All-Sky Search for Individual Primordial Black Hole Bursts with LHAASO

Primordial black holes (PBHs) are hypothetical black holes with a wide range of masses that formed in the early Universe. As a result, they may play an important cosmological role and provide a unique probe of the early Universe. A PBH with an initial mass of approximately 10^{15} g is expected to explode today in a final burst of Hawking radiation. In this Letter, we conduct an all-sky search for individual PBH burst events using the data collected from March 2021 to July 2024 by the Water Cherenkov Detector Array of the Large High Altitude Air Shower Observatory (LHAASO). Three PBH burst durations, 10, 20, and 100 s, are searched in the gamma-ray energy range from about 1 to 15 TeV, with no significant PBH bursts observed. The upper limit on the local PBH burst rate density is set to be as low as 181 pc^{-3} yr^{-1} at 99% confidence level, representing the most stringent limit achieved to date.

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Journal
Physical Review Letters
Published
2025-10-15
DOI
https://doi.org/10.1103/nkby-9cs3
Citations
1
Primary Topic
Pulsars and Gravitational Waves Research
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article
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All-Sky Search for Individual Primordial Black Hole Bursts with LHAASO

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1 citations
Physical Review Letters
Pulsars and Gravitational Waves Research
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All-Sky Search for Individual Primordial Black Hole Bursts with LHAASO

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article en
1 citations

Abstract

Primordial black holes (PBHs) are hypothetical black holes with a wide range of masses that formed in the early Universe. As a result, they may play an important cosmological role and provide a unique probe of the early Universe. A PBH with an initial mass of approximately 10^{15} g is expected to explode today in a final burst of Hawking radiation. In this Letter, we conduct an all-sky search for individual PBH burst events using the data collected from March 2021 to July 2024 by the Water Cherenkov Detector Array of the Large High Altitude Air Shower Observatory (LHAASO). Three PBH burst durations, 10, 20, and 100 s, are searched in the gamma-ray energy range from about 1 to 15 TeV, with no significant PBH bursts observed. The upper limit on the local PBH burst rate density is set to be as low as 181 pc^{-3} yr^{-1} at 99% confidence level, representing the most stringent limit achieved to date.

Physical Review LettersVol. 135(18)
University of Science and Technology of China (CN), Tibet University (CN), Nanchang University (CN), Guangxi University (CN), Nanjing Normal University (CN), Moscow Institute of Physics and Technology (RU), Shandong University (CN), Sun Yat-sen University (CN), Hangzhou Normal University (CN), Chinese University of Hong Kong (HK), Shanghai Jiao Tong University (CN), Yunnan University (CN), Yerevan State University (AM), Chinese Academy of Sciences (CN), Peking University (CN), Université Paris Cité (FR), Sichuan University (CN), Mahidol University (TH), Shanghai Astronomical Observatory (CN), Yunnan Observatories (CN), Laboratoire AstroParticule et Cosmologie (FR), Purple Mountain Observatory (CN), Guangdong Polytechnic of Science and Technology (CN), Guangzhou University (CN), Zhengzhou University (CN), Institute for Nuclear Research (RU), Kavli Institute for Theoretical Sciences (CN), Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou) (CN), National Space Science Center (CN), Zhejiang Lab (CN), Institute of High Energy Physics (CN), Max Planck Institute for Nuclear Physics (DE), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN), Huazhong University of Science and Technology (CN), Southwest Jiaotong University (CN), China Center of Advanced Science and Technology (CN), Universidad del Noreste (MX), Nanjing University (CN), Northeastern University (CN), Hebei Normal University (CN), Tsinghua University (CN)
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Pulsars and Gravitational Waves Research
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