CMB spectral distortions are tiny departures of the average
cosmic microwave background (CMB) frequency spectrum
The power spectrum S_(f) of a time series x(t) describes the distribution of power into frequency components composing that signal. According to Fourier analysis, any physical signal can be decomposed into a number of discrete frequencies, ...
from the predictions given by a perfect
black body
A black body or blackbody is an idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence. The name "black body" is given because it absorbs all colors of light. A black body ...
. They can be produced by a number of standard and non-standard processes occurring at the early stages of
cosmic history, and therefore allow us to probe the standard picture of cosmology. Importantly, the CMB frequency spectrum and its distortions should not be confused with the CMB anisotropy power spectrum, which relates to spatial fluctuations of the CMB temperature in different directions of the sky.
Overview
The energy spectrum of the CMB is extremely close to that of a perfect blackbody with a temperature of
. This is expected because in the early Universe matter and radiation are in
thermal equilibrium
Two physical systems are in thermal equilibrium if there is no net flow of thermal energy between them when they are connected by a path permeable to heat. Thermal equilibrium obeys the zeroth law of thermodynamics. A system is said to be in ...
. However, at
redshift
In physics, a redshift is an increase in the wavelength, and corresponding decrease in the frequency and photon energy, of electromagnetic radiation (such as light). The opposite change, a decrease in wavelength and simultaneous increase in f ...
s
, several mechanisms, both standard and non-standard, can modify the CMB spectrum and introduce departures from a blackbody spectrum. These departures are commonly referred to as CMB spectral distortions and mostly concern the average CMB spectrum across the full sky (i.e., the CMB monopole spectrum).
Spectral distortions are created by processes that drive matter and radiation out of equilibrium. One important scenario relates to spectral distortions from early energy injection, for instance, by decaying particles, primordial black hole evaporation or the dissipation of acoustic waves set up by inflation. In this process, the baryons heat up and transfer some of their excess energy to the ambient CMB photon bath via
Compton scattering
Compton scattering, discovered by Arthur Holly Compton, is the scattering of a high frequency photon after an interaction with a charged particle, usually an electron. If it results in a decrease in energy (increase in wavelength) of the photon ...
. Depending on the moment of injection, this causes a distortion, which can be characterized using so-called
- and
-type distortion spectra. The dimensionless
and
-parameters are a measure for the total amount of energy that was injected into the CMB. CMB spectral distortions therefore provide a powerful probe of early-universe physics and even deliver crude estimates for the epoch at which the injection occurred.
The current best observational limits set in the 1990s by
COBE-satellite/FIRAS-instrument (COBE/FIRAS) are
and
at 95% confidence level. Within
CDM we expect
and
, signals that have come into reach of current-day technology (see ). Richer distortion signals, going beyond the classical
and
distortions, can be created by photon injection processes, relativistic electron distributions and during the gradual transition between the
and
-distortion eras. The cosmological recombination radiation (CRR) is a prime example within
CDM that is created by photon injection from the recombining hydrogen and helium
plasma
Plasma or plasm may refer to:
Science
* Plasma (physics), one of the four fundamental states of matter
* Plasma (mineral), a green translucent silica mineral
* Quark–gluon plasma, a state of matter in quantum chromodynamics
Biology
* Blood pla ...
around redshifts of
.
History
The first considerations of spectral distortions to the CMB go back to the early days of CMB cosmology starting with the seminal papers of
Yakov B. Zeldovich and
Rashid Sunyaev
Rashid Alievich Sunyaev ( tt-Cyrl, Рәшит Гали улы Сөнәев, russian: Раши́д Али́евич Сюня́ев; born 1 March 1943 in Tashkent, USSR) is a Germany, German, Soviet Union, Soviet, and Russia, Russian astrophysicist ...
in 1969 and 1970. These works appeared just a few years after the first detection of the CMB by
Arno Allan Penzias
Arno Allan Penzias (; born April 26, 1933) is an American physicist, radio astronomer and Nobel laureate in physics. Along with Robert Woodrow Wilson, he discovered the cosmic microwave background radiation, which helped establish the Big Bang t ...
and
Robert Woodrow Wilson
Robert Woodrow Wilson (born January 10, 1936) is an American astronomer who, along with Arno Allan Penzias, discovered cosmic microwave background radiation (CMB) in 1964. The pair won the 1978 Nobel Prize in Physics for their discovery.
While ...
and its interpretation as the echo of the
Big Bang
The Big Bang event is a physical theory that describes how the universe expanded from an initial state of high density and temperature. Various cosmological models of the Big Bang explain the evolution of the observable universe from the ...
by
Robert H. Dicke
Robert Henry Dicke (; May 6, 1916 – March 4, 1997) was an American astronomer and physicist who made important contributions to the fields of astrophysics, atomic physics, physical cosmology, cosmology and gravity. He was the Albert Einstein ...
and his team in 1965. These findings constitute one of the most important pillars of Big Bang cosmology, which predicts the blackbody nature of the CMB. However, as shown by Zeldovich and Sunyaev, energy exchange with moving electrons can cause spectral distortions.
The pioneering analytical studies of Zeldovich and Sunyaev were later complemented by the numerical investigations of Illarionov and Sunyaev in the 1970’s. These treated the thermalization problem including Compton scattering and the
Bremsstrahlung
''Bremsstrahlung'' (), from "to brake" and "radiation"; i.e., "braking radiation" or "deceleration radiation", is electromagnetic radiation produced by the deceleration of a charged particle when deflected by another charged particle, typicall ...
process for a single release of energy. In 1982, the importance of
double Compton emission as a source of photons at high redshifts was recognized by Danese and de Zotti. Modern considerations of CMB spectral distortions started with the works of Burigana, Danese and de Zotti and Hu, Silk and Scott in the early 1990’s.
After COBE/FIRAS provided stringent limits on the CMB spectrum, essentially ruling out distortions at the level
, the interest in CMB spectral distortions decreased. In 2011, PIXIE
[ ] was proposed to
NASA
The National Aeronautics and Space Administration (NASA ) is an independent agency of the US federal government responsible for the civil space program, aeronautics research, and space research.
NASA was established in 1958, succeeding t ...
as a mid-Ex satellite mission, providing first strong motivation to revisit the theory of spectral distortions. Although no successor of COBE/FIRAS has been funded so far, this led to a renaissance of CMB spectral distortions with numerous theoretical studies and the design of novel experimental concepts
Thermalisation physics
In the cosmological 'thermalization problem', three main eras are distinguished: the thermalization or temperature-era, the
-era and the
-era, each with slightly different physical conditions due to the change in the density and temperature of particles caused by the Hubble expansion.
Thermalization era
In the very early stages of cosmic history (up until a few months after the
Big Bang
The Big Bang event is a physical theory that describes how the universe expanded from an initial state of high density and temperature. Various cosmological models of the Big Bang explain the evolution of the observable universe from the ...
), photons and baryons are efficiently coupled by scattering processes and, therefore, are in full thermodynamic equilibrium. Energy that is injected into the medium is rapidly redistributed among the photons, mainly by Compton scattering, while the photon number density is adjusted by photon non-conserving processes, such as double Compton and thermal Bremsstrahlung. This allows the photon field to quickly relax back to a
Planckian distribution
In physics, Planck's law describes the spectral density of electromagnetic radiation emitted by a black body in thermal equilibrium at a given temperature , when there is no net flow of matter or energy between the body and its environment.
At ...
, even if for a very short phase a spectral distortion appears. Observations today cannot tell the difference in this case, as there is no independent cosmological prediction for the CMB monopole temperature. This regime is frequently referred to as the thermalization or temperature era and ends at redshift
.
-distortion era
At redshifts between
and
, efficient energy exchange through Compton scattering continues to establish kinetic equilibrium between matter and radiation, but photon number changing processes stop being efficient. Since the photon number density is conserved but the energy density is modified, photons gain an effective non-zero chemical potential, acquiring a
Bose-Einstein distribution. This distinct type of distortion is called
-distortion after the chemical potential known from standard thermodynamics. The value for the chemical potential can be estimated by combining the photon energy density and number density constraints from before and after the energy injection. This yields the well-known expression,
where
determines the total energy that is injected into the CMB photon field. With respect to the equilibrium blackbody spectrum, the
-distortion is characterized by a deficit of photons at low frequencies and an increment at high frequencies. The distortion changes sign at a frequency of
, allowing us to distinguish it observationally from the
-type distortion.
-distortion signals can be created by decaying particles, evaporating primordial black holes, primordial magnetic fields and other non-standard physics examples. Within
CDM cosmology, the adiabatic cooling of matter and dissipation of acoustic waves set up by inflation cause a
-distortion with
. This signal can be used as a powerful test for inflation, as it is sensitive to the amplitude of density fluctuations at scales corresponding to physical scales of
(i.e., dwarf galaxies). By combining COBE’s measurements of the large-scale CMB anisotropies with the
-distortion constraint, the first limits on the small-scale power spectrum could be obtained well-before direct measurements became possible
-distortion era
At redshifts
, also Compton scattering becomes inefficient. The plasma has a temperature of
, such that CMB photons are boosted via non-relativistic Compton scattering, giving rise to a
-distortion. Again, by considering the total energetics of the problem and using photon number conservation, one can obtain the estimate
[ ]
The name for the
-distortion simply stems from the choice of dimensionless variables in the seminal paper of Zeldovich and Sunyaev, 1969.
There, the energy injection caused by the hot electrons residing inside clusters of galaxies was considered and the associated effect is more commonly referred to as the thermal
Sunyaev-Zeldovich (SZ) effect.
Like for the
-distortion, in principle many non-standard physics examples can cause
-type distortions. However, the largest contribution to the all-sky
-distortion stems from the cumulative cluster SZ signal, which provides a way to constrain the amount of hot gas in the Universe. While at
, the cosmic plasma on average has a low temperature, electrons inside galaxy clusters can reach temperatures of a few keV. In this case, the scattering electrons can have speeds of
, such that relativistic corrections to the Compton process become relevant. These relativistic corrections carry information of electron temperatures which can be used as a measure for the cluster energetics.
Beyond and distortions
The classical studies mainly considered
energy release (i.e., heating) as a source of distortions. However, recent work has shown that richer signals can be created by direct photon injection and non-thermal electron populations, both processes that appear in connection with decaying or annihilating particles. Similarly, it was demonstrated that the transition between the
and
-eras is more gradual and that the distortion shape is not simply given by a sum of
- and
. All these effects could allow us to differentiate observationally between a wide range of scenarios, as additional time-dependent information can be extracted.
Cosmological recombination radiation (CRR)
About 280,000 years after the Big Bang, electrons and protons became bound into electrically neutral atoms as the Universe expanded. In cosmology, this is known as recombination and preludes the
decoupling of the CMB photons from matter before they free stream throughout the Universe around 380,000 years after the Big Bang. Within the energy levels of hydrogen and helium atoms, various interactions take place, both collisional and radiative. The line emission arising from these processes is injected into the CMB, showing as small distortions to the CMB blackbody commonly referred to as the cosmological recombination radiation (CRR). The specific spectral shape of this distortion is directly related to the redshift at which this emission takes place, freezing the distortion in time over the microwave frequency bands. Since the distortion signal arises from the hydrogen and two helium recombination eras, this gives us a unique probe of the pre-recombination Universe that allows us to peek behind the last scattering surface that we observe using the CMB anisotropies.
[ ] It gives us a unique way to constrain the primordial amount of helium in the early Universe, before recombination, and measure the early expansion rate.
Experimental and observational challenges
The expected
Lambda-CDM
The ΛCDM (Lambda cold dark matter) or Lambda-CDM model is a parameterization of the Big Bang cosmological model in which the universe contains three major components: first, a cosmological constant denoted by Lambda (Greek Λ) associated with ...
(LCDM) distortion signals are small -- The largest distortion, arising from the cumulative flux of all hot gas in the Universe, has an amplitude that is about one order of magnitude below the limits of COBE/FIRAS. While this is considered to be an ‘easy’ target, the cosmological recombination radiation (CRR), as the smallest expected signal, has an amplitude that is another factor of
smaller. All LCDM distortions are furthermore obscured by large Galactic and extragalactic foreground emissions (e.g., dust, synchrotron and free-free emission, cosmic infrared background), and for observations from the ground or balloons, atmospheric emission poses another hurdle to overcome.
A detection of the LCDM distortions therefore requires novel experimental approaches that provide unprecedented sensitivity, spectral coverage, control of systematics and the capabilities to accurately remove foregrounds. Building on the design of FIRAS and experience with
ARCADE
Arcade most often refers to:
* Arcade game, a coin-operated game machine
** Arcade cabinet, housing which holds an arcade game's hardware
** Arcade system board, a standardized printed circuit board
* Amusement arcade, a place with arcade games
* ...
, this has led to several spectrometer concepts to observe from space (PIXIE, PRISM, PRISTINE, SuperPIXIE and Voyage2050),
balloon (BISOU) and the ground (APSERa and Cosmo at Dome-C, TMS at
Teide Observatory
Teide Observatory ( es, Observatorio del Teide), IAU code 954, is an astronomical observatory on Mount Teide at , located on Tenerife, Spain. It has been operated by the Instituto de Astrofísica de Canarias since its inauguration in 1964. It becam ...
). These are all designed to reach important milestones towards a detection of CMB distortions. As an ultimate frontier, a full characterization and exploitation of the cosmological recombination signal could be achieved by using a coordinated international experimental campaign, potentially including an observatory on the moon
In June 2021, the
European Space Agency
, owners =
, headquarters = Paris, Île-de-France, France
, coordinates =
, spaceport = Guiana Space Centre
, seal = File:ESA emblem seal.png
, seal_size = 130px
, image = Views in the Main Control Room (1205 ...
unveiled its plans for the future L-class missions as part of ''Voyage 2050'' with a chance for ''`high precision spectroscopy`'' for the new ''early universe'' part of their strategy, opening the door for spectral distortions telescopes for the future.
See also
References
{{Portal bar, Physics, Astronomy, Stars, Spaceflight, Outer space, Solar System, Science
Cosmic background radiation