LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan’s fiscal year 2032, marking a major advancement in the exploration of primordial cosmology and fundamental physics. Orbiting the Sun-Earth Lagrangian point L2, this JAXA-led strategic L-class mission will conduct a comprehensive mapping of the CMB polarization across the entire sky. During its 3-year mission, LiteBIRD will employ three telescopes within 15 unique frequency bands (ranging from 34 through 448 GHz), targeting a sensitivity of 2.2 µK-arcmin and a resolution of 0.5◦ at 100 GHz. Its primary goal is to measure the tensor-to-scalar ratio r with an uncertainty δr = 0.001, including systematic errors and margin. If r ≥ 0.01, LiteBIRD expects to achieve a > 5σ detection in the ℓ = 2–10 and ℓ = 11–200 ranges separately, providing crucial insight into the early Universe. We describe LiteBIRD’s scientific objectives, the application of systems engineering to mission requirements, the anticipated scientific impact, and the operations and scanning strategies vital to minimizing systematic effects. We will also highlight LiteBIRD’s synergies with concurrent CMB projects.

Ghigna, T., Adler, A., Aizawa, K., Akamatsu, H., Akizawa, R., Allys, E., et al. (2024). The LiteBIRD mission to explore cosmic inflation. Intervento presentato a: Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave - 16 June 2024 through 22 June 2024, Yokohama, Japan [10.1117/12.3021377].

The LiteBIRD mission to explore cosmic inflation

Gervasi, Massimo;Zannoni, Mario;
2024

Abstract

LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan’s fiscal year 2032, marking a major advancement in the exploration of primordial cosmology and fundamental physics. Orbiting the Sun-Earth Lagrangian point L2, this JAXA-led strategic L-class mission will conduct a comprehensive mapping of the CMB polarization across the entire sky. During its 3-year mission, LiteBIRD will employ three telescopes within 15 unique frequency bands (ranging from 34 through 448 GHz), targeting a sensitivity of 2.2 µK-arcmin and a resolution of 0.5◦ at 100 GHz. Its primary goal is to measure the tensor-to-scalar ratio r with an uncertainty δr = 0.001, including systematic errors and margin. If r ≥ 0.01, LiteBIRD expects to achieve a > 5σ detection in the ℓ = 2–10 and ℓ = 11–200 ranges separately, providing crucial insight into the early Universe. We describe LiteBIRD’s scientific objectives, the application of systems engineering to mission requirements, the anticipated scientific impact, and the operations and scanning strategies vital to minimizing systematic effects. We will also highlight LiteBIRD’s synergies with concurrent CMB projects.
paper
B-mode polarization; cosmic inflation; cosmic microwave background; LiteBIRD; primordial gravitational waves; quantum gravity; space telescope;
English
Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave - 16 June 2024 through 22 June 2024
2024
Coyle, Laura E.
9781510675070
2024
13092
1309228
none
Ghigna, T., Adler, A., Aizawa, K., Akamatsu, H., Akizawa, R., Allys, E., et al. (2024). The LiteBIRD mission to explore cosmic inflation. Intervento presentato a: Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave - 16 June 2024 through 22 June 2024, Yokohama, Japan [10.1117/12.3021377].
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/523299
Citazioni
  • Scopus 0
  • ???jsp.display-item.citation.isi??? ND
Social impact