03628nam a22005655i 4500001001800000003000900018005001700027007001500044008004100059020003700100024003500137050001400172072001700186072002300203072001600226245015800242250001800400264007200418300006600490336002600556337002600582338003600608347002400644490006200668505021500730520123700945650002502182650003402207650001702241650002402258650003402282650002602316650002502342650002402367650004202391650005202433650006402485700008302549700010202632710003402734773002602768776003602794776003602830776003602866830006902902856004602971912001403017912001403031999001703045978-981-97-2871-8DE-He21320251030112622.0cr nn 008mamaa240710s2024    si |    s    |||| 0|eng d  a97898197287189978-981-97-2871-87 a10.1007/978-981-97-2871-82doi 4aQB460-466 7aPHVB2bicssc 7aSCI0050002bisacsh 7aPHVB2thema10aRecent Progress on Gravity Testsh[electronic resource] :bChallenges and Future Perspectives /cedited by Cosimo Bambi, Alejandro Cárdenas-Avendaño.  a1st ed. 2024. 1aSingapore :bSpringer Nature Singapore :bImprint: Springer,c2024.  aVIII, 463 p. 76 illus., 69 illus. in color.bonline resource.  atextbtxt2rdacontent  acomputerbc2rdamedia  aonline resourcebcr2rdacarrier  atext filebPDF2rda1 aSpringer Series in Astrophysics and Cosmology,x2731-73580 a1. Testing gravity in laboratory -- 2. Testing gravity with Solar System experiments -- 3. Testing gravity with pulsars -- 4. Testing gravity with neutron stars -- 5. Testing gravity with black hole X-ray data.  aEinstein's theory of general relativity is one of the pillars of modern physics and it is our standard framework for describing gravitational fields and the spacetime structure. So far, general relativity has passed all experimental tests and agrees with observations. However, the past few years have seen remarkable observational improvements and new techniques that continually challenge the theory's predictions: routinely detect the gravitational wave signals from the coalescence of black holes and neutron stars; can image the supermassive black holes at the center of our Galaxy and of the galaxy M87; can analyze the properties of the X-ray radiation emitted from the very inner part of the accretion disks of several black holes; and keep improving laboratory and Solar System experiments. This book offers an updated self-consistent overview, future perspectives, and challenges of experimental and observational tests of gravity, with both gravitational and electromagnetic spectra. It includes the recent results of laboratory tests of gravity, solar system experiments, tests of gravity in the strong-field regime with astrophysical compact objects, and tests of gravity on large scales with cosmological observations. 0aAstrophysics.968037 0aGeneral relativity (Physics). 0aGravitation. 0aMeasurement.967386 0aMeasuring instruments.967387 0aMathematical physics.14aAstrophysics.96803724aGeneral Relativity.24aClassical and Quantum Gravity.96940924aMeasurement Science and Instrumentation.96738924aTheoretical, Mathematical and Computational Physics.9655631 aBambi, Cosimo.eeditor.4edt4http://id.loc.gov/vocabulary/relators/edt9803171 aCárdenas-Avendaño, Alejandro.eeditor.4edt4http://id.loc.gov/vocabulary/relators/edt9803182 aSpringerLink (Online service)0 tSpringer Nature eBook08iPrinted edition:z978981972870108iPrinted edition:z978981972872508iPrinted edition:z9789819728732 0aSpringer Series in Astrophysics and Cosmology,x2731-735897634240uhttps://doi.org/10.1007/978-981-97-2871-8  aZDB-2-PHA  aZDB-2-SXP  c61489d61489