psi_{ 2 } \psi_{ 1 }^{ * } ) & ( \psi_{ 2 } \psi_{ 2 }^{ * } ) & ( - \psi_{ 2 } \psi_{ 3 }^{ * } ) & ( - \psi_{ 2 } \psi_{ 4 }^{ * } ) \\
( \psi_{ 3 } \psi_{ 1 }^{ * } ) & ( \psi_{ 3 } \psi_{ 2 }^{ * } ) & ( - \psi_{ 3 } \psi_{ 3 }^{ * } ) & ( - \psi_{ 3 } \psi_{ 4 }^{ * } ) \\
( \psi_{ 4 } \psi_{ 1 }^{ * } ) & ( \psi_{ 4 } \psi_{ 2 }^{ * } ) & ( - \psi_{ 4 } \psi_{ 3 }^{ * } ) & ( - \psi_{ 4 } \psi_{ 4 }^{ * } )
\end {array} \right) .
[/tex]
But any [itex]4 \times 4[/itex] matrix can be expanded in the standard (complete) basis of Clifford algebra [itex]\mathcal{ C }_{ ( 1 , 3 ) } ( \mathbb{ C } )[/itex]:
[tex]
\Gamma^{ A } = \{ I_{4 \times 4} , \gamma^{ \mu } , \gamma^{ \mu } \gamma_{ 5 } , \sigma^{ \mu \nu } , \gamma_{ 5 } \} ,
[/tex]
where [itex]A = 1 , 2 , \cdots , 16[/itex]. So, we can write
[tex]
\psi \otimes \bar{ \psi } = \sum_{ A = 1 }^{ 16 } a_{ A } \ \Gamma^{ A } . \ \ \ \ (1)
[/tex]
To find the coefficients [itex]a_{ A }[/itex] we use the trace properties of [itex]\Gamma^{ A }[/itex]: [tex]\mbox{ Tr } ( \Gamma^{ A } ) = 0 , \ \mbox{for} \ \Gamma^{ A } \neq I ,[/tex]
[tex]\mbox{ Tr } ( \Gamma^{ A } ) = 4 , \mbox{for} \ \Gamma^{ A } = I ,[/tex]
and
[tex]\mbox{ Tr } ( \Gamma_{ B } \Gamma^{ A } ) \sim 2^{ 2 } \delta^{ A }_{ B } .[/tex]
So, multiplying Eq(1) with [itex]\Gamma_{ B }[/itex] and taking the trace, we find
[tex]
\mbox{ Tr } ( \Gamma_{ B } \psi \otimes \bar{ \psi } ) = a_{ I } \mbox{ Tr } ( \Gamma_{ B } ) + \sum_{ \Gamma^{ R } \neq I } a_{ R } \mbox{ Tr } ( \Gamma_{ B } \Gamma^{ R } ) . \ \ \ (2)
[/tex]
For [itex]\Gamma_{ B } = I[/itex], we find
[tex]
a_{ I } = \frac{ 1 }{ 4 } \mbox{ Tr } ( \psi \otimes \bar{ \psi } ) = \frac{ 1 }{ 4 } \bar{ \psi } \psi .[/tex]
For [itex]\Gamma_{ B } \neq I[/itex], Eq(2) gives
[tex]
\mbox{ Tr } ( \Gamma_{ B } \psi \otimes \bar{ \psi } ) = 0 + \sum_{ \Gamma^{ R } \neq I } a_{ R } \mbox{ Tr } ( \Gamma_{ B } \Gamma^{ R } ) \sim 2^{ 2 } a_{ B } .
[/tex]
Thus
[tex]
a_{ B } \sim \frac{ 1 }{ 4 } ( \Gamma_{ B } )_{ a b } ( \psi \otimes \bar{ \psi } )_{ b a } = \frac{ 1 }{ 4 } \bar{ \psi }_{ a } ( \Gamma_{ B } )_{ a b } \psi_{ b } = \frac{ 1 }{ 4 } \bar{ \psi }_{ a } \Gamma_{ B } \psi .
[/tex]
So, our expansion Eq(1) becomes
[tex]
\psi \otimes \bar{ \psi } = \frac{ 1 }{ 4 } ( \bar{ \psi } \psi ) \ I + \frac{ c }{ 4 } \sum_{ \Gamma^{ B } \neq I } ( \bar{ \psi } \Gamma^{ B } \psi ) \Gamma_{ B } ,
[/tex]
where [itex]c[/itex] is a constant whose value depends on the definitions of [itex]\gamma_{5}[/itex] and [itex]\sigma^{ \mu \nu }[/itex] and on the signature of the spacetime metric.
From this it follows that
[tex]
\bar{ \psi } \psi + \bar{ \psi } \gamma_{ 5 } \psi \ \in ( 0 , 0 ) \oplus ( 0 , 0 ) , \mbox{ dim } : \ [1] \oplus [1] ,
[/tex]
[tex]
\bar{ \psi } \gamma^{ \mu } \psi + \bar{ \psi } \gamma^{ \mu } \gamma_{ 5 } \psi \ \in ( 1/2 , 1/2 ) \oplus ( 1/2 , 1/2 ) \sim [4] \oplus [4] ,
[/tex]
and
[tex]
\bar{ \psi } \sigma^{ \mu \nu } \psi \ \in ( 1 , 0 ) \oplus ( 0 , 1 ) \sim [6] .
[/tex]
So, going back to the vector space [itex]S \otimes \bar{ S }[/itex], we can say that the [itex]16 \times 16[/itex] matrices which act naturally on the 16-component “vector” [itex]\psi \otimes \bar{ \psi } \in S \otimes \bar{ S }[/itex] can be brought into block diagonal form with matrices of dimensions [itex][1] , [1] , [4] , [4][/itex] and [itex][6][/itex] on the diagonal.
Why we say these are 16 terms and how to descompose ##2(\frac{1}{2},\frac{1}{2})## in the vector ## \bar{\Psi}\gamma^{\mu}\Psi ## and pseudovector ## \bar{\Psi}\gamma^5 \gamma^{\mu}\Psi ## ?
You need to spend more time on group theory in general and the representation theory of Lorentz algebra in particular.

Sam
 
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  • #10
Thank you very much.

Yes, I have started to studying theoretical physics this year. I have a lack of many "basic" things but I am trying to solving them :).

Indeed, I have one when reading you: where can I learn the properties of the traces? I know is the summ of the diagonal terms of a matrix but I do not figure out when I see some of his uses. Maybe if you could tell me why do you can used it in your derivation...
 
  • #11
Which traces derivation?
The [itex]\gamma^\mu[/itex] are traceless matrices, so are the [itex]\gamma_5[/itex]
Then [itex]\gamma^\mu \gamma_5 [/itex] are also traceless, take eg at some particular representation (Weyl):
[itex]\gamma^\mu= \begin{pmatrix} 0 & \sigma^\mu \\ \bar{\sigma}^\mu & 0 \end{pmatrix}, ~~ \gamma_5 = \begin{pmatrix} -1 & 0 \\ 0 & 1 \end{pmatrix}[/itex]
with [itex]\sigma^\mu = (1, \vec{\sigma}), ~~\bar{\sigma}^\mu = (1, -\vec{\sigma})[/itex]

Take the product:

[itex]\gamma^\mu \gamma_5= \begin{pmatrix} 0 & \sigma^\mu \\ \bar{\sigma}^\mu & 0 \end{pmatrix} \begin{pmatrix} -1 & 0 \\ 0 & 1 \end{pmatrix}= \begin{pmatrix} 0 & \sigma^\mu \\ -\bar{\sigma}^\mu & 0 \end{pmatrix} [/itex]

Is still traceless. Of course using the anticommutation relations can also give you this answer (so it's a result of the algebra).
[itex]Tr(\gamma^\mu \gamma_5)= Tr (\gamma_5 \gamma^\mu)= -Tr(\gamma^\mu \gamma_5) \Rightarrow Tr(\gamma^\mu \gamma_5)=0[/itex]

Where I used at first [itex]Tr(AB)=Tr(BA)[/itex] and then [itex]\left \{ \gamma_5, \gamma^\mu \right \}=0[/itex].

For the [itex]\sigma^{\mu \nu} \equiv \frac{i}{2}[\gamma^\mu,\gamma^\nu] [/itex]
Well, since it's a commutor it's traceless...

[itex]Tr(\sigma^{\mu \nu}) \sim Tr(\gamma^\mu \gamma^\nu)-Tr(\gamma^\nu \gamma^\mu) =Tr(\gamma^\mu \gamma^\nu)-Tr(\gamma^\mu \gamma^\nu)=0[/itex]

Where I used the trace property [itex]Tr(AB)=Tr(BA)[/itex]

The rest is in a complete analogy with what you do for the 2x2 complex matrices with a basis [itex]\Gamma^A = \left \{ 1, \sigma^i \right \}[/itex] and when you write a general matrix:

[itex]M= \sum_B a_B \Gamma^B [/itex]

and want to find the coefficients [itex]a_B[/itex].
http://en.wikipedia.org/wiki/Pauli_matrices#Completeness_relation

The even more simple form is what you do to find the coeffecients for a vector in some basis.
[itex]\vec{v}= a_i x^i [/itex]
where you take the inner product with the basis vectors (the analogy to this is seen after you realize that the inner product is a scalar, as is the trace of a matrix)
 
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  • #12
Just as expected, samalkhaiat writes a stunning reply. :) Bravo!
 
  • #13
dextercioby said:
Just as expected, samalkhaiat writes a stunning reply. :) Bravo!

Thanks, it is always a pleasure to help someone understand something. Also, it is fun to do.
 

1. What is a spinorial field representation?

A spinorial field representation is a mathematical tool used in physics and other fields to describe and analyze the properties of spinors, which are mathematical objects that represent the intrinsic angular momentum of particles. It is a way of representing the mathematical objects that describe spinors in a particular coordinate system or space.

2. What is the significance of spinorial field representation in physics?

Spinors are important in physics because they describe the intrinsic spin of particles, which is a fundamental property that affects their behavior and interactions. Spinorial field representation allows scientists to study and manipulate these spinors to better understand the behavior of particles and their interactions with other particles and fields.

3. How is spinorial field representation related to quantum mechanics?

Spinors, and therefore spinorial field representation, are essential in quantum mechanics because they describe the spin of particles, which is a quantum property. In quantum mechanics, spinors are used to describe the spin states of particles, and spinorial field representation is used to analyze the behavior and interactions of these spin states.

4. Are there different types of spinorial field representations?

Yes, there are different types of spinorial field representations, each with its own mathematical properties and applications. Some common types include the Weyl representation, the Dirac representation, and the Majorana representation. Each type is suited for different purposes and may be used in different areas of physics and mathematics.

5. How is spinorial field representation used in other fields besides physics?

Spinorial field representation is not limited to physics and is also used in other fields such as mathematics, computer science, and engineering. In these fields, it is used to study and analyze spinors and their properties, as well as to develop new mathematical models and algorithms for various applications.

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