Diffuse extragalactic background radiation

Schematic representation of the spectral energy distribution of the DEBRA. The dependent quantity is the spectral radiance multiplied by wavelength, i.e. λL_eλ.

The diffuse extragalactic background radiation (DEBRA) refers to the diffuse photon field from extragalactic origin that fill our Universe. It contains photons over ∼ 20 decades of energy from ~10⁻⁷ eV to ~100 GeV. The origin and the physical processes involved are different within every wavelength range. There are plenty of observational evidences that support the existence of the DEBRA. The figure shows a schematic picture, based on many different data sets, of the spectral intensity (also called spectral radiance) multiplied by wavelength of the DEBRA over all the electromagnetic spectrum. This representation is convenient because the area inside the curve is the energy. The nature and history of the universe is coded in this radiation field and any realistic cosmological model must be able to describe it. Understanding the DEBRA is a major challenge of modern cosmology with huge consequences in other fields of astrophysics, therefore extraordinary efforts are being put by theoreticians, observers, and instrumentalists to do so.

Regions of the DEBRA

The overall diffuse extragalactic radiation field may be divided in different regions according to their origin and physical processes involved. This is a standard classification from the highest down to the lowest energies:

• Diffuse extragalactic gamma-ray radiation (also known as cosmic gamma-ray background)
• Cosmic X-ray background
• Extragalactic background light (which includes the cosmic infrared background)
• Cosmic microwave background
• Cosmic radio background

External links

• Caltech papers