Priyamvada Natarajan
Joseph S. and Sophia S. Fruton Professor of Astronomy and Professor of PhysicsCards
About
Research
Publications
2026
Bridging Scales: Modeling Suppressed Bondi Accretion on Black Holes and Its Impact on Galaxy Growth
Porras-Valverde A, Natarajan P, Ricarte A, Su K, Cho H, Narayan R, Prather B. Bridging Scales: Modeling Suppressed Bondi Accretion on Black Holes and Its Impact on Galaxy Growth. The Astrophysical Journal 2026, 1000: 173. DOI: 10.3847/1538-4357/ae47fd.Peer-Reviewed Original ResearchActive galactic nucleiBlack hole massHole massGas accretionBlack holeMagnetic suppressionMagnetic fieldDistribution of black hole massesLuminous active galactic nucleiMagnetically arrested disk stateJames Webb Space TelescopeAccretion rate regimeLow-redshift constraintsBlack hole growthHot gas accretionGalaxy-formation modelsGalactic nucleiGRMHD simulationsGalaxy growthStellar massBondi accretionCircumgalactic mediumSpace TelescopeAccretion physicsGalaxy assemblyMESA-QUEST: Tracing the Formation of Direct Collapse Black Hole Seeds via Quasi-stars
Santarelli A, Campbell C, Farag E, Bellinger E, Natarajan P, Caplan M. MESA-QUEST: Tracing the Formation of Direct Collapse Black Hole Seeds via Quasi-stars. The Astrophysical Journal 2026, 998: 150. DOI: 10.3847/1538-4357/ae371e.Peer-Reviewed Original ResearchSupermassive black holesBlack holeQuasi-starAccreting black holesBlack hole seedsMass-loss prescriptionRelativistic radiation hydrodynamicsRadiation-driven windsEnvelope accretionStellar windBondi accretionAccretion physicsBH seedsMESA codeGas cloudsRadiation hydrodynamicsMagnetic fieldAccretionMass ratioHolesConvection modelChandraJWSTGalaxiesConvection regimeBridging Scales: How Much Do Supermassive Black Holes Grow in the Suppressed Bondi Regime?
Su K, Ricarte A, Natarajan P, Porras-Valverde A, Cho H, Narayan R, Faucher-Giguère C, Hopkins P, Prather B. Bridging Scales: How Much Do Supermassive Black Holes Grow in the Suppressed Bondi Regime? The Astrophysical Journal Letters 2026, 998: l18. DOI: 10.3847/2041-8213/ae3724.Peer-Reviewed Original ResearchSupermassive black holesBlack holeBlack hole-galaxy scaling relationsCoevolution of supermassive black holesLow-luminosity active galactic nucleiSupermassive black hole massSupermassive black hole populationEffective accretion ratesSpin-dependent mannerActive galactic nucleiBlack hole accretionQuenching star formationRelativistic windGalactic nucleiHost galaxiesStar formationCircumgalactic mediumAccretion modeCosmic timeEvent horizonAccretion rateMagnetic stressesSelf-consistentlyMassive seedsScaling relationsTracking the Assembly of Supermassive Black Holes: A Comparison of Diverse Models across Cosmic Time
Porras-Valverde A, Ricarte A, Natarajan P, Somerville R, Gabrielpillai A, Yung L. Tracking the Assembly of Supermassive Black Holes: A Comparison of Diverse Models across Cosmic Time. The Astrophysical Journal 2026, 998: 48. DOI: 10.3847/1538-4357/ae2fb1.Peer-Reviewed Original ResearchBlack hole mass functionSupermassive black holesActive galactic nucleiSemianalytical modelBlack holeMass functionAssembly of supermassive black holesBroad-line active galactic nucleiLocal black hole mass functionActive galactic nucleus activityHot-mode accretionAGN luminosity functionSuper-Eddington accretionBlack hole mergersStellar mass functionMBH ~Galactic nucleiCold accretionDisk instabilityLuminosity evolutionLuminosity functionAccretion modeCosmic timeTotal mass budgetMass assemblyEvolutionary Tracks and Spectral Properties of Quasi-stars and Their Correlation with Little Red Dots
Santarelli A, Farag E, Bellinger E, Natarajan P, Naidu R, Campbell C, Caplan M. Evolutionary Tracks and Spectral Properties of Quasi-stars and Their Correlation with Little Red Dots. The Astrophysical Journal Letters 2026, 998: l4. DOI: 10.3847/2041-8213/ae3713.Peer-Reviewed Original ResearchSupermassive black holesQuasi-starBlack holeBolometric luminosityOrigin of supermassive black holesDirect-collapse black holesNumber densityBalmer line absorptionBlack hole massSpectral energy distributionGrid of modelsStellar absorption featuresEvolutionary modelsSpectral propertiesBalmer breakCalcium tripletHole massEarly universeHigher redshiftsEvolutionary tracksStellar spectraSurface gravityContinuum spectrumSynthetic spectraLine absorptionHeavy Seeds and the First Black Holes: Insights from the BRAHMA Simulations
Bhowmick A, Blecha L, Torrey P, Kelley L, Natarajan P, Somerville R, Weinberger R, Garcia A, Hernquist L, Di Matteo T, Kho J, Vogelsberger M. Heavy Seeds and the First Black Holes: Insights from the BRAHMA Simulations. The Astrophysical Journal 2026, 997: 187. DOI: 10.3847/1538-4357/ae2607.Peer-Reviewed Original ResearchActive galactic nucleiM BHGas accretionBH evolutionActive galactic nucleus feedbackLyman–Werner fluxMetal-poor gasConsistent with current estimatesBH accretionBH mergersGalactic nucleiMerger timescaleStar formationBH dynamicsBlack holeBondi–HoyleOverdense regionsGN-z11AccretionSeed modelQuasarsBHMergerMass ratioUnique constraintsVariability as a new discovery channel for intermediate-mass black holes in the time-domain era
Burke C, Natarajan P. Variability as a new discovery channel for intermediate-mass black holes in the time-domain era. Nature Astronomy 2026, 10: 187-195. DOI: 10.1038/s41550-025-02759-5.Peer-Reviewed Original ResearchIntermediate-mass black holesBlack holeAssembly historyPopulation of supermassive black holesStellar-mass black holesGrowth of black holesVera C. Rubin ObservatoryHierarchical growthQuiescent black holesActive galactic nucleiBlack hole formationSupermassive black holesGalactic nucleiTidal disruptionCosmic timeDiscovery channelHole formationHolesVariability studiesLIGO/Virgo/KAGRAObservatorySkyNucleusConstraining the Nature of Dark Matter from Tidal Radii of Cluster Galaxy Subhalos
Chiang B, Dutra I, Natarajan P. Constraining the Nature of Dark Matter from Tidal Radii of Cluster Galaxy Subhalos. The Astrophysical Journal 2026, 997: 106. DOI: 10.3847/1538-4357/ae23c1.Peer-Reviewed Original ResearchCollisionless cold dark matterSelf-interacting dark matterDark matterTidal radiusSpatial distribution of dark matterDensity profileDensity profiles of subhaloesNature of dark matterDistribution of dark matterCold dark matterRam pressure strippingWeak lensing constraintsCentral density slopeVirial mass M200Core collapseGalaxy clustersLensing clustersGravitational lensingTruncation radiusLensing dataDensity slopeIllustrisTNG simulationsLensing constraintsMass M200SubhalosThe first GLIMPSE of the faint galaxy population at Cosmic Dawn with JWST: The evolution of the ultraviolet luminosity function across z ∼ 9−15
Chemerynska I, Atek H, Furtak L, Chisholm J, Endsley R, Kokorev V, Rosdahl J, Blaizot J, Adamo A, Bouwens R, Fujimoto S, Korber D, Mason C, McQuinn K, Muñoz J, Natarajan P, Nelson E, Oesch P, Pan R, Richard J, Saldana-Lopez A, Schaerer D, Volonteri M, Zitrin A, Berg D, Claeyssens A, Dessauges-Zavadsky M, Jecmen M, Labbé I, Naidu R, Trebitsch M. The first GLIMPSE of the faint galaxy population at Cosmic Dawn with JWST: The evolution of the ultraviolet luminosity function across z ∼ 9−15. Monthly Notices Of The Royal Astronomical Society 2026, 546: staf2267. DOI: 10.1093/mnras/staf2267.Peer-Reviewed Original ResearchUV luminosity functionLuminosity functionGalaxy populationCosmic star formation rate densityBursty star formation historiesEvolving initial mass functionStar formation rate densityPhases of galaxy formationLow-redshift contaminantsUltraviolet luminosity functionInitial mass functionStar formation historyFaint-end slopeStar formation efficiencyFaint galaxy populationDust attenuationGalaxy candidatesRedshift evolutionFaint-endGalaxy formationGLIMPSE surveyCosmic varianceGravitational lensingFaint galaxiesFormation history
2025
A Luminous and Hot Infrared through X-Ray Transient at a 5 kpc Offset from a Dwarf Galaxy
Somalwar J, Ravi V, Margutti R, Chornock R, Natarajan P, Lu W, Angus C, Graham M, Hammerstein E, Nathan E, Nicholl M, Sharma K, Stein R, Verdi F, Yao Y, Bellm E, Chen T, Coughlin M, Hale D, Kasliwal M, Laher R, Riddle R, Sollerman J. A Luminous and Hot Infrared through X-Ray Transient at a 5 kpc Offset from a Dwarf Galaxy. The Astrophysical Journal 2025, 995: 228. DOI: 10.3847/1538-4357/ae1501.Peer-Reviewed Original ResearchOptical transientsTidal disruption eventsX-ray transientsStar formation rateX-ray emissionMillimeter emissionOptical flaresHost galaxiesDwarf galaxiesBlack holeEvolution timescalesOptical emissionAccretion eventsLate-timeLow massGalaxiesHigh energyDay timescaleDensity profileX-rayFormation rateDisruptive eventsEarly timesEmissionTimescales