The Large High Altitude Air Shower Observatory (LHAASO) Science Book (2021 Edition)
arXiv:1905.02773
Abstract
Since the science white paper of the Large High Altitude Air Shower Observatory (LHAASO) published on arXiv in 2019 [e-Print: 1905.02773 (astro-ph.HE)], LHAASO has completed the transition from a project to an operational gamma-ray astronomical observatory LHAASO is a new generation multi-component facility located in Daocheng, Sichuan province of China, at an altitude of 4410 meters. It aims at measuring with unprecedented sensitivity the spectrum, composition, and anisotropy of cosmic rays in the energy range between 10 and 10~eV, and acting simultaneously as a wide aperture (one stereoradiant) continuously operating gamma-ray telescope in the energy range between 10 and ~eV with the designed sensitivity of 1.3\% of the Crab Unit (CU) above 100 TeV. LHAASO's capability of measuring simultaneously different shower components (electrons, muons, and Cherenkov/fluorescence light), will allow it to investigate the origin, acceleration, and propagation of CR through measurement of the energy spectrum, elemental composition, and anisotropy with unprecedented resolution. The remarkable sensitivity of LHAASO will play a key role in CR physics and gamma-ray astronomy for a general and comprehensive exploration of the high energy universe and will allow important studies of fundamental physics (such as indirect dark matter search, Lorentz invariance violation, quantum gravity) and solar and heliospheric physics. The LHAASO Collaboration organized an editorial working group and finished all editorial work of this science book, to summarize the instrumental features and outline the prospects of scientific researches with the LHAASO experiment.
arXiv commentThis document is a collaborative effort, 185 pages, 110 figures
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- Revealing a peculiar supernova remnant G106.3+2.7 as a petaelectronvolt proton accelerator with X-ray observations
- Nearby SN-Associated GRB~190829A: Environment, Jet Structure, and VHE Gamma-Ray Afterglows
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- Using Interstellar Clouds to Search for Galactic PeVatrons: Gamma-ray Signatures from Supernova Remnants
- Ground-based gamma-ray astronomy: history and development of techniques
- Design and Development of the Core Software for STCF Offline Data Processing
- Detection of UHE gamma rays from the Crab Nebula: Physical Implications
- Investigating the multiband nonthermal emission of the 100 TeV source eHWC J2019368 with a pulsar wind nebula scenario
- Searching for Exploding Black Holes
- Ultra-High-Energy Gamma-Ray Astronomy
- Morphology of Gamma-Ray Halos around Middle-Aged Pulsars: Influence of the Pulsar Proper Motion
- Search for the Hawking radiation of primordial black holes: prospective sensitivity of LHAASO
- A Three-component Model for Cosmic-ray Spectrum and Dipole Anisotropy
- Sensitivity reach of gamma-ray measurements for strong cosmological magnetic fields
- Expected Signature For the Lorentz Invariance Violation Effects on Absorption
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- Probes for String-Inspired Foam, Lorentz, and CPT Violations in Astrophysics
- Probing the nova shock physics with future gamma-ray observations of the upcoming outburst from T Coronae Borealis
- Evaluation of Hadronic Emission in Starburst Galaxies and Star-forming Galaxies
- A Universal Energy Relation between synchrotron and Synchrotron Self-Compton radiation in GRBs and Blazars
- TeV afterglow from GRB 221009A: photohadronic origin?
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