1994
DOI: 10.1016/0550-3213(94)90530-4
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Supersymmetric calculation of mixed Kähler-gauge and mixed Kähler-Lorentz anomalies

Abstract: We present a manifestly supersymmetric procedure for calculating the contributions from matter loops to the mixed Kähler-gauge and to the mixed Kähler-Lorentz anomalies in N = 1, D = 4 supergravity-matter systems. We show how this procedure leads to the well-known result for the mixed Kähler-gauge anomaly. For general supergravity-matter systems the mixed Kähler-Lorentz anomaly is found to contain a term proportional to R 2 with a background field dependent coefficient as well as terms proportional to (C mnpq … Show more

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Cited by 23 publications
(35 citation statements)
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“…Using this Lagrangian, we now compute the one-loop moduli-gravity-gravity anomalous threshold correction [8]. This must actually be carried out in the conventional (string frame) superspace formalism and then transformed to Kähler superspace [9]. We also compute the relevant superGreen-Schwarz graphs.…”
Section: Superspace Formalismmentioning
confidence: 99%
“…Using this Lagrangian, we now compute the one-loop moduli-gravity-gravity anomalous threshold correction [8]. This must actually be carried out in the conventional (string frame) superspace formalism and then transformed to Kähler superspace [9]. We also compute the relevant superGreen-Schwarz graphs.…”
Section: Superspace Formalismmentioning
confidence: 99%
“…(2), on the dilaton field. Note that in the case of Z 3 and Z 7 orbifolds the moduli-dependent part of ∆ a vanishes, and therefore it cannot contribute to the cancellation of the anomaly; the cancellation comes entirely from the variation of S; so, in [29].…”
Section: The Loop-corrected Four-derivatives Termmentioning
confidence: 99%
“…String loop corrections have been much studied in the literature, especially for Z N orbifold compactifications of the heterotic string [19][20][21][22][23][24][25][26][27][28][29][30][31][32][33][34], and we can therefore ask whether, at least in some compactification scheme, they fulfill the non-trivial properties needed for a graceful exit. In particular, corrections to the Kähler potential are known at all loops; this will be very important for our analysis, since in order to follow the cosmological evolution into the strong coupling regime, a knowledge of the first few terms of the perturbative expansion is not really sufficient, and one must have at least some glimpse into the structure at all loops.…”
Section: Introductionmentioning
confidence: 99%
“…So the simplest way to see how this is obtained is to follow the argument given in subsection (2.2) above. However these authors use instead (a modified version) of the non-local anomaly action of [14].…”
Section: The Bagger Poppitz Moroi Calculation [6]mentioning
confidence: 99%
“…In [6] it is stated that the effective action must reflect separately the anomalies under separate Weyl and Kähler transformations (unlike the one in [14]) and indeed theirs does that. However it is non-local and not generally covariant.…”
Section: The Bagger Poppitz Moroi Calculation [6]mentioning
confidence: 99%