Radio detection prospects for a bulge population of millisecond pulsars as suggested by Fermi LAT observations of the inner Galaxy
arXiv:1512.06825 · doi:10.3847/0004-637X/827/2/143
Abstract
Analogously to globular clusters, the dense stellar environment of the Galactic center has been proposed to host a large population of as-yet undetected millisecond pulsars (MSPs). Recently, this hypothesis found support in the analysis of gamma rays from the inner Galaxy seen by the Large Area Telescope (LAT) aboard the Fermi satellite, which revealed a possible excess of diffuse GeV photons in the inner 15 deg about the Galactic center (Fermi GeV excess). The excess can be interpreted as the collective emission of thousands of MSPs in the Galactic bulge, with a spherical distribution that strongly peaks towards the Galactic center. In order to fully establish the MSP interpretation, it is essential to find corroborating evidence in multi-wavelength searches, most notably through the detection of radio pulsation from individual bulge MSPs. Based on globular cluster observations and the gamma-ray emission from the inner Galaxy, we investigate the prospects for detecting MSPs in the Galactic bulge. While previous pulsar surveys failed to identify this population, we demonstrate that, in the upcoming years, new large-area surveys with focus on regions a few degrees north or south of the Galactic center should lead to the detection of dozens of bulge MSPs. Additionally, we show that, in the near future, deep targeted searches of unassociated Fermi sources should be able to detect the first few MSPs in the bulge. The prospects for these deep searches are enhanced by a tentative gamma-ray/radio correlation that we infer from high-latitude gamma-ray MSPs. Such detections would constitute the first clear discoveries of field MSPs in the Galactic bulge, with far-reaching implications for gamma-ray observations, the formation history of the central Milky Way and strategy optimization for future radio observations.
arXiv comment24 pages, 17 figures, 5 tables. Minor clarifications. Matches version published in ApJ
References in corpus (66)
- The ATNF Pulsar Catalogue
- Asymptotic formulae for likelihood-based tests of new physics
- Monitoring stellar orbits around the Massive Black Hole in the Galactic Center
- The Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
- Dark Matter Annihilation in The Galactic Center As Seen by the Fermi Gamma Ray Space Telescope
- Birth and Evolution of Isolated Radio Pulsars
- On The Origin Of The Gamma Rays From The Galactic Center
- Detection of a Gamma-Ray Source in the Galactic Center Consistent with Extended Emission from Dark Matter Annihilation and Concentrated Astrophysical Emission
- Background model systematics for the Fermi GeV excess
- Dark Matter and Pulsar Model Constraints from Galactic Center Fermi-LAT Gamma Ray Observations
- Fermi-LAT Observations of High-Energy Gamma-Ray Emission Toward the Galactic Center
- Very high energy gamma rays from the direction of Sagittarius A*
- Astrophysical and Dark Matter Interpretations of Extended Gamma-Ray Emission from the Galactic Center
- The High Time Resolution Universe Pulsar Survey I: System configuration and initial discoveries
- Multifrequency Observations of Radio Pulse Broadening and Constraints on Interstellar Electron Density Microstructure
- Strong support for the millisecond pulsar origin of the Galactic center GeV excess
- The characteristics of millisecond pulsar emission: I. Spectra, pulse shapes and the beaming fraction
- Evidence for Unresolved Gamma-Ray Point Sources in the Inner Galaxy
- Observations of 20 millisecond pulsars in 47 Tucanae at 20 cm
- Pulsar spectra of radio emission
- The Consistency of Fermi-LAT Observations of the Galactic Center with a Millisecond Pulsar Population in the Central Stellar Cluster
- The pulsar spectral index distribution
- Co-Evolution of Galactic Nuclei and Globular Cluster Systems
- The Green Bank Northern Celestial Cap Pulsar Survey - I: Survey Description, Data Analysis, and Initial Results
- A Deep Chandra Catalog of X-ray Point Sources toward the Galactic Center
- GeV excess in the Milky Way: The Role of Diffuse Galactic gamma ray Emission template
- Cosmic Ray Protons in the Inner Galaxy and the Galactic Center Gamma-Ray Excess
- A population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope
- Disrupted Globular Clusters Can Explain the Galactic Center Gamma Ray Excess
- Chandra X-Ray Observations of Nineteen Millisecond Pulsars in the Globular Cluster 47 Tucanae
- Galactic Center gamma-ray "excess" from an active past of the Galactic Centre?
- Millisecond pulsars and the Galactic Center gamma-ray excess: the importance of luminosity function and secondary emission
- Gamma-ray sky points to radial gradients in cosmic-ray transport
- Gamma-Ray Emission in Dissipative Pulsar Magnetospheres: From Theory to Fermi Observations
- The Contribution of Cosmic Rays Interacting With Molecular Clouds to the Galactic Center Gamma-Ray Excess
- The Galactic Center GeV Excess from a Series of Leptonic Cosmic-Ray Outbursts
- Discovery of Three Pulsars from a Galactic Center Pulsar Population
- A 1.4-GHz Arecibo Survey for Pulsars in Globular Clusters
- The Globular Cluster Migratory Origin of Nuclear Star Clusters
- Millisecond pulsar interpretation of the Galactic center gamma-ray excess
- Parkes radio searches of Fermi gamma-ray sources and millisecond pulsar discoveries
- The Pulsar Contribution to the Gamma-Ray Background
- Discovery of two pulsars towards the Galactic Centre
- The High Time Resolution Universe Pulsar Survey VIII: The Galactic millisecond pulsar population
- Diffuse gamma-ray emission from galactic pulsars
- The High Time Resolution Universe Pulsar Survey X: Discovery of four millisecond pulsars and updated timing solutions of a further 12
- Optical spectroscopic observations of blazars and gamma-ray blazar candidates in the Sloan Digital Sky Survey Data Release Nine
- Pulsar searches of Fermi unassociated sources with the Effelsberg telescope
- Unveiling the nature of the unidentified gamma-ray sources II: radio, infrared and optical counterparts of the gamma-ray blazar candidates
- Luminosities of recycled radio pulsars in globular clusters
- Gamma-ray pulsars: a gold mine
- New Associations of Gamma-Ray Sources from the Fermi Second Source Catalog
- Pulsar Wind Nebulae and the X-Ray Emission of Non-Accreting Neutron Stars
- On Detecting Millisecond Pulsars at the Galactic Center
- Source population synthesis and the Galactic diffuse gamma-ray emission
- Radio Detection of the Fermi LAT Blind Search Millisecond Pulsar J1311-3430
- Swift observations of SAX J1808.4-3658: monitoring the return to quiescence
- Testing the millisecond pulsar scenario of the Galactic center gamma-ray excess with very high energy gamma-rays
- Refining the associations of the Fermi Large Area Telescope Source Catalogs
- The Parkes multibeam pulsar survey: VII. Timing of four millisecond pulsars and the underlying spin period distribution of the Galactic millisecond pulsar population
- Gamma-rays from millisecond pulsar population within the central stellar cluster in the Galactic Center
- A stacked analysis of 115 pulsars observed by the Fermi LAT
- The identification of the optical companion to the binary millisecond pulsar J0610-2100 in the Galactic field
- Searching for Millisecond Pulsars: Surveys, Techniques and Prospects
- The Magnetic Fields of Millisecond Pulsars in Globular Clusters
- Gamma-ray emission from globular clusters 2MS-GC01, IC 1257, NGC5904, NGC6656 and FSR1735
Cited by in corpus (58)
- Fundamental Physics with the Square Kilometre Array
- Science with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics)
- The origin of Galactic cosmic rays: challenges to the standard paradigm
- Searching for Primordial Black Holes in the radio and X-ray sky
- The Fermi-LAT GeV Excess Traces Stellar Mass in the Galactic Bulge
- Dark Matter Strikes Back at the Galactic Center
- Recognising Axionic Dark Matter by Compton and de-Broglie Scale Modulation of Pulsar Timing
- Strong constraints on thermal relic dark matter from Fermi-LAT observations of the Galactic Center
- The Return of the Templates: Revisiting the Galactic Center Excess with Multi-Messenger Observations
- Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO--Virgo data
- Modelling Neutron Star-Black Hole Binaries: Future Pulsar Surveys and Gravitational Wave Detectors
- Birth, life, and death of black hole binaries around supermassive black holes: dynamical evolution of gravitational wave sources
- A New Mask for An Old Suspect: Testing the Sensitivity of the Galactic Center Excess to the Point Source Mask
- Transient Radio Signatures from Neutron Star Encounters with QCD Axion Miniclusters
- Status and perspectives of Continuous Gravitational Wave searches
- Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar
- Characterizing the Nature of the Unresolved Point Sources in the Galactic Center
- Model-independent analysis of the DAMPE excess
- Consistency Between the Luminosity Function of Resolved Millisecond Pulsars and the Galactic Center Excess
- Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures
- Bayesian Model Comparison and Analysis of the Galactic Disk Population of Gamma-Ray Millisecond Pulsars
- Galactic Binaries Can Explain the Fermi Galactic Center Excess and 511 keV Emission
- Disrupted Globular Clusters and the Gamma-Ray Excess in the Galactic Centre
- Les Houches Lectures on Indirect Detection of Dark Matter
- Dissecting the inner Galaxy with -ray pixel count statistics
- Gamma-ray and X-ray emission from the Galactic Centre: hints on the nuclear star cluster formation history
- Evidence of TeV Halos Around Millisecond Pulsars
- Investigating the Uniformity of the Excess Gamma rays towards the Galactic Center Region
- Dim but not entirely dark: Extracting the Galactic Center Excess' source-count distribution with neural nets
- Probing the formation history of the nuclear star cluster at the Galactic Centre with millisecond pulsars
- Point Sources from Dissipative Dark Matter
- Hunting for Dark Matter and New Physics with GECCO
- Searching For Pulsars Associated With the Fermi GeV Excess
- The Galactic bulge millisecond pulsars shining in X rays: A gamma-ray perspective
- Cherenkov Telescope Array sensitivity to the putative millisecond pulsar population responsible for the Galactic center excess
- Robust inference of the Galactic centre gamma-ray excess spatial properties
- Multi-wavelength detectability of isolated black holes in the Milky Way
- Probing the Fermi-LAT GeV excess with gravitational waves
- Detection of a dense group of hyper-compact radio sources in the central parsec of the Galaxy
- Probing the pulsar explanation of the Galactic-Center GeV excess using continuous gravitational-wave searches
- Two Extreme Steep-Spectrum, Polarized Radio Sources Towards the Galactic Bulge
- Revisiting Primordial Black Hole Capture by Neutron Stars
- A Multi-frequency analysis of possible Dark Matter Contributions to M31 Gamma-Ray Emissions
- Towards resolving the Galactic center GeV excess with millisecond-pulsar-like sources using machine learning
- Relativistic scattering of a fast spinning neutron star by a massive black hole
- TeV gamma-ray sensitivity to velocity-dependent dark matter models in the Galactic Center
- The Cherenkov Telescope Array Will Test Whether Pulsars Generate the Galactic Center Gamma-Ray Excess
- The effect of kick velocities on the spatial distribution of millisecond pulsars and implications for the Galactic center excess
- Reconciling Higgs physics and pseudo-Nambu-Goldstone dark matter in the S2HDM using a genetic algorithm
- Einstein@Home Searches for Gamma-ray Pulsars in the Inner Galaxy
- Signatures of Dark Matter in Cosmic-Ray Observations
- Physics of radio emission in gamma-ray pulsars
- Characterizing the Expected Behavior of Non-Poissonian Template Fitting
- Multiwavelength identification of millisecond pulsar candidates in the Galactic bulge
- On the Energy Distribution of the Galactic Center Excess' Sources
- Pulsar Timing Response to Gravitational Waves with Spherical Wavefronts from a Massive Compact Source in the Quadrupole Approximation
- Dark matter properties implied by gamma ray interstellar emission models
- High Energy Emission from the Galactic Center