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The Dipole of the Pantheon+SH0ES Data

Francesco Sorrenti · CERN

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About

We determine the dipole in the Pantheon+ data. We find that, while its amplitude roughly agrees with the dipole found in the cosmic microwave background which is attributed to the motion of the solar system with respect to the cosmic rest frame, the direction is different at very high significance. While the amplitude depends on the lower redshift cutoff, the direction is quite stable. For redshift cuts of order $z_{\rm cut} \simeq 0.05$ and higher, the dipole is no longer detected with high statistical significant. An important rôle seems to be played by the redshift corrections for peculiar velocities..

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The talk

  1. The Dipole of the Pantheon+SH0ES Data 2023-06-01 · 8 min · CERN's player

Credits and licence

Institution
CERN
Department
Eucapt Conferences
Speaker
Francesco Sorrenti
Year
2023
Language
English
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
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