activity
20162024
most citedNew Suns in the Cosmos III: multifractal signature analysis

19 citations · 36 across the 5 of their papers we have counts for

collaborators

8 papers

gr-qc2024

Nonadditive entropy of the gravitational wave signal from GW150914

Daniel B. de Freitas, Cleo V. da Silva, Mackson M. F. Nepomuceno

We study the first gravitational wave, GW150914, detected by advanced LIGO and constructed from the data of measurement of strain relative deformation of the fabric of spacetime. W…

gr-qc2023

Multiscale structure of the gravitational wave signal from GW150914 based on the nonextensivity -triplet

C. V. da Silva, M. M. F. Nepomuceno, D. B. de Freitas

We study the first gravitational wave, GW150914, detected by advanced LIGO and constructed from the data of measurement of strain relative deformation of the fabric of spacetime. W…

astro-ph.HE2019

Multifractal signatures of gravitational waves detected by LIGO

Daniel B. de Freitas, Mackson M. F. Nepomuceno, J. R. De Medeiros

We analyze the data from the 6 gravitational waves signals detected by LIGO through the lens of multifractal formalism using the MFDMA method, as well as shuffled and surrogate pro…

astro-ph.SR2019

Multifractal detrended moving average analysis of Kepler stars with surface differential rotation traces

D. B. de Freitas, M. M. F. Nepomuceno, J. G. Cordeiro +2

A multifractal formalism is employed to analyse high-precision time-series data of \textit{Kepler} stars with surface differential rotation traces. The multifractal detrended movin…

astro-ph.SR2019

New Suns in the Cosmos V: Stellar rotation and multifractality in active \textit{Kepler} stars

D. B. de Freitas, M. M. F. Nepomuceno, L. D. Alves Rios +2

In the present study, high-precision time series photometry for the active \emph{Kepler} stars is described in the language of multifractals. We explore the potential of using the…

astro-ph.SR2019★ 3 cited

A nonextensive insight to the stellar initial mass function

D. B. de Freitas, R. T. Eufrasio, M. M. F. Nepomuceno +1

the present paper, we propose that the stellar initial mass distributions as known as IMF are best fitted by -Weibulls that emerge within nonextensive statistical mechanics. As…