Orthochronous Lorentz group
The orthochronous Lorentz group
since
Discussion
First note that by definition for all
,1 ( Ξ π π ) β πΏ Ξ π π π π π Ξ π π = π π π and taking adjoints
Ξ π π π π π Ξ π π = π π π the
component of which yield 0 0 β ( Ξ 0 0 ) 2 + Ξ π 0 Ξ π 0 = Ξ π 0 π π π Ξ π 0 = π 0 0 = β 1 β ( Ξ 0 0 ) 2 + Ξ 0 π Ξ 0 π = Ξ 0 π π π π Ξ 0 π = π 0 0 = β 1 implying the properties
( Ξ 0 0 ) 2 = 1 + Ξ π 0 πΏ π π Ξ π 0 β₯ 1 = 1 + Ξ 0 π πΏ π π Ξ 0 π β₯ 1 the former yields equality iff
for Ξ π 0 = 0 the latter yields equality iff π = 1 , 2 , 3 for each Ξ 0 π = 0 . Thus in particular π iff Ξ 0 0 = 1 for each Ξ 0 π = Ξ π 0 = 0 , in which case π . Now since ( Ξ π π ) β O ( 3 ) , ( Ξ 0 0 ) 2 β₯ 1 which splits Ξ 0 0 β β β ( β 1 , 1 ) into disconnected components based on the sign of πΏ . Ξ 0 0
Proof of defining property
Let
. Consider a timelike vector Ξ β O β ( 3 , 1 ) , i.e. π£ β β 4 implying π π π π£ π π£ π < 0 . Now if π£ 0 π£ 0 > π£ π π£ π , then π£ 0 > 0 Ξ 0 π π£ π = Ξ 0 0 π£ 0 + Ξ 0 π π£ π β₯ Ξ 0 0 π£ 0 β β Ξ 0 π Ξ 0 π β π£ π π£ π = Ξ 0 0 π£ 0 β β ( Ξ 0 0 ) 2 + 1 β π£ π π£ π > Ξ 0 0 π£ 0 β Ξ 0 0 π£ 0 = 0 Now let
, and Ξ β² β O β ( 3 , 1 ) be timelike with π£ . It follows π£ 0 < 0 is timelike with β π£ and π£ 0 > 0 , thus β Ξ β² β O β ( 3 , 1 ) Ξ 0 π ( β 1 ) π£ β² π > 0 βΉ Ξ 0 π π£ β² π < 0 ( β 1 ) Ξ β² 0 π π£ π > 0 βΉ Ξ β² 0 π π£ π < 0 ( β 1 ) Ξ β² 0 π ( β 1 ) π£ β² π > 0 βΉ Ξ β² 0 π π£ β² π > 0 Hence an arbitrary
preserves the direction of time iff Ξ β O ( 3 , 1 ) and reverses the direction of time iff Ξ 0 0 β₯ 1 . Ξ 0 0 β€ β 1 From this it immediately follows that
is a group, since if O β ( 3 , 1 ) and Ξ preserve the direction of time so too must Ξ β² and Ξ Ξ β² . Furthermore it follows that Ξ β 1 is a Normal subgroup since for any O β ( 3 , 1 ) and Ξ β O β ( 3 , 1 ) we the result of Ξ β² β O β ( 3 , 1 ) will preserve the direction of time. Ξ β² β 1 Ξ Ξ β²
Alternate proof of normal subgroup
Define
. Let π ( Ξ ) = s g n β‘ ( Ξ 0 0 ) . If Ξ , Ξ β² β O ( 3 , 1 ) then applying the inequalities in ^eq1 and the Cauchy-Schwarz inequality π ( Ξ ) π ( Ξ β² ) = 1 ( Ξ Ξ β² ) 0 0 = Ξ 0 π Ξ β² π 0 = Ξ 0 0 Ξ β² 0 0 + Ξ 0 π Ξ β² π 0 β₯ Ξ 0 0 Ξ β² 0 0 β β£ Ξ 0 π Ξ π 0 β£ = β£ Ξ 0 0 β£ β£ Ξ β² 0 0 β£ β β£ Ξ 0 π Ξ π 0 β£ > β Ξ 0 π Ξ 0 π β Ξ π 0 Ξ π 0 β β£ Ξ 0 π Ξ π 0 β£ β₯ 0 and indeed
since otherwise it would have null determinant. Similarly if ( Ξ Ξ β² ) 0 0 > 0 π = β 1 ( Ξ Ξ β² ) 0 0 = Ξ 0 π Ξ β² π 0 = Ξ 0 0 Ξ β² 0 0 + Ξ 0 π Ξ β² π 0 β€ Ξ 0 0 Ξ β² 0 0 + β£ Ξ 0 π Ξ π 0 β£ = β β£ Ξ 0 0 β£ β£ Ξ β² 0 0 β£ + β£ Ξ 0 π Ξ π 0 β£ < β Ξ 0 π Ξ 0 π β Ξ π 0 Ξ π 0 β β£ Ξ 0 π Ξ π 0 β£ β€ 0 and by the same
since otherwise it would have null determinant. Hence ( Ξ Ξ β² ) 0 0 < 0 is a group homomorphism and its kernel π : O ( 3 , 1 ) β β€ 2 is a normal subgroup. k e r β‘ π = O β ( 3 , 1 )
Footnotes
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2018. From the Lorentz Group to the Celestial Sphere, Β§1.3, p. 9 β©