中文
相关论文

相关论文: The observational signatures of high-redshift dark…

200 篇论文

The first stars in the history of the Universe are likely to form in the dense central regions of 10^5-10^6 Msolar cold dark matter halos at z=10-50. The annihilation of dark matter particles in these environments may lead to the formation…

Some of the first stars could be cooler and more massive than standard stellar models would suggest, due to the effects of dark matter annihilation in their cores. It has recently been argued that such objects may attain masses in the…

The first stars to form in the history of the universe may have been powered by dark matter annihilation rather than by fusion. This new phase of stellar evolution may have lasted millions to billions of years. These dark stars can grow to…

宇宙学与河外天体物理 · 物理学 2010-11-23 K. Freese , E. Ruiz , M. Valluri , C. Ilie , D. Spolyar , P. Bodenheimer

We study the capability of the James Webb Space Telescope (JWST) to detect Supermassive Dark Stars (SMDS). If the first stars are powered by dark matter heating in triaxial dark matter haloes, they may grow to be very large and very bright,…

宇宙学与河外天体物理 · 物理学 2016-11-09 Cosmin Ilie , Katherine Freese , Monica Valluri , Ilian T. Iliev , Paul Shapiro

The James Webb Space Telescope (JWST) has recently conducted observations of massive galaxies at high redshifts, revealing a notable anomaly in their star formation efficiency (SFE). Motivated by the recent identification of three $\sim…

宇宙学与河外天体物理 · 物理学 2025-05-12 Lei Lei , Yi-Ying Wang , Guan-Wen Yuan , Tong-Lin Wang , Martin A. T. Groenewegen , Yi-Zhong Fan

Gravitational lensing may render individual high-mass stars detectable out to cosmological distances, and several extremely magnified stars have in recent years been detected out to redshifts $z\approx 6$. Here, we present Muspelheim, a…

The first population III stars are predicted to form in minihalos at a redshift of approximately 10-30. The James Webb Space Telescope (JWST), tentatively scheduled for launch in 2018, will probably be able to detect some of the first…

宇宙学与河外天体物理 · 物理学 2013-08-02 Claes-Erik Rydberg , Erik Zackrisson , Peter Lundqvist , Pat Scott

The high sensitivity of JWST will open a new window on the end of the cosmological dark ages. Small stellar clusters, with a stellar mass of several 10^6 M_sun, and low-mass black holes (BHs), with a mass of several 10^5 M_sun should be…

天体物理学 · 物理学 2015-05-13 Zoltan Haiman

JWST is discovering star forming `candidate' galaxies with photometric redshifts $z>9$ and little attenuation. We model presumptive massive black holes (MBHs) in such galaxies and find that their unobscured emission is fainter than the…

星系天体物理 · 物理学 2023-03-06 Marta Volonteri , Melanie Habouzit , Monica Colpi

High redshift quasars emit copious X-ray photons which heat the intergalactic medium to temperatures up to $\sim$ 10$^6$ K. At such high temperatures the primordial gas will not form stars until it is assembled into dark matter haloes with…

星系天体物理 · 物理学 2019-07-10 Jarrett L. Johnson , Aycin Aykutalp

We propose a novel use of high-redshift galaxies, discovered in deep Hubble Space Telescope (HST) fields around strong lensing clusters. These fields probe small comoving volumes (about 1000 cubic Mpc) at high magnification ({\mu} > 10),…

宇宙学与河外天体物理 · 物理学 2013-08-15 Fabio Pacucci , Andrei Mesinger , Zoltan Haiman

Isolated population III stars are postulated to exist at approximately z=10-30 and may attain masses up to a few hundred solar masses. The James Webb Space telescope (JWST) is the next large space based infrared telescope and is scheduled…

宇宙学与河外天体物理 · 物理学 2011-03-08 C. -E. Rydberg , E. Zackrisson , P. Scott

The presence of supermassive black holes (SMBHs) at high redshifts ($z>5$), as revealed by James Webb Space Telescope (JWST), challenges standard black hole (BH) formation scenarios. We propose a mechanism in which non-annihilating dark…

高能物理 - 唯象学 · 物理学 2026-01-05 Sulagna Bhattacharya , Debajit Bose , Basudeb Dasgupta , Jaya Doliya , Ranjan Laha

The James Webb Space Telescope (JWST) has recently uncovered a new record-breaking quasar, UHZ1, at a redshift of $z\sim10$. This discovery continues JWST's trend of confronting the expectations from the standard $\Lambda$CDM model of…

星系天体物理 · 物理学 2023-12-22 Cosmin Ilie , Katherine Freese , Andreea Petric , Jillian Paulin

Deep imaging of galaxy cluster fields have in recent years revealed tens of candidates for gravitationally lensed stars at redshifts $z\approx$ 1-6, and future searches are expected to reveal highly magnified stars from even earlier epochs.…

星系天体物理 · 物理学 2024-10-23 Emma Lundqvist , Erik Zackrisson , Calum Hawcroft , Anish M. Amarsi , Brian Welch

Dark Stars are the very first phase of stellar evolution in the history of the universe: the first stars to form (typically at redshifts $z \sim 10-50$) are powered by heating from dark matter (DM) annihilation instead of fusion (if the DM…

天体物理学 · 物理学 2011-02-11 Katherine Freese , Peter Bodenheimer , Douglas Spolyar , Paolo Gondolo

Surveys with James Webb Space Telescope (JWST) have discovered candidate galaxies in the first 400 Myr of cosmic time. Preliminary indications have suggested these candidate galaxies may be more massive and abundant than previously thought.…

The first generation of stars in the Universe is yet to be observed. There are two leading theories for those objects that mark the beginning of the cosmic dawn: hydrogen burning Population~III stars and Dark Stars, made of hydrogen and…

宇宙学与河外天体物理 · 物理学 2023-08-16 Cosmin Ilie , Jillian Paulin , Katherine Freese

Gravitationally lensed galaxies with magnification ~10-100 are routinely detected at high redshifts, but magnifications significantly higher than this are hampered by a combination of low probability and large source sizes. Magnifications…

宇宙学与河外天体物理 · 物理学 2015-06-23 Erik Zackrisson , Juan Gonzalez , Simon Eriksson , Saghar Asadi , Chalence Safranek-Shrader , Michele Trenti , Akio K. Inoue

Dark stars powered by dark matter annihilation have been proposed as the first luminous sources in the universe. These stars are believed to form in the central dark matter cusp of low-mass minihalos. Recent calculations indicate stellar…

天体物理学 · 物理学 2009-08-26 Dominik R. G. Schleicher , Robi Banerjee , Ralf S. Klessen
‹ 上一页 1 2 3 10 下一页 ›