Zobrazeno 1 - 10
of 37 672
pro vyhledávání: '"SINGH, G."'
The expansion dynamics of the universe in $f(Q)$ gravity is examined with the Gong-Zhang kind of dark energy equation of state parameter. By considering the $f(Q)$ gravity form $f(Q)=Q+ \alpha Q^{n}$, we obtain the Hubble parameters in terms of redsh
Externí odkaz:
http://arxiv.org/abs/2410.18568
Publikováno v:
Eur. Phys. J. Spec. Top. (2024)
This study examines the radiative capture of a neutron by $^{10}$Be using the Coulomb dissociation approach within the FRDWBA theory. We analyze the elastic Coulomb breakup of $^{11}$Be on a $^{208}$Pb target at 72 MeV/A to determine the photodisinte
Externí odkaz:
http://arxiv.org/abs/2407.16775
In this study, we construct a theoretical framework based on the generalized Hubble parameter form which may arise within the particle creation, viscous and $f(R)$ gravity theory. The Hubble parameter is scrutinized for its compatibility with the obs
Externí odkaz:
http://arxiv.org/abs/2405.15626
Autor:
Singh, G.
While forming an ($A$+2) nucleus from a nucleus $A$ via a two-neutron transfer reaction, the constructive interference of the many possible reaction channels favors significant pairing enhancement through the continuum of the intermediate ($A$+1) nuc
Externí odkaz:
http://arxiv.org/abs/2402.14964
We calculate the $^{11}$B$(n,\gamma)^{12}$B reaction rate, an important constituent in nucleosynthesis networks, contributed by resonant as well as non-resonant capture. For the resonant rate, we use the narrow resonance approximation whereas the non
Externí odkaz:
http://arxiv.org/abs/2402.06755
In this paper, we examine the universe's expansion in $ f(R, L_{m}) $ gravity for a particular form of $ f(R, L_{m})=\frac{R}{2}+L_{m}^{n}$. The field equations for flat FLRW metric with matter Lagrangian $ L_{m}=\rho$ are derive. Hubble parameter in
Externí odkaz:
http://arxiv.org/abs/2310.17340
Autor:
Giuffrida A, Saia-Owenby C, Andriano C, Beall D, Bailey-Classen A, Buchanan P, Budwany R, Desai MJ, Comer A, Dudas A, Tieppo Francio V, Grace W, Gill B, Grunch B, Goldblum A, Garcia RA, Lee DW, Lavender C, Lawandy M, Mandell L, Mata R, Rabii M, Patel K, Patel RG, Patel AA, Sayed D, Singh G, Strand N, Tate J, Schatman ME, Deer T
Publikováno v:
Journal of Pain Research, Vol Volume 17, Pp 3587-3599 (2024)
Anthony Giuffrida,1 Christy Saia-Owenby,2 Chris Andriano,3,* Douglas Beall,4,* Ashley Bailey-Classen,5,* Patrick Buchanan,6,* Ryan Budwany,7,* Mehul J Desai,8,* Ashley Comer,9,* Andrew Dudas,10,* Vinicius Tieppo Franci
Externí odkaz:
https://doaj.org/article/9103d8ab1c164db981899ec5aaca51c0
Autor:
Jovanovic, N., Cvetojevic, N., Schwab, C., Norris, B., Lozi, J., Gross, S., Betters, C., Singh, G., Guyon, O., Martinache, F., Doughty, D., Tuthill, P.
High-order wavefront correction is not only beneficial for high-contrast imaging, but also spectroscopy. The size of a spectrograph can be decoupled from the size of the telescope aperture by moving to the diffraction limit which has strong implicati
Externí odkaz:
http://hdl.handle.net/10150/622807
http://arizona.openrepository.com/arizona/handle/10150/622807
http://arizona.openrepository.com/arizona/handle/10150/622807
Autor:
Jovanovic, N., Guyon, O., Lozi, J., Currie, T., Hagelberg, J., Norris, B., Singh, G., Pathak, P., Doughty, D., Goebel, S., Males, J., Kuhn, J., Serabyn, E., Tuthill, P., Schworer, G., Martinache, F., Kudo, T., Kawahara, H., Kotani, T., Ireland, M., Feger, T., Rains, A., Bento, J., Schwab, C., Coutts, D., Cvetojevic, N., Gross, S., Arriola, A., Lagadec, T., Kasdin, J., Groff, T., Mazin, B., Minowa, Y., Takato, N., Tamura, M., Takami, H., Hayashi, M.
SCExAO is the premier high-contrast imaging platform for the Subaru Telescope. It offers high Strehl ratios at near-IR wavelengths (y-K band) with stable pointing and coronagraphs with extremely small inner working angles, optimized for imaging faint
Externí odkaz:
http://hdl.handle.net/10150/622018
http://arizona.openrepository.com/arizona/handle/10150/622018
http://arizona.openrepository.com/arizona/handle/10150/622018
We aim to explore the bubble nature of the exotic nucleus $^{20}$N within the microscopic antisymmetrized molecular dynamics (AMD) approach. Constraining its structural parameters, we analyse its static properties. Subsequently, we use the AMD infuse
Externí odkaz:
http://arxiv.org/abs/2302.06986