Dark Matter Annihilation in The Galactic Center As Seen by the Fermi Gamma Ray Space Telescope

Abstract

We analyze the first two years of data from the Fermi Gamma Ray Space Telescope from the direction of the inner 10 degrees around the Galactic Center with the intention of constraining, or finding evidence of, annihilating dark matter. We find that the morphology and spectrum of the emission between 1.25 degrees and 10 degrees from the Galactic Center is well described by a the processes of decaying pions produced in cosmic ray collisions with gas, and the inverse Compton scattering of cosmic ray electrons in both the disk and bulge of the Inner Galaxy, along with gamma rays from known points sources in the region. The observed spectrum and morphology of the emission within approximately 1.25 degrees (~175 parsecs) of the Galactic Center, in contrast, departs from the expectations for by these processes. Instead, we find an additional component of gamma ray emission that is highly concentrated around the Galactic Center. The observed morphology of this component is consistent with that predicted from annihilating dark matter with a cusped (and possibly adiabatically contracted) halo distribution (density proportional to r^{-gamma}, with gamma=1.18 to 1.33). The observed spectrum of this component, which peaks at energies between 1-4 GeV (in E^2 units), can be well fit by a 7-10 GeV dark matter particle annihilating primarily to tau leptons with a cross section in the range of 4.6 x 10^-27 to 5.3 x 10^-26 cm^3/s, depending on how the dark matter distribution is normalized. We also discuss other sources for this emission, including the possibility that much of it originates from the Milky Way's supermassive black hole.

23 pages, 16 figures

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• Pseudoscalar Portal Dark Matter and New Signatures of Vector-like Fermions
• Quark-flavored scalar dark matter
• Light weakly interacting massive particles
• Identification of point sources in gamma rays using U-shaped convolutional neural networks and a data challenge
• Saving the MSSM from the Galactic Center Excess
• Dark Matter Astrometry: Accuracy of sub-halo positions for the measurement of self-interaction cross sections
• Exploring A Cosmic-Ray Origin of the Multi-wavelength Emission in M31
• Galactic-Centre Gamma Rays in CMSSM Dark Matter Scenarios
• Anti-Deuterons and Anti-Helium Nuclei from Annihilating Dark Matter
• A 3.55 keV Line from Exciting Dark Matter without a Hidden Sector
• Improving the Sensitivity of Gamma-Ray Telescopes to Dark Matter Annihilation in Dwarf Spheroidal Galaxies
• Constraining decaying very heavy dark matter from galaxy clusters with 14 year Fermi-LAT data
• Study of the excess Fe XXV line emission in the central degrees of the Galactic centre using XMM-Newton data
• Gamma-Ray Excess and the Minimal Dark Matter Model
• Higgsino Dark Matter Confronts 14 years of Fermi Gamma Ray Data
• Toward the ultimate reach of current imaging atmospheric Cherenkov telescopes and their sensitivity to TeV dark matter
• Leptonic origin of the 100 MeV gamma-ray emission from the Galactic Centre
• A Latitude-Dependent Analysis of the Leptonic Hypothesis for the Fermi Bubbles
• Testing Type II Radiative Seesaw Model: from Dark Matter Detection to LHC Signatures
• Updated Collider and Direct Detection Constraints on Dark Matter Models for the Galactic Center Gamma-Ray Excess
• Cherenkov Telescope Array sensitivity to the putative millisecond pulsar population responsible for the Galactic center excess
• Searching for Dark Matter Annihilation in the Smith High-Velocity Cloud
• Known Radio Pulsars Do Not Contribute to the Galactic Center Gamma-Ray Excess
• Impact of QCD uncertainties on antiproton spectra from dark-matter annihilation
• Indirect Probes of Dark Matter and Globular Cluster Properties From Dark Matter Annihilation within the Coolest White Dwarfs
• Cosmic-ray antiprotons in the AMS-02 era: A sensitive probe of dark matter
• Molecular Clouds as the Origin of the Fermi Gamma-Ray GeV-Excess
• Dark Higgs Channel for FERMI GeV $\gamma$-ray Excess
• Cosmic-Ray Models of the Ridge-Like Excess of Gamma Rays in the Galactic Center
• An Elusive Vector Dark Matter
• Lepton-Flavor Violating Mediators
• Constraints on dark matter annihilation and decay from the large-scale structure of the nearby universe
• Multi-messenger constraints on dark matter annihilation into electron-positron pairs
• Robustness of dark matter constraints and interplay with collider searches for New Physics
• Mixed Dark Matter in Left-Right Symmetric Models
• Robust inference of the Galactic centre gamma-ray excess spatial properties
• Muon g-2 and galactic centre $\gamma$-ray excess in a scalar extension of the 2HDM type-X
• A Phantom Menace: On the Morphology of the Galactic Center Excess
• Dark matter annihilation into right-handed neutrinos and the galactic center gamma-ray excess
• Determining the Quantum Numbers of Simplified Models in $t\bar{t}X$ production at the LHC
• Dark Matter Annihilation into Four-Body Final States and Implications for the AMS Antiproton Excess
• Strongly Interacting Neutrino Portal Dark Matter
• Reconstructing WIMP properties through an interplay of signal measurements in direct detection, Fermi-LAT, and CTA searches for dark matter
• Wavelet-Based Techniques for the Gamma-Ray Sky
• A Robust Approach to Constraining Dark Matter from Gamma-Ray Data
• The Sensitivity of Future Gamma-Ray Telescopes to Primordial Black Holes
• Dark Matter, Shared Asymmetries, and Galactic Gamma Ray Signals
• The effect of stellar encounters on the dark matter annihilation signal from prompt cusps
• Antiproton signatures from astrophysical and dark matter sources at the galactic center
• Inverse Compton emission from millisecond pulsars in the Galactic bulge
• Fermi LAT observations of Sagittarius A*: Imaging Analysis
• Tau Portal Dark Matter models at the LHC
• Connecting the new H.E.S.S. diffuse emission at the Galactic center with the Fermi GeV excess: a combination of millisecond pulsars and heavy dark matter?
• Robustness of the Galactic Center Excess Morphology Against Masking
• Exploring the Nature of the Galactic Center Gamma-Ray Source with the Cherenkov Telescope Array
• Di-photon excess at LHC and the gamma ray excess at the Galactic Centre
• Illuminating the Darkest Galaxies
• Dark matter annihilation and the Galactic Centre Excess
• Search for gamma-ray line features from Milky Way satellites with Fermi-LAT Pass 8 data
• 3FGL J1924.8-1034 : A Spatially-Extended Stable Unidentified GeV Source?
• Fermionic Dark Matter through a Light Pseudoscalar Portal: Hints from the DAMA Results
• Revisiting XENON100's Constraints (and Signals?) For Low-Mass Dark Matter
• Muonphilic Dark Matter explanation of gamma-ray galactic center excess: a comprehensive analysis
• Dark matter substructure cannot explain properties of the Fermi Galactic Centre excess
• A Compound Poisson Generator approach to Point-Source Inference in Astrophysics
• The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation
• Dark matter implications of the WMAP-Planck Haze
• Dark Matter Overview: Collider, Direct and Indirect Detection Searches
• Degeneracies between baryons and dark matter: the challenge of constraining the nature of dark matter with JWST
• Constraints on dark matter annihilation from the FAST observation of the Coma Berenices dwarf galaxy
• Gamma Ray polarimetry; a new window for the non-thermal Universe
• Search for gamma-ray emission from the 12 nearby dwarf spheroidal galaxies with 12 years of Fermi-LAT data
• Comparing Galactic Center MSSM dark matter solutions to the Reticulum II gamma-ray data
• Probing the pulsar explanation of the Galactic-Center GeV excess using continuous gravitational-wave searches
• Planck-scale effects on WIMP dark matter
• On the importance of direct detection combined limits for spin independent and spin dependent dark matter interactions
• New determination of the production cross section for $\gamma$ rays in the Galaxy
• Gamma-rays From Warm WIMP Dark Matter Annihilation
• A Combined Radio Multi-Survey Catalog of Fermi Unassociated Sources
• What the Milky Way's Dwarfs tell us about the Galactic Center extended excess
• Mind the gap: The discrepancy between simulation and reality drives interpretations of the Galactic Center Excess
• Dark Matter annihilation energy output and its effects on the high-z IGM
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• Search for dark matter particles in proton-proton collisions at sqrt(s) = 8 TeV using the razor variables
• Dark Matter Detection with Hard X-ray Telescopes
• Search for gamma-ray emission from the nearby dwarf spheroidal galaxies with 9 years of Fermi-LAT data
• Gamma-Ray Constraints on the First Stars from Annihilation of Light WIMPs
• Asymmetric Dark Matter
• Thermodynamic Evolution of Secluded Vector Dark Matter: Conventional WIMPs and Nonconventional WIMPs
• Gamma-ray image reconstruction of the Andromeda galaxy
• Signatures of top flavour-changing dark matter
• Baryogenesis from spontaneous CP violation in the early Universe
• Prospects for higgsino-singlino dark matter detection at IceCube and PINGU
• Explaining Low Energy $\gamma$-ray Excess from the Galactic Centre using a Two Component Dark Matter Model
• Interpretation of the gamma-ray excess and AMS-02 antiprotons: Velocity dependent dark matter annihilations
• Probing Flavor Structure of Cosmic Ray $e^{\mp }$ Spectrum and Implications for Dark Matter Indirect Searches
• A Closer Look at CP-Violating Higgs Portal Dark Matter as a Candidate for the GCE
• The Andromeda Gamma-Ray Excess: Background Systematics of the Millisecond Pulsars and Dark Matter Interpretations
• The case for 100 GeV bino dark matter: A dedicated LHC tri-lepton search
• An update on the two singlet Dark Matter model
• The consequence of a new ISRF model of the Milky Way on predictions for diffuse gamma-ray emission
• Interpreting the galactic center gamma-ray excess in the NMSSM
• How to calculate dark matter direct detection exclusion limits that are consistent with gamma rays from annihilation in the Milky Way halo
• Neutrinos from WIMP annihilation in the Sun : Implications of a self-consistent model of the Milky Way's dark matter halo
• A New Determination of the Millisecond Pulsar Gamma-Ray Luminosity Function and Implications for the Galactic Center Gamma-Ray Excess
• Effective field theory analysis of dark matter-standard model interactions with spin one mediators
• Multi-Component Imaging of the Fermi Gamma-ray Sky in the Spatio-spectral Domain
• Interpreting the Fermi-LAT gamma ray excess in the simplified framework
• Searching for High Energy Neutrino counterpart signals; The case of the Fermi Bubbles signal and of Dark Matter annihilation in the inner Galaxy
• How to produce antinuclei from dark matter
• Searching for Gamma-Ray Emission from Reticulum II by Fermi-LAT
• A Multi-frequency analysis of possible Dark Matter Contributions to M31 Gamma-Ray Emissions
• Revisiting GeV-scale annihilating dark matter with the AMS-02 positron fraction
• The Galactic Center Excess from Z3 Scalar Semi-Annihilations
• Velocity-dependent annihilation radiation from dark matter subhalos in cosmological simulations
• Very Old Isolated Compact Objects as Dark Matter Probes
• New dark matter analysis of Milky Way dwarf satellite galaxies with MADHATv2
• On Dark Matter Explanations of the Gamma-Ray Excesses from the Galactic Center and M31
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• Everything You Always Wanted to Know About Dark Matter Elastic Scattering Through Higgs Loops But Were Afraid to Ask
• Towards resolving the Galactic center GeV excess with millisecond-pulsar-like sources using machine learning
• Enhanced lines and box-shaped features in the gamma-ray spectrum from annihilating dark matter in the NMSSM
• Towards a Bullet-proof test for indirect signals of dark matter
• Possible explanation of indirect gamma ray signatures from hidden sector fermionic dark matter
• Search for a new pseudoscalar decaying into a pair of muons in events with a top-quark pair at $\sqrt{s}=13$ TeV with the ATLAS detector
• Study of WIMP annihilations into a pair of on-shell scalar mediators
• Millisecond Pulsars in Dense Star Clusters: Evolution, Scaling Relations, and the Galactic-Center Gamma-ray Excess
• "Non-Local" Effects from Boosted Dark Matter in Indirect Detection
• Hidden Higgs Portal Vector Dark Matter for the Galactic Center Gamma-Ray Excess from the Two-Step Cascade Annihilation, and Muon g-2
• The prediction of using LHAASO's cosmic-ray electron measurements to constrain decaying heavy dark matter
• Late-forming black holes and the antiproton, gamma-ray, and anti-helium excesses
• Indirect Detection Imprint of a CP Violating Dark Sector
• Dark Matter in Leptophilic Higgs Models After the LHC Run-I
• Millisecond Pulsar Kicks Cause Difficulties in Explaining the Galactic Center Gamma-Ray Excess
• Exotic Lepton-Flavor Violating Higgs Decays
• Extracting the unresolved pulsar contribution to the gamma-ray background
• Searching for velocity-dependent dark matter annihilation signals from extragalactic halos
• Consistency test of the AMS-02 antiproton excess with direct detection data based on the effective field theory approach
• Search for Scalar Dark Matter via Pseudoscalar Portal Interactions: In Light of the Galactic Center Gamma-Ray Excess
• Collider probes of singlet fermionic dark matter scenarios for the Fermi gamma-ray excess
• Saas-Fee Lecture Notes: Multi-messenger Astronomy and Dark Matter
• A light scalar WIMP through the Higgs portal?
• Explaining the Fermi Galactic Centre Excess in the CMSSM
• Using $\gamma$-ray observations of dwarf spheroidal galaxies to test the possible common origin of the W-boson mass anomaly and the GeV $\gamma$-ray/antiproton excesses
• Testing the dark matter origin of the WMAP-Planck Haze with radio observations of Spiral Galaxies
• Low-mass neutralino dark matter in supergravity scenarios: phenomenology and naturalness
• Current status and desired accuracy of the isotopic production cross-sections relevant to astrophysics of cosmic rays II. Fluorine to Silicon (and updated LiBeB)
• Gamma rays from dark matter spikes in EAGLE simulations
• TeV gamma-ray sensitivity to velocity-dependent dark matter models in the Galactic Center
• Phenomenology of Colored Radiative Neutrino Mass Model and Its Implications on the Cosmic-ray Observations
• Gamma-ray line constraints on Coy Dark Matter
• Quantum Simulations of Dark Sector Showers
• Interpretations of galactic center gamma-ray excess confronting the PandaX-II constraints on dark matter-neutron spin-dependent scatterings in the NMSSM
• The Cherenkov Telescope Array Will Test Whether Pulsars Generate the Galactic Center Gamma-Ray Excess
• Cold Positrons from Decaying Dark Matter
• Search for pseudoscalar-mediated WIMPs in $t\to c$ transitions with missing energy
• Dwarf Galaxy $\gamma$-excess and 3.55 keV X-ray Line In A Nonthermal Dark Matter Model
• Collider limits on dark matter
• Absence of TeV halos around millisecond pulsars
• Low Mass Pseudoscalar Dark Matter in an Extended B - L Model
• Investigating the Fermi Large Area Telescope sensitivity of detecting the characteristics of the Galactic center excess
• Interpretations of the possible 42.7 GeV $\gamma$-ray line
• Can Dark Stars account for the star formation efficiency excess at very high redshifts?
• Constraints on Axion-like Particles from the gamma-ray observation of the Galactic Center
• Dark Matter Is The New BBN
• Semi-dark Higgs decays: sweeping the Higgs neutrino floor
• Searching for Dark Photon Dark Matter with Cosmic Ray Antideuterons
• Reconciling Higgs physics and pseudo-Nambu-Goldstone dark matter in the S2HDM using a genetic algorithm
• Constraining Dwarf Spheroidal Dark Matter Halos With The Galactic Center Excess
• Soft Gamma Rays from Heavy WIMPs
• Fermi-LAT searches for gamma-ray pulsars
• One of Everything: The Breakthrough Listen Exotica Catalog
• TeV Gamma Rays From Galactic Center Pulsars
• The Velocity-Dependent $J$-factor of the Milky Way Halo: Does What Happens in the Galactic Bulge Stay in the Galactic Bulge?
• Scalar Dark Matter Candidates in Two Inert Higgs Doublet Model
• Indirect detection of Dark matter with gamma-rays - status and perspectives
• Extension of Minimal Fermionic Dark Matter Model : A Study with Two Higgs Doublet Model
• Dark matter cooling during early matter-domination boosts sub-earth halos
• Connecting the LHC diphoton excess to the Galatic center gamma-ray excess
• Applying Simulation-Based Inference to Spectral and Spatial Information from the Galactic Center Gamma-Ray Excess
• A Potentially Detectable Gamma-Ray Line in the Fermi Galactic Center Excess -- In Light of One-Step Cascade Annihilations of Secluded (Vector) Dark Matter via the Higgs Portal
• Indirect Dark Matter Searches and Models
• Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
• Detectability of dark matter density distribution via gravitational waves from binary black holes in the Galactic center
• Electron-positron pair production near the Galactic Centre and the 511 keV emission line
• Optimal observing strategies for velocity-suppressed dark matter annihilation
• Leptophilic Dark Matter in Direct Detection Experiments and in the Sun
• Using dust to constrain dark matter models
• Non-relativistic matter and Dark energy in a quantum conformal model
• Deep Learning Models of the Discrete Component of the Galactic Interstellar Gamma-Ray Emission
• Einstein@Home Searches for Gamma-ray Pulsars in the Inner Galaxy
• Exploring the MeV Sky with a Combined Coded Mask and Compton Telescope: The Galactic Explorer with a Coded Aperture Mask Compton Telescope (GECCO)
• An alternative Explanation for the Fermi GeV Gamma-Ray Excess
• Fundamental Physics from the Sky: Cosmic Rays, Gamma Rays and the Hunt for Dark Matter
• Interpretation of the Galactic gamma-ray excess with the dark matter indicated by ${}^8$Be and ${}^4$He anomalous transitions
• Closing in on the Wino LSP via trilepton searches at the LHC
• Observations of the Fermi bubbles and the Galactic center excess with the DArk Matter Particle Explorer
• Dark Matter and Electroweak Baryogenesis with Spontaneous $CP$ Violation in the Early Universe
• Flares from Galactic centre pulsars: a new class of X-ray transients?
• Possible counterpart signal of the Fermi bubbles at the cosmic-ray positrons
• Impact of ATLAS constraints on effective dark matter-standard model interactions with spin-one mediators
• Characterizing the Expected Behavior of Non-Poissonian Template Fitting
• $\mathcal{O}$(1) GeV dark matter in SUSY and a very light pseudoscalar at the LHC
• Improved Modeling of the Discrete Component of the Galactic Interstellar Gamma-ray Emission and Implications for the Fermi-LAT Galactic Center Excess
• Are we really seeing dark matter signals from the Milky Way center?
• The Galactic Isotropic $\gamma$-ray Background and Implications for Dark Matter
• Investigating the dark matter minispikes with the gamma-ray signal from the halo of M31
• Blois 2019: highlights and outlook
• Extended Higgs-portal dark matter and the Fermi-LAT Galactic Center Excess
• Millisecond Pulsars in Globular Clusters and Implications for the Galactic Center Gamma-Ray Excess
• GeV excess and phenomenological astrophysics modeling
• On the Energy Distribution of the Galactic Center Excess' Sources
• Dark matter properties implied by gamma ray interstellar emission models
• The Density of Dark Matter in the Galactic Bulge and Implications for Indirect Detection
• Informational corrections to the early-Universe radiation sector: CET Omega, WIMP freeze-out, and implications for a possible 20 GeV gamma-ray excess
• Implications of the Fermi-LAT Pass 8 Galactic Center Excess on Supersymmetric Dark Matter
• A GeV-TeV particle component and the barrier of cosmic-ray sea in the Central Molecular Zone
• Spin-one dark matter and gamma ray signals from the galactic center
• Theoretical and phenomenological consequences of active and sterile neutrino within Beyond Standard Model framework
• On a possible origin of the gamma-ray excess around the Galactic Center
• Limits on Dark Matter Annihilation from the Shape of Radio Emission in M31
• On the morphology of $\gamma -$ray emission induced by $e^{\pm }$ from annihilating self-interacting dark matter
• The contribution to Galactic Centre γ-ray excess from cluster-born millisecond pulsars. Constraints from direct N-body simulations
• Extragalactic Searches for Dark Matter Annihilation
• From the Cosmological Constant: Higgs Boson, Dark Matter, and Quantum Gravity Scales
• Probing Bottom-flavored Scalar Dark Matters at Loop Level
• Exotic Decays of Heavy B quarks
• Measurement of High Energy Gamma Rays from 200 MeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station
• New energy spectra in neutrino and photon detectors to reveal hidden dark matter signals
• Analysis of shape and angular orientation parameters of velocity-dependent dark matter annihilation signals in Galactic Centers for FIRE simulations
• Searching for dark matter annihilation in the Sun with the IceCube Upgrade
• Dark Matter Phenomenology: Sterile Neutrino Portal and Gravitational Portal in Extra-Dimensions
• Assessing the Impact of Hydrogen Absorption on the Characteristics of the Galactic Center Excess
• A GeV Gamma-Ray Spectral Excess in the Fermi Blazar 4FGL J0136.5+3906
• Constraining light dark matter in vector-scalar portals with COSI and AMEGO-X
• Probing the millisecond pulsar origin of the $\gamma$-ray excess in the Galactic centre with LISA
• What Can Gamma-rays from Space tell us About the Madala Hypothesis?
• Sensitivity to keV-MeV dark matter from cosmic-ray scattering with current and the upcoming ground-based arrays CTA and SWGO
• Exploring the nature of Galactic unassociated sources detected by the Fermi-LAT