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Note About the Spin Connection in General Relativity

Note About the Spin Connection in General Relativity

arXiv:1911.05283v2 [gr-qc] 22 Apr 2020 n enstegmamtie ntecre pc as: space [3] curved the [2], in formalism in matrices a further gamma in the developed Then defines and one . Cartan associ- spin fields by the gauge introduced the the this, gauge introduce general to to to a ated of and then and group be Lorentz space-time would curved transformation a of coordinate presence the in where httecvratdrvtv ftemti esri zero: is metric the of covariant the that edter,tefrinfils nQTtefrin lie group quantum Lorentz fermions the the a of SO QFT representation in dimensional In relevance four a fields. of in fermion con- fields the to theory, of needs field one type time another space curved sider in modified be must . odagbawt h nicmuainrule: anti-commutation the with algebra ford needn famti.I atclrhwvri sal- [1]: is requirements that main it connection two however affine satisfies an particular consider to In amenable more metric. ways a of independent Γ Here ffiecneto.Freapefravco h covariant the by: vector given a an is for of re- derivative example is terms For in tensor, connection. a written affine derivative of covariant behavior the general by the placed obtain to order in where quantities uvdsaeand space curved ∗ [email protected] )t emti optbewihaon oasking to amount which compatible metric be to b) aigetbihdhwadrvtv fatno field tensor a of derivative a how established Having )t etrinfe,ie Γ i.e. free, torsion be to a) ngnrlrltvt h riaydrvtv fatensor, a of derivative ordinary the relativity general In (3 , η )gvnb h am arcswihsa Clif- a span which matrices gamma the by given 1) γ µν ρ ab µ ∆ eedo h coordinate, the on depend ersnstean oncinwihmybe may which connection affine the represents a steMnosimti.Tentrlapproach natural The metric. Minkowski the is ρ e g a µ ainlIsiueo hsc n ula niern OBo PO Engineering Nuclear and of Institute National ∂ µν xcl ihtesi oncinoti hog h erdf tetrad the through Lo obtain to gauged connection generalized the spin bilinears the on with theory, fermion exactly the der of we of work properties covariance this general space-time In the connection. on affine fro the only stems , and a formalism co to ”vielbein” spin ciated so-called the fields the gauge to related corresponding the introducing by and r aldatta n aif h relation: the satisfy and tetrad a called are µ ngnrlrltvt h emosaetetdfo h pers the from treated are fermions the relativity general In V = ν ∂ → a ρ g { steidxi h a pc.The space. flat the in index the is g D γ µν γ µν µ a µ oeaottesi oncini eea relativity general in connection spin the about Note ( γ , V − x = ν = ) b Γ } = e ρµ σ a µ 2 = µν ρ ∂ e γ g b ν µ σν a η Γ = V e η ab ν a µ ab − , . − , νµ ρ Γ µ Γ ρν σ . steidxi the in index the is µν ρ g σµ V ρ . 0 = . eaaJora Renata (3) (2) (1) (4) (5) where h emo oain eiaiewtotteueo the assump- natural of some tions. use making only the by without formalism vielbein derivative covariant fermion the their of formalism own. entire an and curvilinear complicated structures the and mathematical new only usually of involved These terms in coordinates. formalism vielbein use the the without of derivative covariant fermion introduce to pc aif eeaie lffr ler ihteanti the curved with the algebra in relation: Clifford commutation matrices generalized gamma a the satisfy that space considered is It matrices ini httequantity the that is tion h uvdsaetm.Te h quantity, the Then space-time. curved the ueoearvso h ilenpostulate: parallel vielbein of com- the indices of operations curved arrives and the one flat mute on that projection further and transport requires one If where where h emo ed uhta h uniyi q (10) this that Eq. Consider as, in tensor. expressed quantity is rank derivative the second covariant a that as such transforms fields fermion the tensor. two rank a rmE.()t be: to (7) Eq. from hntecvratdrvtv faDrcfrini the in as: fermion written Dirac is time a space of curved derivative covariant the Then osdrtoDrcfrin and Ψ fermions Dirac two Consider for expression exact the derive will we following the In [4] literature the in made been have attempts Various eaeitrse nwiigacvratdrvtv for derivative covariant a writing in interested are We a ∗ h eea tutr htcnb asso- be can that structure general the m h uvdsae u eutcoincides result Our space. curved the D ω σ D ab ρn m ormalism. ncin hspoeuei intimately is procedure This nnection. ρ γ ρ G6 uhrs-auee Romania Bucharest-Magurele, MG-6, x etv ftegue oet group Lorentz gauged the of pective v h orc pncneto based connection spin correct the ive a nrdcdi q 1 hudtasomas transform should (1) Eq. in introduced was µ e = stesi oncinwihcnb extracted be can which connection spin the is et ymtyado h known the on and symmetry rentz µ m ω e ntecre pc ie h anassump- main The time. space curved the in 2 i ν m µ mn = [ γ Γ D a ∂ σµ ν = ρ γ , ρ D = Ψ e e e µ m b { σn ρ ]. ν m γ = Ψ ( x µ Γ D − ∂ γ , ) σµ ν ρ ρ Ψ − ∂ ¯ Ψ [ ν ∂ e µ Ψ γ ¯ } ρ Γ σn e − µ γ + Ψ ν m ρµ ν 2 = rnfrsa etrin vector a as transforms Ψ µ + e 4 i Ψ] e νn ω ν m g e X , ρ ab ν m µν . − ρ σ ∂ Ψ . ω µ ab , e ρn m n h gamma the and Ψ Ψ ¯ νn e , mu n = 0 = , (10) (11) (9) (6) (7) (8) 2 where Xρ may contain in it gamma matrices in the curved behaves as a second rank tensor. Since the term in the space. first line of Eq. (21) behaves like a tensor then also the We make the assumption that the covariant derivative terms on the second plus the third line must behave as a operator is linear, although acting with different expres- second rank tensor. Then, sion on various fields. Consider the quantity: µ αβ αβ µ Ψ¯ iγ Aραβ σ Ψ − Ψ¯ iAραβσ γ Ψ+ ¯ Y µ, ¯ µ µ ¯ σ µ ΨΨ (12) Ψ(∂ργ )Ψ+Γρσ Ψγ Ψ= Tρ , (22) µ µ where Tρ is an arbitrary tensor expressed in terms of the where Y is a vector in the curved space. Then, fermion fields. Since there is not such tensor besides those µ introduced at this point with the correct mass Dρ[ΨΨ¯ Y ], (13) one can consider this tensor zero. is a rank two tensor. The linearity of the operator implies One may rewrite Eq. (22) as: that the quantity, µ αβ µ σ µ iAραβ[γ , σ ]= −Γρσγ − ∂ργ . (23) [D (ΨΨ)]¯ Y µ + ΨΨ¯ D Y µ, (14) ρ ρ In the flat space we know that: is also a second rank tensor. Further on then, 1 [γa, σbc]= i(ηabγc − ηacγb). (24) 2 Dρ[ΨΨ]¯ = [DρΨ]Ψ¯ + Ψ¯ DρΨ, (15) Since we consider in the curved space a similar Clifford ¯ is also a second rank tensor. Since ΨΨ is a scalar the algebra this time with the gamma matrices space time only second rank tensor that one may form from it is: dependent the same relation should work if the flat in- dices would be replaced by the curved indices. Then Eq. ∂ [ΨΨ]¯ . (16) ρ (23) becomes: Eqs. (11), (15) and (16) then imply that: µ β µ σ µ −4Aρβγ = −Γρσγ − ∂ργ . (25) D Ψ=¯ ∂ Ψ¯ − Ψ¯ X . (17) ρ ρ ρ We multiply Eq. (25) by γλ and take the trace to obtain:

In order to determine the composition of Xρ in the µ 1 µ 1 λ µ 16 dimensional Lorentz space associated to the gamma A = Γ + Tr[γ ∂ργ ]. (26) ρ λ 4 ρλ 16 matrices we take into account the fact that the covari- ant derivative is a result of gauging the Lorentz symme- Finally the covariant derivative for the fermion fields is try and therefore should be an expansion in σµν . Then written in terms of only quantities in the curved space without loss of generality one may write: as: αβ D ∂ iAα σ β , Xρ = −iAραβσ , (18) ρΨ= ρΨ − ρβ α Ψ (27) α In summary one has: where Aρβ is given in Eq. (26). Next we will show that the spin connection introduced αβ DρΨ= ∂ρΨ − iAραβ σ in Eq. (27) is identical to that in Eq. (9). For that we βα write: DρΨ=¯ ∂ρΨ − iAραβ σ . (19) −iAµ σ λ = One can expand Eq. (10) which leads to: ρ λ µ 1 µ 1 λ µ λ µ −i [Γρλ + Tr[γ ∂ργ ]]σµ = Dρ[Ψ¯γ Ψ] = 4 4 µ µ (∂ρΨ)¯ γ Ψ+ Ψ[¯ ∂ργ ]Ψ + 1 µ µ λ ab λ cd −i [Γ + ∂ρea eb η ]eµced σ = ¯ µ µ ¯ σ 4 ρλ Ψγ ∂ρΨ+ΓρσΨγ Ψ. (20) 1 µ λ µ cd −i [Γ eµce + ∂ρe eµc]σ . (28) If we introduce the expression in Eq. (19) into Eq. 4 ρλ d d (20) one obtains that the quantity, Eq. (28) shows that the exact expression of the spin µ µ connection obtained through the vielbein formalism can DρΨ¯ γ Ψ+ Ψ¯ γ DρΨ+ be obtained by using only quantities defined in the curved ¯ µ αβ ¯ αβ µ +Ψiγ Aραβ σ Ψ − ΨiAραβσ γ Ψ+ space with the gamma matrices in the curved space sat- ¯ µ µ ¯ σ Ψ(∂ργ )Ψ+ΓρσΨγ Ψ, (21) isfying a similar Clifford algebra.

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