Zobrazeno 1 - 10
of 12
pro vyhledávání: '"Darsh Kodwani"'
Publikováno v:
The Open Journal of Astrophysics, Vol 2 (2019)
Cosmological large-scale structure analyses based on two-point correlation functions often assume a Gaussian likelihood function with a fixed covariance matrix. We study the impact on cosmological parameter estimation of ignoring the parameter depend
Externí odkaz:
https://doaj.org/article/cf13f4d0098742ce9ba2b712277a511e
Publikováno v:
The Open Journal of Astrophysics, Vol 2 (2019)
Cosmological large-scale structure analyses based on two-point correlation functions often assume a Gaussian likelihood function with a fixed covariance matrix. We study the impact on cosmological parameter estimation of ignoring the parameter depend
Publikováno v:
Physical Review D, 99(12):123518. AMER PHYSICAL SOC
In the standard big bang model the universe starts in a radiation dominated era, where the gravitational perturbations are described by second order differential equations, which will generally have two orthogonal set of solutions. One is the so call
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d0e86332e5f421e5f286c3607b747260
http://arxiv.org/abs/1903.05042
http://arxiv.org/abs/1903.05042
Publikováno v:
Journal of Cosmology and Astroparticle Physics. 2021:055
We present a novel application of partial convolutional neural networks (PCNN) that can inpaint masked images of the cosmic microwave background. The network can reconstruct both the maps and the power spectra to a few percent for circular and irregu
Autor:
Harry Desmond, Darsh Kodwani
Cross-correlating two different types of galaxy gives rise to parity breaking in the correlation function that derives from differences in the galaxies' properties and environments. This is typically associated with a difference in galaxy bias, descr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf838a965937dfd18936d9c4c32cc54f
Autor:
D. Lowe, Darsh Kodwani
Publikováno v:
International Journal of Thermophysics. 36:2654-2665
Re-calibration of a thermocouple after it has been installed in a process is often not practical. In situ monitoring of performance is desirable and can be done with built-in reference standards based on melting or freezing phase transitions. Binary
We show that when a supernova explodes, a nearby pulsar signal goes through a very specific change. The observed period first changes smoothly, then is followed by a sudden change in the time derivative. A stable millisecond pulsar can allow us to me
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::925dba63f4a2663d20ebfe5931faba57
http://arxiv.org/abs/1601.03917
http://arxiv.org/abs/1601.03917
Publikováno v:
INSPIRE-HEP
When a supernova explodes, most of its energy is released in a shell of relativistic neutirnos which changes the surrounding geometry. We calculate the potentially observable responses to such a change in both pulsar scintillation and conventional in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4cc60371d9e722da01d26c1b5dd757dd
Publikováno v:
International Journal of Modern Physics A. 32:1750198
The black hole information paradox presumes that quantum field theory in curved space–time can provide unitary propagation from a near-horizon mode to an asymptotic Hawking quantum. Instead of invoking conjectural quantum-gravity effects to modify