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Recently the EDGES collaboration reported an anomalous absorption signal in the sky-averaged 21-cm spectrum around $z=17$. Such a signal may be understood as an indication for an unexpected cooling of the hydrogen gas during or prior to the…

高能物理 - 唯象学 · 物理学 2018-11-14 Rennan Barkana , Nadav Joseph Outmezguine , Diego Redigolo , Tomer Volansky

The EDGES low-band experiment has measured an absorption feature in the cosmic microwave background radiation (CMB), corresponding to the 21 cm hyperfine transition of hydrogen at redshift $z \simeq 17$, before the era of cosmic…

宇宙学与河外天体物理 · 物理学 2019-11-04 Axel Widmark

The cosmic radio-frequency spectrum is expected to show a strong absorption signal corresponding to the 21-centimetre-wavelength transition of atomic hydrogen around redshift 20, which arises from Lyman-alpha radiation from some of the…

宇宙学与河外天体物理 · 物理学 2018-03-20 Rennan Barkana

Cosmic Dawn, when the first stars and proto-galaxies began to form, is commonly expected to be accompanied by an absorption signature at radio frequencies. This feature arises as Lyman-$\alpha$ photons emitted by these first luminous…

宇宙学与河外天体物理 · 物理学 2020-01-15 Peter H. Sims , Jonathan C. Pober

The EDGES experiment recently announced evidence for a broad absorption feature in the sky-averaged radio spectrum around 78 MHz, as may result from absorption in the 21 cm line by neutral hydrogen at z~15-20. If confirmed, one implication…

宇宙学与河外天体物理 · 物理学 2018-07-18 Adam Lidz , Lam Hui

The Experiment to Detect the Global Epoch of Reionization Signature (EDGES) collaboration has reported the detection of an absorption feature in the sky-averaged spectrum at $\approx 78$ MHz. This signal has been interpreted as the…

宇宙学与河外天体物理 · 物理学 2018-08-27 J. Colin Hill , Eric J. Baxter

The EDGES Collaboration has reported an anomalously strong 21cm absorption feature corresponding to the era of first star formation, which may indirectly betray the influence of dark matter during this epoch. We demonstrate that, by virtue…

高能物理 - 唯象学 · 物理学 2018-09-19 Nick Houston , Chuang Li , Tianjun Li , Qiaoli Yang , Xin Zhang

The EDGES Collaboration has recently announced the detection of the 21-cm spectrum with an absorption profile centred at $78$ megahertz, of which the depth is deeper than that expected by the standard cosmological paradigm. To enrich the…

宇宙学与河外天体物理 · 物理学 2018-12-03 Chunlong Li , Yi-Fu Cai

The EDGES Collaboration has recently reported the detection of a stronger-than-expected absorption feature in the global 21-cm spectrum, centered at a frequency corresponding to a redshift of z ~ 17. This observation has been interpreted as…

高能物理 - 唯象学 · 物理学 2018-07-11 Asher Berlin , Dan Hooper , Gordan Krnjaic , Samuel D. McDermott

The EDGES collaboration reported the finding of an unexpectedly deep absorption in the radio background at 78 MHz and interpreted the dip as a first detection of redshifted 21-cm from Cosmic Dawn. We have attempted an alternate analysis,…

宇宙学与河外天体物理 · 物理学 2019-07-31 Saurabh Singh , Ravi Subrahmanyan

It is predicted that the spectrum of radio emission from the whole sky should show a dip arising from the action of the light from the first stars on the hydrogen atoms in the surrounding gas, which causes the 21-cm line to appear in…

宇宙学与河外天体物理 · 物理学 2020-01-27 Richard Hills , Girish Kulkarni , P. Daniel Meerburg , Ewald Puchwein

The absorption feature in the global spectrum is likely the first 21 cm observable from the cosmic dawn, which provides valuable insights into the earliest history of structure formation. We run a set of high-resolution hydrodynamic…

宇宙学与河外天体物理 · 物理学 2021-12-23 Yidong Xu , Bin Yue , Xuelei Chen

The recent detection of an anomalously strong 21-cm signal of neutral hydrogen from Cosmic Dawn by the EDGES Low-Band radio experiment can be explained if cold dark matter particles scattered off the baryons draining excess energy from the…

宇宙学与河外天体物理 · 物理学 2018-07-11 Anastasia Fialkov , Rennan Barkana , Aviad Cohen

The EDGES experiment has detected the global absorption signal of 21 cm line at $z\sim17$ in cosmic dawn era and reported its amplitude larger than the standard cosmological prediction. One of the possible explanation requires that the…

宇宙学与河外天体物理 · 物理学 2019-10-02 Jitesh R. Bhatt , Arvind Kumar Mishra , Alekha C. Nayak

The dark ages 21-cm signal is a powerful tool for precision cosmology and probing new physics. We study two non-standard models: an excess radio background (ERB) model (possibly generated by dark matter decay) and the millicharged dark…

宇宙学与河外天体物理 · 物理学 2023-11-09 Rajesh Mondal , Rennan Barkana , Anastasia Fialkov

The unexpectedly strong 21cm absorption signal detected by the EDGES experiment suggests that the baryonic gas was colder at redshift $z\sim 17$ than predicted in the standard scenario. We discuss a mechanism to lower the baryon temperature…

高能物理 - 唯象学 · 物理学 2018-04-03 Adam Falkowski , Kalliopi Petraki

The tentative detection by the EDGES experiment of a global 21-cm absorption trough centered at redshift 17 opens up the opportunity to study the birth of the first luminous sources, the intensity of radiation backgrounds at cosmic dawn,…

宇宙学与河外天体物理 · 物理学 2018-07-18 Piero Madau

Recently the EDGES experiment has claimed the detection of an absorption feature centered at 78 MHz. When interpreted as a signature of cosmic dawn, this feature appears at the correct wavelength (corresponding to a redshift range of…

高能天体物理现象 · 物理学 2018-08-15 Prateek Sharma

The recent tentative detection by the EDGES Low-Band antenna of the hydrogen 21-cm line from cosmic dawn, if confirmed, is the first ever signature observed from the epoch of primordial star formation. However, the magnitude and the shape…

宇宙学与河外天体物理 · 物理学 2019-04-24 Anastasia Fialkov , Rennan Barkana

The recently announced result by EDGES points an unexpected excess in the 21 cm global brightness temperature from cosmic dawn at $z\sim 17$, potentially indicating new phenomena beyond the $\Lambda$CDM model. A generic cosmological model…

宇宙学与河外天体物理 · 物理学 2019-02-06 Linfeng Xiao , Rui An , Le Zhang , Bin Yue , Yidong Xu , Bin Wang
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