Mario Schenberg (Gravitational Wave Detector)

Nowadays, Mario Schenberg (Gravitational Wave Detector) has become a topic of great relevance in our society. With the advancement of technology and globalization, Mario Schenberg (Gravitational Wave Detector) has significantly impacted people's lives, both personally and professionally. Since its emergence, Mario Schenberg (Gravitational Wave Detector) has generated extensive debate and has been the subject of numerous studies and research. In this article, we will explore in detail all aspects related to Mario Schenberg (Gravitational Wave Detector), from its origin to its influence today. We will analyze how Mario Schenberg (Gravitational Wave Detector) has shaped our behaviors, our interactions and our environment, and reflect on the challenges and opportunities it presents.

Mario Schenberg
Alternative namesBrazilian Graviton Project Edit this at Wikidata
Location(s)São Paulo, Brazil
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The Mario Schenberg (Gravitational Wave Detector, or Brazilian Graviton Project[1] or Graviton) is a spherical, resonant-mass, gravitational wave detector formerly run by the Physics Institute of the University of São Paulo, named after Mário Schenberg. Similar to the Dutch-run MiniGrail, the 1.15 ton, 65 cm diameter spherical test mass is suspended in a cryogenic vacuum enclosure, kept at 20 mK; and the sensors (transducers) for this detector/antenna are developed at the National Institute for Space Research (INPE), in Sao José dos Campos, Brazil.[2][3] As of 2016, the antenna has not detected any gravitational waves, and development of the antenna continues. It has been decided that the antenna will be transferred from the University of São Paulo to INPE.[4]

See also

References

  1. ^ Aguiar; et al. (October 2002). "The status of the Brazilian spherical detector". Class. Quantum Grav. 19 (1949): 1949–1953. Bibcode:2002CQGra..19.1949A. doi:10.1088/0264-9381/19/7/397. S2CID 250864475.
  2. ^ Aguiar; et al. (April 2005). "The Brazilian gravitational wave detector Mario Schenberg: progress and plans". Class. Quantum Grav. 22 (10): S209 – S214. Bibcode:2005CQGra..22S.209A. CiteSeerX 10.1.1.497.325. doi:10.1088/0264-9381/22/10/011. S2CID 110087646.
  3. ^ Aguiar; et al. (May 2008). "The Schenberg spherical gravitational wave detector: the first commissioning runs". Class. Quantum Grav. 25 (11): 114042. Bibcode:2008CQGra..25k4042A. doi:10.1088/0264-9381/25/11/114042. S2CID 122231110.
  4. ^ Oliveira Jr; et al. (October 2016). "The Mario Schenberg Gravitational Wave Antenna". Brazilian Journal of Physics. 46 (5): 596–603. Bibcode:2016BrJPh..46..596O. doi:10.1007/s13538-016-0436-1. S2CID 256197402.