--- title: "Back-Reaction of Einstein's Gravitational-Waves as the Origin of Natal Pulsar Kicks • CBPF Index" description: "CBPF INDEX es el sistema de seguimiento de la producción científica y tecnológica del CBPF. En él se puede obtener la lista de publicaciones de artículos, libros, informes técnicos, etc. de toda la comunidad del CBPF." canonical_url: "https://index.cbpf.br/es/publicacoes/6ad2a767639f62b11adbb3ed" locale: es meta: "og:description": "CBPF INDEX es el sistema de seguimiento de la producción científica y tecnológica del CBPF. En él se puede obtener la lista de publicaciones de artículos, libros, informes técnicos, etc. de toda la comunidad del CBPF." "og:image": "https://index.cbpf.br/_og/d/c_Item%2Ctitulo_Back-Reaction%2Bof%2BEinstein's%2BGravitational-Waves%2Bas%2Bthe%2BOrigin%2Bof%2BNatal%2BPulsar%2BKicks%2Ctipo_~Tm90YSBkZSBGw61zaWNh%2Ccor_~I2E4MmMwMA%2Cautores_Herman%2BJ.%2BMosquera%2BCuesta%2Cdetalhe_2000%2Csecao_Publicaciones%2Cp_Ii9lcy9wdWJsaWNhY29lcy82YWQyYTc2NzYzOWY2MmIxMWFkYmIzZWQi%2Cs_hy-y2V873gG7z2sL.png" "og:image:height": "600" "og:image:type": image/png "og:image:width": "1200" "og:title": "Back-Reaction of Einstein's Gravitational-Waves as the Origin of Natal Pulsar Kicks • CBPF Index" "twitter:image": "https://index.cbpf.br/_og/d/c_Item%2Ctitulo_Back-Reaction%2Bof%2BEinstein's%2BGravitational-Waves%2Bas%2Bthe%2BOrigin%2Bof%2BNatal%2BPulsar%2BKicks%2Ctipo_~Tm90YSBkZSBGw61zaWNh%2Ccor_~I2E4MmMwMA%2Cautores_Herman%2BJ.%2BMosquera%2BCuesta%2Cdetalhe_2000%2Csecao_Publicaciones%2Cp_Ii9lcy9wdWJsaWNhY29lcy82YWQyYTc2NzYzOWY2MmIxMWFkYmIzZWQi%2Cs_hy-y2V873gG7z2sL.png" --- > Index of every page on this site: [llms.txt](https://index.cbpf.br/llms.txt) **Nota de Física****Publicado** # **Back-Reaction of Einstein's Gravitational-Waves as the Origin of Natal Pulsar Kicks** **Herman J. Mosquera Cuesta** 2000 [**Descargar PDF **0,1 MB](https://index.cbpf.br/files/publicacao/6ad2a767639f62b11adbb3ed/pdf) [**Contactar al responsable**](mailto:apub@cbpf.br?subject=Back-Reaction%20of%20Einstein's%20Gravitational-Waves%20as%20the%20Origin%20of%20Natal%20Pulsar%20Kicks) ## **Datos de la publicación**
Autores
Herman J. Mosquera Cuesta
Tipo
Nota de Física
Estado
Publicado
Fecha de publicación
2000
Descripción
Pulsars are observed to be born with mean spatial (3-D) velocities of ~ 450 kms<math>^{-1}</math> [1,2]. Since most stars in our galaxy are observed to possess mean velocities of ~ 30 kms<math>^{-1}</math> [3], it has been suggested such large velocities should be given to the proto-neutron star at its birth. The mechanism responsible for the impulses has not been properly identified, despite of interesting proposals have been advanced [4,5]. Here I identify such a mechanism to be linked to the ''back-reaction force'' of the ''gravitational wave burst'' released during the first millisecond after the core bounce of a supernova collapse. This behavior of the gravity wave is predicted by Einstein's general relativity theory. It turns that the overwhelming population of fast moving pulsars cataloged, compared to the tiny one of neutron star-neutron star binaries [6], makes these objects the most compelling evidence for the existence of gravitational waves, and correspondently points towards the Einstein theory of gravitation as the most correct one.
Año
2000
Número
CBPF-NT-081/00
Vínculo con tesis
No
Vínculo con beca
No
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