The Galactic Center is one of the most dense stellar environments in the Galaxy and is considered to be a plausible place to harbor many neutron stars. In this brief review, we summarize observational efforts in search of neutron stars within a few degrees about the Galactic Center. Up to 10% of Galactic neutron stars may reside in this central region and it is possible that more than a thousand neutron stars are located within only ∼ 25'' about the Galactic Center. Based on observations, we discuss prospects of detecting neutron stars in the Galactic Center via gravitational waves as well as electromagnetic waves.

Abstract
1. INTRODUCTION
2. DIFFERENT OBSERVATIONS AND NS CANDIDATESIN THE GCR
    2.1. Central Molecular Zone
    2.2. Supernova Remnants
    2.3. Radio Pulsars
    2.4. LMXBs
    2.5. PWNe
    2.6. Gamma-Ray Sources
3. DISCUSSION
REFERENCES

• Chunglee Kim(Department of Physics, Ewha Womans University) Corresponding author
• Melvyn B. Davies(Lund Observatory, Department of Astronomy and Theoretical Physics)