scholarly journals Cosmological Tests of Gravity with the Latest Observations

2019 ◽  
Vol 871 (2) ◽  
pp. 196 ◽  
Author(s):  
Jian Li ◽  
Gong-Bo Zhao
2010 ◽  
Vol 325 (7) ◽  
pp. 1479-1516 ◽  
Author(s):  
Bhuvnesh Jain ◽  
Justin Khoury

2008 ◽  
Vol 23 (17n20) ◽  
pp. 1252-1265 ◽  
Author(s):  
JÉRÔME MARTIN

Models where the accelerated expansion of our Universe is caused by a quintessence scalar field are reviewed. In the framework of high energy physics, the physical nature of this field is discussed and its interaction with ordinary matter is studied and explicitly calculated. It is shown that this coupling is generically too strong to be compatible with local tests of gravity. A possible way out, the chameleon effect, is also briefly investigated.


2007 ◽  
Author(s):  
László Á. Gergely ◽  
Zoltán Keresztes ◽  
Gyula M. Szabó ◽  
Arttu Rajantie ◽  
Carlo Contaldi ◽  
...  

Author(s):  
Simone Rijavec ◽  
Matteo Carlesso ◽  
Angelo Bassi ◽  
Vlatko Vedral ◽  
Chiara Marletto
Keyword(s):  

Author(s):  
G. Mathez ◽  
Y. Mellier ◽  
J.-P. Picat ◽  
L. Van Waerbeke
Keyword(s):  

2021 ◽  
pp. 425-450
Author(s):  
Yashar Akrami ◽  
Matteo Martinelli
Keyword(s):  

Author(s):  
Timothy Clifton

By studying objects outside our Solar System, we can observe star systems with far greater gravitational fields. ‘Extrasolar tests of gravity’ considers stars of different sizes that have undergone gravitational collapse, including white dwarfs, neutron stars, and black holes. A black hole consists of a region of space-time enclosed by a surface called an event horizon. The gravitational field of a black hole is so strong that anything that finds its way inside the event horizon can never escape. Other star systems considered are binary pulsars and triple star systems. With the invention of even more powerful telescopes, there will be more tantalizing possibilities for testing gravity in the future.


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