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pro vyhledávání: '"Shirke AN"'
This study explores the effectiveness of layer pruning for developing more efficient BERT models tailored to specific downstream tasks in low-resource languages. Our primary objective is to evaluate whether pruned BERT models can maintain high perfor
Externí odkaz:
http://arxiv.org/abs/2501.00733
Autor:
Shirke, Parisee S., Shirke, Swarnim S.
The paper presents model pulse profiles from binary accreting X-ray pulsars using high-resolution numerical simulations for pencil and fan emission beam geometries, each with two different optical depths obtained using a new numerical code $\texttt{A
Externí odkaz:
http://arxiv.org/abs/2408.07509
Autor:
Chen, Tiejin, Shirke, Prithvi, Chakravarthi, Bharatesh, Vaghela, Arpitsinh, Da, Longchao, Lu, Duo, Yang, Yezhou, Wei, Hua
This paper introduces SynTraC, the first public image-based traffic signal control dataset, aimed at bridging the gap between simulated environments and real-world traffic management challenges. Unlike traditional datasets for traffic signal control
Externí odkaz:
http://arxiv.org/abs/2408.09588
Autor:
Shirke, Parisee S.
Publikováno v:
ApJ 977 (2024) 139
Free-Free Gaunt factors for X-ray absorption by hot plasma in the presence of a strong magnetic field are reported. Modified formulae are used for application to the non-local thermodynamic equilibrium conditions found in accreting pulsar atmospheres
Externí odkaz:
http://arxiv.org/abs/2408.07512
Autor:
Shirke, Parisee S., Dewangan, Gulab C.
The pulse shapes simulated in the accompanying paper Part $-$ I are compared with observations of a model binary accreting X-ray pulsar, Centaurus X-3. With known Cen X-3 inclination angles provided as input to the $\texttt{AXP4}$ code, the generated
Externí odkaz:
http://arxiv.org/abs/2408.07504
Autor:
Shirke, Swarnim, Pradhan, Bikram Keshari, Chatterjee, Debarati, Sagunski, Laura, Schaffner-Bielich, Jürgen
Publikováno v:
PRD 110.6, 063025 (2024)
The effect of dark matter (DM) on $f$-mode oscillations in DM admixed neutron stars (NSs) is investigated in a comprehensive analysis with particular attention to the role of the nuclear equation of state. Hadronic matter is modeled by the relativist
Externí odkaz:
http://arxiv.org/abs/2403.18740
Autor:
Shirke, Swarnim, Ghosh, Suprovo, Chatterjee, Debarati, Sagunski, Laura, Schaffner-Bielich, Jürgen
Publikováno v:
JCAP12(2023)008
In this work, we perform the first systematic investigation of effects of the presence of dark matter on $r$-mode oscillations in neutron stars (NSs). Using a self-interacting dark matter (DM) model based on the neutron decay anomaly and a hadronic m
Externí odkaz:
http://arxiv.org/abs/2305.05664
Publikováno v:
ApJ 944 7 (2023)
At the ultra-high densities existing in the core of neutron stars, it is expected that a phase transition from baryonic to deconfined quark matter may occur. Such a phase transition would affect the underlying equation of state (EoS) as well as the o
Externí odkaz:
http://arxiv.org/abs/2210.09077
Autor:
Kadam, Uttam D. a, Pandav, Rajkumar S. a, Arde, Satyanarayan M. a, Hossain, Md. Sanower c, Dinesh, Ayyar d, Radhakrishnan, Kothalam e, Ayyar, Manikandan e, Patil, Rajendra P. b, ⁎, Shirke, Bajirao S. a, ⁎⁎
Publikováno v:
In Journal of the Indian Chemical Society January 2025 102(1)
Autor:
Saez, Pablo a, b, ⁎, Shirke, Pallavi U. c, Seth, Jyoti R. c, Alegre-Cebollada, Jorge d, Majumder, Abhijit c
Publikováno v:
In Mathematical Biosciences February 2025 380