SPECTER: An Instrument Concept for CMB Spectral Distortion Measurements with Enhanced Sensitivity
arXiv:2409.12188 · doi:10.1088/1475-7516/2025/10/088
Abstract
Deviations of the cosmic microwave background (CMB) energy spectrum from a perfect blackbody uniquely probe a wide range of physics, ranging from fundamental physics in the primordial Universe (-distortion) to late-time baryonic feedback processes (-distortion). While the -distortion can be detected with a moderate increase in sensitivity over that of COBE/FIRAS, the CDM-predicted -distortion is roughly two orders of magnitude smaller and requires substantial improvements, with foregrounds presenting a serious obstacle. Within the standard model, the dominant contribution to arises from energy injected via Silk damping, yielding sensitivity to the primordial power spectrum at wavenumbers Mpc. Here, we present a new instrument concept, SPECTER, with the goal of robustly detecting . The instrument technology is similar to that of LiteBIRD, but with an absolute temperature calibration system. Using a Fisher approach, we optimize the instrument's configuration to target while marginalizing over foreground contaminants. Unlike Fourier-transform-spectrometer-based designs, the specific bands and their individual sensitivities can be independently set in this instrument, allowing significant flexibility. We forecast SPECTER to observe the CDM-predicted -distortion at (10) assuming an observation time of 1 (4) year(s) (corresponding to mission duration of 2 (8) years), after foreground marginalization. Our optimized configuration includes 16 bands spanning 1-2000 GHz with degree-scale angular resolution at GHz and 1100 total detectors. SPECTER will additionally measure the -distortion at sub-percent precision and its relativistic correction at percent-level precision, yielding tight constraints on the total thermal energy and mean temperature of ionized gas.
arXiv comment47 pages, 15 figures, updated to match JCAP version
References in corpus (72)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- The Herschel-SPIRE instrument and its in-flight performance
- The Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set
- The Temperature of the Cosmic Microwave Background
- New cosmological constraints on primordial black holes
- The Primordial Inflation Explorer (PIXIE): A Nulling Polarimeter for Cosmic Microwave Background Observations
- The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: II. Model of the Interplanetary Dust Cloud
- Cosmic microwave background limits on accreting primordial black holes
- The evolution of CMB spectral distortions in the early Universe
- Planck 2018 results. III. High Frequency Instrument data processing and frequency maps
- Diffuse Galactic Emission from Spinning Dust Grains
- Relativistic Corrections to the Sunyaev-Zel'dovich Effect for Clusters of Galaxies
- Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
- Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum
- Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data
- CMB at 2x2 order: the dissipation of primordial acoustic waves and the observable part of the associated energy release
- Relativistic corrections to the Sunyaev-Zel'dovich effect
- Planck 2013 results. XIII. Galactic CO emission
- PRISM (Polarized Radiation Imaging and Spectroscopy Mission): An Extended White Paper
- SZ effects in the Magneticum Pathfinder Simulation: Comparison with the Planck, SPT, and ACT results
- Planck early results: first assessment of the High Frequency Instrument in-flight performance
- Power Spectrum Constraints from Spectral Distortions in the Cosmic Microwave Background
- Systematic Bias in Cosmic Shear: Beyond the Fisher Matrix
- Calibrating the Nonlinear Matter Power Spectrum: Requirements for Future Weak Lensing Surveys
- A Limit on Primordial Small-Scale Magnetic Fields from CMB Distortions
- Limits on primordial black holes from distortions in cosmic microwave background
- Planck 2013 results. XIV. Zodiacal emission
- Rethinking CMB foregrounds: systematic extension of foreground parameterizations
- Teasing bits of information out of the CMB energy spectrum
- Which spectral distortions does CDM actually predict?
- Design, Implementation and Testing of the MAP Radiometers
- Beyond y and μ: the shape of the CMB spectral distortions in the intermediate epoch, 1.5x10^4 < z < 2x10^5
- Distinguishing different scenarios of early energy release with spectral distortions of the cosmic microwave background
- Green's function of the cosmological thermalization problem
- Taking the Universe's Temperature with Spectral Distortions of the Cosmic Microwave Background
- Carbon monoxide line emission as a CMB foreground: tomography of the star-forming universe with different spectral resolutions
- Signals From the Epoch of Cosmological Recombination
- Line-Intensity Mapping: Theory Review
- The synergy between CMB spectral distortions and anisotropies
- Prospects for Measuring Cosmic Microwave Background Spectral Distortions in the Presence of Foregrounds
- Sunyaev-Zeldovich signal processing and temperature-velocity moment method for individual clusters
- Cosmic Microwave Background constraint on residual annihilations of relic particles
- Constraining primordial magnetic fields with distortions of the black-body spectrum of the cosmic microwave background: pre- and post-decoupling contributions
- Does Bose-Einstein condensation of CMB photons cancel μ distortions created by dissipation of sound waves in the early Universe?
- Cosmological constraints from CMB distortion
- Dissecting the high-z interstellar medium through intensity mapping cross-correlations
- Forecasts for CMB μ- and i-type spectral distortion constraints on the primordial power spectrum on scales 8 < k < 10^4 Mpc^-1 with the future Pixie-like experiments
- The ARCADE 2 Instrument
- The Cosmic Thermal History Probed by Sunyaev-Zeldovich Effect Tomography
- CosmoSpec: Fast and detailed computation of the cosmological recombination radiation from hydrogen and helium
- -Distortions or Running: A Guaranteed Discovery from CMB Spectrometry
- Ultra-sensitive Super-THz Microwave Kinetic Inductance Detectors for future space telescopes
- Testing Inflation and Curvaton Scenarios with CMB Distortions
- Horn Coupled Multichroic Polarimeters for the Atacama Cosmology Telescope Polarization Experiment
- Multi-Chroic Feed-Horn Coupled TES Polarimeters
- Baryonic feedback biases on fundamental physics from lensed CMB power spectra
- A 4-8 GHz Kinetic Inductance Travelling-Wave Parametric Amplifier Using Four-Wave Mixing with Near Quantum-Limit Noise Performance
- CMB spectral distortions from the decay of causally generated magnetic fields
- Spectral Distortion of the CMB by the Cumulative CO Emission from Galaxies throughout Cosmic History
- CMB Distortions from Damping of Acoustic Waves Produced by Cosmic Strings
- BoloCalc: a sensitivity calculator for the design of Simons Observatory
- Calibration Method and Uncertainty for the Primordial Inflation Explorer (PIXIE)
- Percent-level constraints on baryonic feedback with spectral distortion measurements
- Extragalactic CO emission lines in the CMB experiments: a forgotten signal and a foreground
- Demonstration of 220/280 GHz Multichroic Feedhorn-Coupled TES Polarimeter
- How to measure CMB spectral distortions with an imaging telescope
- FSD: Frequency Space Differential measurement of CMB spectral distortions
- Cosmoglobe: Simulating zodiacal emission with ZodiPy
- Importance of intracluster scattering and relativistic corrections from tSZ effect with Cosmic Infrared Background
- On the contributions of extragalactic CO emission lines to ground-based CMB observations