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The Swept-back Multipolar Magnetic Field of Neutron Stars: Application to NICER MSP J0030+0451

  • Authors: Anu Kundu, Constantinos Kalapotharakos, Zorawar Wadiasingh, Greg Olmschenk, Wendy F. Wallace, Alice K. Harding, Christo Venter, Demosthenes Kazanas

Anu Kundu et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 12.

Top and middle panels: model light curves for the RV1 and RV2 input field configurations, respectively, at truncation orders l ∈ {3, 5, 7, 10, 15} (colored lines), overlaid on the l = 18 reference (black points with NICER-like uncertainties). The χ2 values with respect to the reference light curve are indicated in the legend. (We note that these light curves would recover the exact RV1 and RV2 light curves of CK21 if the swept-back Bout were replaced by the corresponding static-vacuum configuration). Bottom panel: χ2 as a function of multipolar truncation order l for the above cases: RV1 (circles, black connecting line) and RV2 (squares, gray connecting line). Colors indicate the truncation order l, as shown in the legend.

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