Effective field theory and keV lines from dark matter
arXiv:1403.1240 · doi:10.1088/1475-7516/2014/09/007
Abstract
We survey operators that can lead to a keV photon line from dark matter decay or annihilation. We are motivated in part by recent claims of an unexplained 3.5 keV line in galaxy clusters and in Andromeda, but our results could apply to any hypothetical line observed in this energy range. We find that given the amount of flux that is observable, explanations in terms of decay are more plausible than annihilation, at least if the annihilation is directly to Standard Model states rather than intermediate particles. The decay case can be explained by a scalar or pseudoscalar field coupling to photons suppressed by a scale not far below the reduced Planck mass, which can be taken as a tantalizing hint of high-scale physics. The scalar case is particularly interesting from the effective field theory viewpoint, and we discuss it at some length. Because of a quartically divergent mass correction, naturalness strongly suggests the theory should be cut off at or below the 1000 TeV scale. The most plausible such natural UV completion would involve supersymmetry. These bottom-up arguments reproduce expectations from top-down considerations of the physics of moduli. A keV line could also arise from the decay of a sterile neutrino, in which case a renormalizable UV completion exists and no direct inference about high-scale physics is possible.
arXiv commentv2: Minor correction, references and comments on LARGE volume string compactifications added
References in corpus (36)
- de Sitter Vacua in String Theory
- Axions In String Theory
- On the Geometry of the String Landscape and the Swampland
- Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications
- Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56
- Detection of An Unidentified Emission Line in the Stacked X-ray spectrum of Galaxy Clusters
- Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-5
- Cosmological Simulations with Self-Interacting Dark Matter I: Constant Density Cores and Substructure
- The role of sterile neutrinos in cosmology and astrophysics
- Model Independent Properties and Cosmological Implications of the Dilaton and Moduli Sectors of 4-d Strings
- Cosmological Implications of Dynamical Supersymmetry Breaking
- Large-Volume Flux Compactifications: Moduli Spectrum and D3/D7 Soft Supersymmetry Breaking
- Thermal Inflation and the Moduli Problem
- Sterile neutrinos: the dark side of the light fermions
- Constraining Light Dark Matter with Diffuse X-Ray and Gamma-Ray Observations
- Gravitino Dark Matter without R-parity
- A Test of the Collisional Dark Matter Hypothesis from Cluster Lensing
- Cosmology of Supersymmetric Models with Low-energy Gauge Mediation
- Solving the Cosmological Moduli Problem with Weak Scale Inflation
- Chandra Evidence for a Flattened, Triaxial Dark Matter Halo in the Elliptical Galaxy NGC 720
- Astrophysical and Cosmological Implications of Large Volume String Compactifications
- A 3.55 keV hint for decaying axion-like particle dark matter
- How Dark Are Majorana WIMPs? Signals from MiDM and Rayleigh Dark Matter
- The 7 keV axion dark matter and the X-ray line signal
- A 3.55 keV Photon Line and its Morphology from a 3.55 keV ALP Line
- Long-Lived Neutralino NLSPs
- UV Completions of Magnetic Inelastic Dark Matter and RayDM for the Fermi Line(s)
- 7 keV sterile neutrino dark matter from split flavor mechanism
- Constraint on Cosmic Density of the String Moduli Field in Gauge-Mediated Supersymmetry-Breaking Theories
- Moduli dark matter and the search for its decay line using Suzaku X-ray telescope
- One-loop Kahler potential in non-renormalizable theories
- Cosmological Constraint on the String Dilaton in Gauge-mediated Supersymmetry Breaking Theories
- Study of the Gauge Mediation Signal with Non-pointing Photons at the CERN LHC
- Mitigating Moduli Messes in Low-Scale SUSY Breaking
- Effective Theory of Dark Matter Decay into Monochromatic Photons and its Implications: Constraints from Associated Cosmic-Ray Emission
- Longevity Problem of Sterile Neutrino Dark Matter
Cited by in corpus (20)
- Checking the dark matter origin of 3.53 keV line with the Milky Way center
- Discovery of a 3.5 keV line in the Galactic Center and a Critical Look at the Origin of the Line Across Astronomical Targets
- Two component WIMP-FImP dark matter model with singlet fermion, scalar and pseudo scalar
- Nonthermal Two Component Dark Matter Model for Fermi-LAT -ray excess and 3.55 keV X-ray Line
- 3.5 keV X-ray Line Signal from Decay of Right-Handed Neutrino due to Transition Magnetic Moment
- Shining Light on Polarizable Dark Particles
- Return of the X-rays: A New Hope for Fermionic Dark Matter at the keV Scale
- Nonabelian dark matter models for 3.5 keV X-rays
- A Couplet from Flavored Dark Matter
- 3.55 keV line in Minimal Decaying Dark Matter scenarios
- Displaced Vertices from X-ray Lines
- 3.5 keV X-ray line and R-Parity Conserving Supersymmetry
- Common Origin of 3.55 keV X-Ray Line and Galactic Center Gamma Ray Excess in a Radiative Neutrino Mass Model
- Structure formation in a mixed dark matter model with decaying sterile neutrino: the 3.5 keV X-ray line and the Galactic substructure
- Common Origin of keV X-ray line and Gauge Coupling Unification with Left-Right Dark Matter
- SUSY's Ladder: Reframing Sequestering at Large Volume
- Anomalous X-Ray Galactic signal from 7 keV spin- dark matter decay
- A sensitive search for unknown spectral emission lines in the diffuse X-ray background with XMM-Newton
- 3.5 keV X-ray Line Signal from Dark Matter Decay in Local Extension of Zee-Babu Model
- Supersymmetric Higgs-portal and X-ray lines