LiteBIRD: an all-sky cosmic microwave background probe of inflation

The Litebird mission will map polarized fluctuations in the cosmic microwave background (CMB) to search for the signature of gravitational waves from inflation, potentially opening a window on the Universe a fraction of a second after the Big Bang. CMB measurements from space give access to the largest angular scales and the full frequency range to constrain Galactic foregrounds, and Litebird has been designed to take best advantage of the unique window of space. Litebird will have a powerful ability to separate Galactic foreground emission from the CMB due to its 15 frequency bands spaced between 40 and 402 GHz and sensitive 100-mK bolometers. Litebird will provide stringent control of systematic errors due to the benign thermal environment at the second Lagrange point, L2, 20-K rapidly rotating half-wave plates on each telescope, and the ability to crosscheck its results by measuring both the reionization and recombination peaks in the B-mode power spectrum. Litebird would be the next step in the series of CMB space missions, COBE, WMAP, and Planck, each of which has given landmark scientific discoveries. The 4,736 detectors are distributed between three 5-K cooled telescopes, called the Low-, Medium-, and High-frequency telescopes (LFT, MFT, and HFT), with 31 arc-min resolution at 140 GHz. Litebird will map 20 times deeper than Planck, with a total error of \u3b4r < 0.001, conservatively assuming equal contributions of statistical error, systematic error, and margin. Litebird will be designed to discover or disfavor the best motivated inflation models \u2013 singlefield models that naturally explain the observed value of the spectral index of primordial density perturbations, with a characteristic scale of the potential comparable to or larger than the Planck scale. Litebird will also measure the optical depth to reionization to cosmicvariance-limited error, enabling ground-based high-resolution CMB experiments to measure the sum of neutrino masses. The proposed mission will be a partnership. Japan Aerospace Exploration Agency (JAXA) will provide the launch, spacecraft, Joule-Thomson coolers, LFT and its wave-plate. Europe will build the MFT and HFT, their waveplates, and the 100-mK cooler. Canada will contribute the 300-K detector readout electronics. The U.S. will build the detector arrays, cold readout electronics, and the 1.8-K cooler likely through a NASA mission of opportunity cost capped at $75M. In May 2019, JAXA selected Litebird as a \u201cstrategic L-class\u201d mission for launch in early 2028. The total mission cost is estimated to be approximately$500M, and therefore the U.S. contribution is highly leveraged. Finally, Litebird technologies have been tested or will be tested in the near future on ground-based experiments. Litebird\u2019s ability to measure the entire sky at the largest angular scales with 15 frequency bands is complementary to that of ground-based experiments such as South Pole Observatory, Simons Observatory, and CMB-S4, which will focus on deep observations of low-foreground sky. Litebird can provide valuable foreground information for ground-based experiments and ground-based experiments can improve Litebird\u2019s observations with high-resolution lensing data

Concept design of the LiteBIRD satellite for CMB B-mode polarization

International audienceLiteBIRD is a candidate for JAXA’s strategic large mission to observe the cosmic microwave background (CMB) polarization over the full sky at large angular scales. It is planned to be launched in the 2020s with an H3 launch vehicle for three years of observations at a Sun-Earth Lagrangian point (L2). The concept design has been studied by researchers from Japan, U.S., Canada and Europe during the ISAS Phase-A1. Large scale measurements of the CMB B-mode polarization are known as the best probe to detect primordial gravitational waves. The goal of LiteBIRD is to measure the tensor-to-scalar ratio (r) with precision of r < 0:001. A 3-year full sky survey will be carried out with a low frequency (34 - 161 GHz) telescope (LFT) and a high frequency (89 - 448 GHz) telescope (HFT), which achieve a sensitivity of 2.5 μK-arcmin with an angular resolution 30 arcminutes around 100 GHz. The concept design of LiteBIRD system, payload module (PLM), cryo-structure, LFT and verification plan is described in this paper

Optical Characterization of OMT-Coupled TES Bolometers for LiteBIRD

International audienceFeedhorn- and orthomode transducer- (OMT) coupled transition edge sensor (TES) bolometers have been designed and micro-fabricated to meet the optical specifications of the LiteBIRD high frequency telescope (HFT) focal plane. We discuss the design and optical characterization of two LiteBIRD HFT detector types: dual-polarization, dual-frequency-band pixels with 195/280 GHz and 235/337 GHz band centers. Results show well-matched passbands between orthogonal polarization channels and frequency centers within 3% of the design values. The optical efficiency of each frequency channel is conservatively reported to be within the range 0.64-0.72, determined from the response to a cryogenic, temperature-controlled thermal source. These values are in good agreement with expectations and either exceed or are within 10% of the values used in the LiteBIRD sensitivity forecast. Lastly, we report a measurement of loss in Nb/SiN x/Nb microstrip at 100 mK and over the frequency range 200-350 GHz, which is comparable to values previously reported in the literature