The influence of rotation deceleration on the shape of a pulsar may reflect on the star's braking index
Author:
Affiliation:
1. Sao Paulo Federal Institute Sao Paulo Federal Institute (IFSP) Sao Paulo Brazil
2. Department of Physics Federal University of Sao Paulo (UNIFESP) Diadema Brazil
Funder
CNPq
Fundação de Amparo à Pesquisa do Estado de São Paulo
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.202113908
Reference28 articles.
1. The gravitational wave detector "Mario Schenberg": status of the project
2. Effect of Angular Velocity on Sensors Based on Morphology Dependent Resonances
3. Ultra-low phase noise 10 GHz oscillator to pump the parametric transducers of the Mario Schenberg gravitational wave detector
4. Negative Poisson's Ratios for Extreme States of Matter
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