Zobrazeno 1 - 10
of 511
pro vyhledávání: '"Balakrishna S"'
Publikováno v:
Cogent Engineering, Vol 11, Iss 1 (2024)
Precision machine tool structures require enhanced stability with higher static stiffness and increased damping. Granite epoxy (G-E) composite offers improved damping properties and is a promising alternative material. This study evaluates the mechan
Externí odkaz:
https://doaj.org/article/7c77d375d68a48c1b8eefd5988e4bb5e
Autor:
Deepak Nayak, Purushotham G. Sarvade, H. N. Udayashankar, Balakrishna S. Maddodi, M. Prasanna Kumar
Publikováno v:
Geosciences, Vol 14, Iss 4, p 92 (2024)
The present study explores the intricate relationship between the geotechnical and mineralogical properties of lithomargic clays in the Uttara Kannada region of south India. Lithomargic clays, characterized by their unique composition of clay mineral
Externí odkaz:
https://doaj.org/article/d9c2d02ab87445009b5cd8a53086ace3
Autor:
Andrea Lapi, Giovanni Gandolfi, Lumen Boco, Francesco Gabrielli, Marcella Massardi, Balakrishna S. Haridasu, Carlo Baccigalupi, Alessandro Bressan, Luigi Danese
Publikováno v:
Universe, Vol 10, Iss 3, p 141 (2024)
We aim to constrain the stellar initial mass function (IMF) during the epoch of reionization. To this purpose, we build up a semi-empirical model for the reionization history of the Universe based on various ingredients: the latest determination of t
Externí odkaz:
https://doaj.org/article/439ea816697641bf8317ef0f402bd592
Autor:
Francesco Benetti, Andrea Lapi, Giovanni Gandolfi, Minahil Adil Butt, Yacer Boumechta, Balakrishna S. Haridasu, Carlo Baccigalupi
Publikováno v:
Universe, Vol 9, Iss 11, p 478 (2023)
Recently, we put forward a framework where the dark matter (DM) component within virialized halos is subject to a non-local interaction originated by fractional gravity (FG) effects. In previous works, we demonstrated that such a framework can substa
Externí odkaz:
https://doaj.org/article/ebaaa56b3fd14655b3e855073ddea5e8
Autor:
Andrea Lapi, Lumen Boco, Marcos M. Cueli, Balakrishna S. Haridasu, Tommaso Ronconi, Carlo Baccigalupi, Luigi Danese
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 2, p 83 (2023)
We propose a model of the Universe (dubbed η CDM) featuring a controlled stochastic evolution of the cosmological quantities that is meant to render the effects of small deviations from homogeneity/isotropy on scales of 30–50 h ^−1 Mpc at late c
Externí odkaz:
https://doaj.org/article/5ab4347fdfc2466cb618918c00720cb7
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 2, p 105 (2023)
We look for possible evidence of a nonminimal coupling (NMC) between dark matter (DM) and gravity using data from the X-COP compilation of galaxy clusters. We consider a theoretically motivated NMC that may dynamically arise from the collective behav
Externí odkaz:
https://doaj.org/article/7f7956537e674ec3888475377c1bb96e
Utilizing the well-established Radial Tully-Fisher (RTF) relation observed in a `large' (843) sample of local galaxies, we report the maximum allowed variance in the Hubble parameter, $H_0$. We estimate the total intrinsic scatter in the magnitude of
Externí odkaz:
http://arxiv.org/abs/2403.06859
Autor:
Butt, Minahil Adil, Haridasu, Balakrishna S., Boumechta, Yacer, Benetti, Francesco, Pizzuti, Lorenzo, Baccigalupi, Carlo, Lapi, Andrea
We propose and perform a joint analysis of the two different mass estimates of galaxy clusters, namely the hydrostatic and caustic techniques. Firstly, we show comprehensively that the mass bias between these two techniques can be possibly alleviated
Externí odkaz:
http://arxiv.org/abs/2401.04698
Autor:
Lapi, Andrea, Boco, Lumen, Cueli, Marcos M., Haridasu, Balakrishna S., Ronconi, Tommaso, Baccigalupi, Carlo, Danese, Luigi
[abridged] We propose a model of the Universe (dubbed $\eta$CDM) featuring a stochastic evolution of the cosmological quantities, that is meant to render small deviations from homogeneity/isotropy on scales of $30-50\, h^{-1}$ Mpc at late cosmic time
Externí odkaz:
http://arxiv.org/abs/2310.06028
Autor:
Benetti, Francesco, Lapi, Andrea, Gandolfi, Giovanni, Haridasu, Balakrishna S., Danese, Luigi
Publikováno v:
Universe, 9 (2023), 329
[abridged] Recently, in Benetti et al. (Astrophys. J. 2023, 949, 65), we suggested that the dark matter (DM) component in galaxies may originate fractional gravity. In such a framework, the DM component exists, but the gravitational potential associa
Externí odkaz:
http://arxiv.org/abs/2307.04655