最清晰的引力波信号，证实了霍金的著名定理

Core Viewpoint - The article discusses the significant advancements in gravitational wave astronomy, particularly focusing on the recent detection of gravitational wave event GW250114, which confirms key theories about black holes and their properties [4][7][21]. Summary by Sections Gravitational Wave Detection - The event GW250114, detected on January 14, 2025, is similar to the first gravitational wave event GW150914 detected in 2015, both originating from the merger of black holes approximately 1.3 billion light-years away [4][7]. - The detection technology has improved significantly, allowing for clearer signals; GW250114's signal is over three times clearer than that of GW150914, with a signal-to-noise ratio of 80 [7]. Characteristics of Black Holes - The merging black holes in GW250114 have masses between 30 to 40 times that of the Sun, and the event provides insights into the nature of Kerr black holes, which are defined by mass and spin [9][12]. - The study identified at least two distinct frequencies of gravitational waves emitted during the merger, aligning with theoretical predictions for Kerr black holes [12][14]. Hawking's Area Theorem - The detection of gravitational waves from black hole mergers allows for testing Hawking's area theorem, which states that the total surface area of black holes cannot decrease over time [16][18]. - The analysis of the merger's gravitational wave signals indicated that the final black hole's surface area increased from approximately 240,000 square kilometers to about 400,000 square kilometers, confirming Hawking's prediction of an area increase of about 65% [18][20]. - This finding marks the second verification of the area theorem, with the latest results achieving a confidence level of 99.999%, significantly higher than the previous verification in 2021 [20]. Future of Gravitational Wave Astronomy - The advancements in detection technology and the clarity of signals suggest that the era of gravitational wave astronomy is just beginning, with many exciting discoveries anticipated in the future [21].