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Type IIB Einstein Frame Pseudoaction
Conditional pointwise Weyl rewrite of the source-free two-derivative type IIB pseudoaction. The full local divergence from the NS sector is retained; dropping it from the integrated action requires zero boundary flux, while compactly supported bulk variations are unaffected. The five-form constraint remains separate.
Statement
Assume the conventions and action of Type IIB Two Derivative Supergravity Pseudoaction and set on the oriented Lorentzian ten-manifold. For any covariant -form , , while . Therefore the Einstein-frame action is bulk-equivalent, for compactly supported variations, to
More precisely, the full NS local density includes the additional total-divergence term from String Einstein Frame NS Action Calculation; removing its integral requires the boundary flux to vanish. The middle-degree Hodge star is unchanged by this Weyl rescaling, so the separately imposed constraint is .
Statement references
Supergravity Conventions And Normalizations
Type IIB Two Derivative Supergravity Pseudoaction
String Einstein Frame NS Action Calculation
Lorentzian Hodge Star in Ten Dimensions
Existence and Five-Form Properties of the Lorentzian Hodge Star
Conformal Scaling of the Ten-Dimensional Lorentzian Hodge Star
Facts & Assumptions
Given: A smooth real scalar , the two metrics , the fields and norms in [F1], and the planned string-frame pseudoaction.
Type IIB Two Derivative Supergravity Pseudoaction: the RR terms are with common coefficient , and the Chern–Simons term is the metric-independent integral .
String Einstein Frame NS Action Calculation: writing , the complete transformed NS density is . By [F5], , so this is ; the last summand is a total divergence.
Conformal Scaling of the Ten-Dimensional Lorentzian Hodge Star: in dimension ten, for a -form.
Type IIB Five Form Self Duality Constraint: impose the five-form equation only after varying the pseudoaction.
Supergravity Conventions And Normalizations: use Lorentzian signature , , , and ; keep distinct from the asymptotically shifted physical .
Proof
Write with , using the frame relation in [F5]. In ten dimensions the determinant contributes , while each inverse metric in the squared norm of a covariant -form contributes . Thus and , as stated.
Multiplying the measure and norm factors gives for a -form kinetic density: this is for , for , and for . The action coefficient already contains the additional factor for the five-form and it is unchanged. The Chern–Simons integral contains only differential forms and orientation, so no metric scaling occurs.
By [F2], the raw NS three-form term is . Since the convention [F5] defines , this raw contraction equals , which is the coefficient in the Statement. The other NS terms give and the explicitly retained total divergence . Compactly supported variations of its local current integrate to zero by the supplier's stated hypothesis, but its unvaried value is removed only if the boundary flux vanishes. Combining this NS result with step 2.1 proves the bulk-equivalent action formula without discarding an unqualified boundary term.
Here , so [F3] on has exponent ; therefore . Applying [F4] after the Weyl rewrite leaves this same self-duality equation as a separate constraint, not a term varied in either action.
Depends on
Supergravity Conventions And Normalizations
Type IIB Two Derivative Supergravity Pseudoaction
Type IIB Five Form Self Duality Constraint
String Einstein Frame NS Action Calculation
Lorentzian Hodge Star in Ten Dimensions
Existence and Five-Form Properties of the Lorentzian Hodge Star
Conformal Scaling of the Ten-Dimensional Lorentzian Hodge Star