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Silpa S

Publications and source records attributed to Silpa S.

2 recordsLinked to original sources

Hierarchically Engineered Titanium Suboxide Films for High-Efficiency Solar Thermal Conversion

We report the development of broadband solar absorber coatings based on titanium suboxide composite thin films on aluminium substrates. The films are fabricated via scalable DC magnetron sputtering using a Ti target, followed by post-annealing in a fixed $O_2$ partial pressure of 0.45 mbar. By tuning deposition time and annealing temperature, a composite phase of $Ti_2O_3$ and $TiO_2$ was achieved. The Raman mapping of the films substantiates the distribution and coexistence of the two phases. The optimized sample, deposited for 10 min and annealed at 500 $^oC$, exhibited a superior solar absorptance (${\alpha}_s$ = 0.913) and optimally low thermal emittance (${\epsilon}_t$ = 0.11). Nevertheless, the 15- and 20-min deposited films also showed a promising absorptance (>0.85) and emittance values (<0.13). Morphological studies revealed island-type nanostructures, leading to enhanced photothermal performance via electric field confinement, which is validated by optical simulations. This work provides a promising route toward efficient, scalable, and cost-effective spectrally selective solar absorbers for solar thermal applications.

cond-mat.mtrl-sci

A Kpc-scale Radio Polarization Study of PG BL Lacs with the uGMRT

We present here uGMRT band 4 (~650MHz) polarization images of 8 BL~Lac objects belonging to the Palomar-Green (PG) `blazar' sample. A large fraction of the sources (~63%) reveal core-halo radio structures with most of the polarization detected in the inner core-jet regions. PG1101+385 and PG2254+075 exhibit a `spine-sheath structure' in polarization. The core-halo and `spine-sheath' structures are consistent with the Unified Scheme suggestion that BL~Lacs are the pole-on beamed counterparts of Fanaroff-Riley (FR) type I radio galaxies. PG1418+546 and PG0851+203 (OJ287) show the presence of terminal hotspots similar to FR type II radio galaxies. They were also found to be low-spectrally peaked BL Lacs, supportive of the `blazar envelope' scenario for BL~Lacs and quasars. Fractional polarization ranges from 1-13% in the cores and 2-26% in the inner jets/lobes of the sample BL Lacs. Compared to the varied radio morphology of quasars from the PG `blazar' sample, the BL~Lacs appear to be less diverse. A comparison of the inferred core magnetic (B-) field structures on arcsec- (kpc-) scales w.r.t. the Very Long Baseline Interferometry (VLBI) jet direction does not reveal any preferred orientation, suggesting that if large-scale ordered B-fields exist, they do so on scales smaller than probed by the current observations. However, the presence of polarized emission on arcsec-scales suggests that any mixing of thermal plasma with the synchrotron emitting plasma is insufficient to fully depolarize the emission via the internal depolarization process.

astro-ph.GA