A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background

Abstract

This paper presents a measurement of the angular power spectrum of the Cosmic Microwave Background from l=75 to l=1025 (~10' to 5 degrees) from a combined analysis of four 150 GHz channels in the BOOMERANG experiment. The spectrum contains multiple peaks and minima, as predicted by standard adiabatic-inflationary models in which the primordial plasma undergoes acoustic oscillations. These results significantly constrain the values of Omega_tot, Omega_b h^2, Omega_c h^2 and n_s.

changes to reflect version accepted by ApJ

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• Power-law solutions and accelerated expansion in scalar-tensor theories
• Determining Foreground Contamination in CMB Observations: Diffuse Galactic Emission in the MAXIMA-I Field
• Feedback Processes in Early-Type Galaxies
• Light mass galileon and late time acceleration of the Universe
• Interacting generalized ghost dark energy in non-flat universe
• Asymptotic behavior of Cardassian cosmologies with exponential potentials
• LRS Bianchi I model with bulk viscosity in f(R,T) gravity
• Unified Model for Inflation and Dark Energy with Planck-Scale Pseudo-Goldstone Bosons
• Gravitation, electromagnetism and the cosmological constant in purely affine gravity
• Cosmological dynamics of scalar fields with O(N) symmetry
• Search for very high energy gamma-rays from WIMP annihilations near the Sun with the Milagro Detector
• Comparing teh holographic principle inspired dark energy models
• Entropy and statefinder diagnosis in chameleon cosmology
• Solar System Constraints on a Cosmologically Viable $f(R)$ Theory
• Interacting entropy-corrected holographic scalar field models in non-flat universe
• Anisotropic evolution of 5D Friedmann-Robertson-Walker spacetime
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Scalar Perturbations in Synchronous Gauge
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• Some doubts on the validity of the foreground Galactic contribution subtraction from microwave anisotropies
• The amplitude of mass fluctuations and mass density of the Universe constrained by strong gravitational lensing
• Neutron Diffusion and Nucleosynthesis in an Inhomogeneous Big Bang Model
• Gravitational Coupling and Dynamical Reduction of The Cosmological Constant
• Hamiltonian perturbation theory in f(R) gravity
• Observational Constraints on Axions as Quintessence in String Theory
• Cosmology With Axionic-quintessence Coupled with Dark Matter
• Fast calculation of the Fisher matrix for cosmic microwave background experiments
• Lensed Density Perturbations in Braneworlds: An Alternative to Perturbations from Inflation
• UHECR as Decay Products of Heavy Relics? The Lifetime Problem
• Late-time acceleration with steep exponential potentials
• WMAP Constraints on Quintessence
• The Revival of Cosmic Strings
• Brane gas-driven bulk expansion as a precursor stage to brane inflation
• Effect of component separation on the temperature distribution of the CMB
• Strong lensing, cosmology and lensing halos
• Holographic Inflation
• The universe dynamics in the tachyon cosmology with non-minimal coupling to matter
• Conformal symmetry of gravity and the cosmological constant problem
• Probing modified gravity in cosmic filaments
• Transition from decelerated to accelerated cosmic expansion in braneworld universes
• Applications to cosmological models of a complex scalar field coupled to a U(1) vector gauge field
• Why CMB physics?
• Ghost dark energy with sign-changeable interaction term
• Comments on Scalar-Tensor Representation of $f(R)$ Theories
• Scalar Field as Dark Energy Accelerating Expansion of the Universe
• Scale-Free model for governing universe dynamics
• Non-Minimal Quintessence With Nearly Flat Potential
• Spectral Indications of thermal Sunyaev-Zel'dovich Effect in Archeops and WMAP Data
• The Star Formation Rate Intensity Distribution Function -- Comparison of Observations with Hierarchical Galaxy Formation
• Unsqueezing of standing waves due to inflationary domain structure
• Thermodynamics of charged rotating dilaton black branes coupled to logarithmic nonlinear electrodynamics
• Late-time-accelerated expansion arisen from gauge fields in an anisotropic background and a fruitful trick for Noether's approach
• Is there a common origin for the WMAP low multipole and for the ellipticity in BOOMERanG CMB maps?
• Overproduction of primordial helium-4 in the presence of neutrino oscillations
• Universal procedure to cure future singularities of dark energy models
• Dynamical systems analysis of an interacting scalar field model in an anisotropic universe
• Anisotropies in the redshift-space correlations of galaxy groups and clusters II: Analysis of observational cluster samples
• CMB Power Spectrum Estimation for the Planck Surveyor
• A canonical formalism of f(T)-type gravity in terms of Lie derivatives
• Super-horizon cosmic string correlations
• The Infuence of Omega_baryon on High-Redshift Structure
• Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
• CMB Anisotropy Constraints on Flat-Lambda and Open CDM Cosmogonies from DMR, UCSB South Pole, Python, ARGO, MAX, White Dish, OVRO, and SuZIE Data
• Using bright ellipticals as dark energy cosmic clocks
• First Results from the Arcminute Cosmology Bolometer Array Receiver
• `Hyper Parameters' Approach to Joint Estimation: Applications to Cepheid-Calibrated Distances and X-Ray Clusters
• Accelerating expansion of the universe may be caused by inhomogeneities
• Accurate estimation of angular power spectra for maps with correlated masks
• The cosmological constant and the paradigm of adiabaticity
• Constraining $f(R)$ Theories with Temporal Variation of Fine Structure Constant
• Separation of foreground and background signals in single frequency measurements of the CMB Polarization
• Flat cosmological models with massive scalar field in gauge theories of gravity
• Accelerating Universe from Extra Spatial Dimension
• New holographic Chaplygin gas model of dark energy
• Palatini $f(\mathcal{R},{\mathcal{L}}_m,{\mathcal{R}}_{\mu \nu }{T}^{\mu \nu })$ gravity and its Born-Infeld semblance
• Bulk scalar field in brane-worlds with induced gravity inspired by the $\mathcal{L}(R)$ term
• Non-Minimal Cosmological Model in Modified Yang--Mills Theory
• Fine Tuning Problem of the Cosmological Constant in a Generalized Randall-Sundrum Model
• Nature of Dark Energy and Polarization Measurements
• SuperBIT Superpressure Flight Instrument Overview and Performance: Near diffraction-limited Astronomical Imaging from the Stratosphere
• On the wavelet analysis of CMB time ordered data: application to Archeops
• A Solution to the Cosmological Constant Problem
• Predictions of Dynamically Emerging Brane Inflation Models
• Stability analysis and observational constraints in scalar tensor theory
• Problems with the Current Cosmological Paradigm
• Some characteristics of three exact solutions of Einstein equations minimally coupled to a Quintessence field
• The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps
• $f(R)$ Gravity and Crossing the Phantom Divide Barrier
• Isotropisation of flat homogeneous universes with scalar fields
• LRS Bianchi I model with perfect fluid equation of state
• Dark energy from the gas of wormholes
• A convolutional-neural-network estimator of CMB constraints on dark matter energy injection
• Can MONDian vector theories explain the cosmic speed up ?
• Observational constraints in scalar tensor theory with tachyonic potential
• OVRO CMB Anisotropy Measurement Constraints on Flat-Lambda and Open CDM Cosmogonies
• Properties of subhalos in the interacting dark matter scenario
• Power-law solutions for TeVeS
• On the origin of the large scale structures of the universe
• Systematic effects induced by a flat isotropic dielectric slab
• Cosmological constraints in Lambda-CDM and Quintessence paradigms with Archeops
• Relativity principle with a low energy invariant scale
• Testing the CMB Data for Systematic Effects
• Primordial Nucleosynthesis in the New Cosmology
• MOND and Methodology
• Cosmological expansion governed by a scalar field from a 5D vacuum
• Goodness--of--fit Statistics and CMB Data Sets
• The interplay between high energy physics and cosmology: an example
• The Virtues of Frugality - Why cosmological observers should release their data slowly
• Constraints on scalar-tensor theories from observations
• Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
• Exact Cosmological Models with the Yang - Mills Fields on Lyra Manifold
• Archeops: an instrument for present and future cosmology
• An Inflationary Scenario Taking into Account of Possible Dark Energy Effects in the Early Universe
• Natures of Statefinder Parameters and Om Diagnostic for Cardassian Universe in Horava-Lifshitz Gravity
• Reply to "On scaling solutions with a dissipative fluid"
• Structure Formation in Dynamical Dark Energy Models
• Correspondence between modified gravity and 5D Ricci-flat cosmologies
• Phase space of multi-fluid universe in $F(T)$-gravity and some enhancements for the oscillating interaction model
• Challenges to the cosmological constant model following results from the Dark Energy Survey
• Geometric and thermodynamic properties in Gauss-Bonnet gravity
• Quasilinear observables in dark energy cosmologies
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• Dynamical effects of the neutrino gravitational clustering at Planck angular scales
• Cosmic Acceleration Caused by the Extra-Dimensional Evolution in a Generalized Randall-Sundrum Model
• An update on Archeops: flights and data products
• Anisotropic evolution of D-dimensional FRW spacetime
• Status of CMB observations in 2015
• Cosmological Model of Interacting Phantom and Yang-Mills Fields
• Cosmological models with the spinor and non-minimally interacting scalar field
• Maps of the Cosmos: The Cosmic Microwave Background
• Thermodynamics of Apparent Horizon and Friedmann Equations in Big Bounce Universe