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white dwarfPlace
A simple cooling model of white dwarf stars is re-analyzed in Palatini $f(R)$ gravity. Modified gravity affects the white dwarf structures and consequently their ages. We find that the resulting super-Chandrasekhar white dwarfs need more time to cool down than sub-Chandrasekhar ones, or when compared to the Newtonian models.Comment: 9 pages including 3 figures; comments welcom
This article belongs to the Special Issue Physics and Symmetry Section: Feature Papers 2022.We inves...
We investigate the effect of the quadratic correction $\alpha R^2$ and non-minimal coupling $\xi \ph...
Context. An accurate assessment of white dwarf cooling times is paramount so that white dwarf cosmoc...
We analyze the effects of modified gravity on specific heats of electrons and ions, Debye temperatur...
We investigate the Chandrasekhar mass limit for white dwarfs in various models of $f(R)$ gravity. Tw...
Cooling processes of brown dwarf stars and giant planets are studied in the framework of DHOST theor...
As dense and hot bodies with a well-understood equation of state, white dwarfs offer a unique opport...
In recent times, there has been an increasing interest with theories of modified gravity as a means ...
We investigate electromagnetic and gravitational radiation generated during a process of the tidal s...
A recent analysis of the 100 pc white dwarf sample in the SDSS footprint demonstrated for the first ...
In the context of $f\left(R, T\right) = R + 2 \beta T$ gravity, where $R$ is the Ricci scalar and $T...
We present new white dwarf cooling models which incorporate an accurate outer boundary condition bas...
White dwarfs are the most common stellar evolutionary end-point. Moreover, they can be considered as...
We study the effects of light QCD axions on the stellar configuration of white dwarfs. At finite bar...
In the first part of the paper, we study the evolution of hot horizontal-branch models which miss th...
This article belongs to the Special Issue Physics and Symmetry Section: Feature Papers 2022.We inves...
We investigate the effect of the quadratic correction $\alpha R^2$ and non-minimal coupling $\xi \ph...
Context. An accurate assessment of white dwarf cooling times is paramount so that white dwarf cosmoc...
We analyze the effects of modified gravity on specific heats of electrons and ions, Debye temperatur...
We investigate the Chandrasekhar mass limit for white dwarfs in various models of $f(R)$ gravity. Tw...
Cooling processes of brown dwarf stars and giant planets are studied in the framework of DHOST theor...
As dense and hot bodies with a well-understood equation of state, white dwarfs offer a unique opport...
In recent times, there has been an increasing interest with theories of modified gravity as a means ...
We investigate electromagnetic and gravitational radiation generated during a process of the tidal s...
A recent analysis of the 100 pc white dwarf sample in the SDSS footprint demonstrated for the first ...
In the context of $f\left(R, T\right) = R + 2 \beta T$ gravity, where $R$ is the Ricci scalar and $T...
We present new white dwarf cooling models which incorporate an accurate outer boundary condition bas...
White dwarfs are the most common stellar evolutionary end-point. Moreover, they can be considered as...
We study the effects of light QCD axions on the stellar configuration of white dwarfs. At finite bar...
In the first part of the paper, we study the evolution of hot horizontal-branch models which miss th...
This article belongs to the Special Issue Physics and Symmetry Section: Feature Papers 2022.We inves...
We investigate the effect of the quadratic correction $\alpha R^2$ and non-minimal coupling $\xi \ph...
Context. An accurate assessment of white dwarf cooling times is paramount so that white dwarf cosmoc...
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