Yun Wang

Yun Wang (an haife ta shekara ta 1964) mawakiyace kuma masanin ilimin sararin samaniya. Ta fito ne daga Gaoping, wani karamin gari kusa da Zunyi, a Lardin Guizhou, a kasar Sin .

Mawallafi kuma masanin ilimin sararin samaniya Yun Wang .

Ayyukan kwararru a cikin astrophysics

Yun Wang ta sami digiri na farko a fannin kimiyyar lissafi daga Jami'ar Tsinghua da ke Beijing, bayan haka ta zo Amurka kuma ta sami digiri da digiri (kuma a fannin lissafi) daga Jami'a ta Carnegie Mellon . Babban masanin kimiyya a Cibiyar Fasaha ta California tun 2015, kuma farfesa a sashen kimiyyar lissafi da astronomy na Jami'ar Oklahoma har zuwa 2017, ta wallafa takardu sama da 100, kwanan nan ta ƙware kan binciken makamashi mai duhu a sararin samaniya, tare da kulawa ta musamman ga amfani da supernovae da binciken redshift na galaxy a matsayin binciken cosmological, nazarin bayanan microwave, da ma'aunin cosmological.

Yun Wang ta ɓullo da dabarun don inganta bincike na gaba don bincikar makamashi mai duhu, kuma ya ƙirƙira manufar manufa don NASA-DOE Joint Dark Energy Mission (JDEM), da Haɗin gwiwar Ingancin duhu-makamashi (JEDI), kuma ya zama babban mai binciken JEDI.  Manufar manufa ta JEDI/JDEM tana misalta ingantaccen ingantaccen aiki ta hanyar sabbin kayan aiki, da manyan fa'idodin kimiyya na haɗa hanyoyin lura masu zaman kansu guda uku (tarin galaxy, lensing mai rauni, da supernovae) don bincika kuzarin duhu.  JEDI ya yi tasiri sosai kan ƙirar ayyukan sararin samaniya don bincika makamashi mai duhu..

An zabi Yun Wang a matsayin Fellow na American Physical Society a cikin shekara ta 2012, tare da ambaton: "Domin jagorancinta a cikin binciken makamashi mai duhu, musamman a cikin haɓaka tsari mai ƙarfi da daidaituwa don nazarin da fassara bayanan sararin samaniya don sanya ƙuntatawa masu zaman kansu akan makamashi na duhu, da kuma inganta dawowar kimiyya na ayyukan sararin samaniya da aka tsara don bincika makamashi masu duhu" (daga http://www.aps.org/programs/fellowships/archive-all.cfm?initi=2012&Punit_id)

Yun Wang shine wanda ya kafa Ofishin Jakadancin Euclid na ESA, wanda aka kaddamar a ranar 1 ga Yuli, 2023. Ta jagoranci daya daga cikin manyan kungiyoyin kimiyya guda biyu na Euclid Consortium, Euclid Galaxy Clustering Science Working Group. Wang ya jagoranci kimiyyar tarin taurari don NASA's Nancy Grace Roman Space Telescope, tare da ƙaddamarwa da ake sa ran a watan Oktoba 2026. Roman yana da haɗin kai sosai tare da Euclid wajen haskaka asirin sararin samaniya mai duhu, duba https://www.jpl.nasa.gov/news/nasas-roman-and-esas-euclid-will-team-up-to-investigate-dark-energy.

Yun Wang shine PI na ATLAS Probe, manufa don aikin bincike-aji na NASA.  ATLAS Probe zai ta tsara taswirar sararin yanar gizo na duhun kwayoyin halitta, kuma zai warware ilimin lissafi na juyin halittar galaxy.  Hakanan zai samar da tabbataccen ma'auni akan makamashi mai duhu, bincika yankuna masu ƙura na Hanyar Milky Way, da bincika tarihin samuwar Tsarin Rana na Wuta.  Yun Wang kuma shine PI na manufa ta sararin samaniya ISCEA (Infrared SmallSat don Cluster Evolution Astrophysics), wanda NASA ta zaba a cikin Satumba 2018 don nazarin ra'ayi na manufa..

Wiley ne ya buga littafinta na fasaha "Dark Energy" ( ) a cikin shekara ta 2010.ISBN 978-3-527-40941-9

Takardun da ta fi ambaton kwanan nan guda shida sune:

• Wang, Yun; Mukherjee, P (Oktoba 2006). "Ƙuntatawa na Dark Energy daga Supernovae, Galaxy Clustering, da kuma Wilkinson Microwave Anisotropy Probe Observations na Shekaru Uku". Jaridar Astrophysical. 650 (1): 1–6. arXiv:astro-ph/0604051. Bibcode: 2006ApJ... 650.... 1W. [Hotuna a shafi na 106]507091. S2CID 847741. (Lokacin da aka ambata: 328) Wang, Yun; Mukherjee, P (October 2006). "Robust Dark Energy Constraints from Supernovae, Galaxy Clustering, and Three-Year Wilkinson Microwave Anisotropy Probe Observations". Astrophysical Journal. 650 (1): 1–6. arXiv:astro-ph/0604051. Bibcode:2006ApJ...650....1W. doi:10.1086/507091. S2CID 847741.
• (Lokacin da aka ambata: 285) Wang, Yun; Mukherjee, P (Nov 2007). "Observational constraints on dark energy and cosmic curvature". Physical Review. D76 (10): 103533–63. arXiv:astro-ph/0703780. Bibcode:2007PhRvD..76j3533W. doi:10.1103/PhysRevD.76.103533. S2CID 119093990.
• (Lokacin da aka ambata: 276) Wang, Yun; Tegmark, M (June 2004). "New dark energy constraints from supernovae, microwave background, and galaxy clustering". Physical Review Letters. 92 (24): 241302. arXiv:astro-ph/0403292. Bibcode:2004PhRvL..92x1302W. doi:10.1103/PhysRevLett.92.241302. PMID 15245074. S2CID 22090047.
• Chuang, Chia-Hsun; Wang, Yun (Oktoba 2013). "Matsayin ma'aunin ma'auni na ma'aikatar ma'auratan ma'aunoni guda ɗaya na H (z), DA (z) da f (z) σ8 (z) daga Sloan Digital Sky Survey DR7 haske ja galaxies". Sanarwar kowane wata na Royal Astronomical Society. 435 (1): 255–262. arXiv:1209.0210. Bibcode: 2013MNRAS. 435. 255C. [Hotuna a shafi na 10] S2CID 119277476. (Lokacin da aka ambata: 258) Chuang, Chia-Hsun; Wang, Yun (October 2013). "Modelling the anisotropic two-point galaxy correlation function on small scales and single-probe measurements of H(z), DA(z) and f(z)σ8(z) from the Sloan Digital Sky Survey DR7 luminous red galaxies". Monthly Notices of the Royal Astronomical Society. 435 (1): 255–262. arXiv:1209.0210. Bibcode:2013MNRAS.435..255C. doi:10.1093/mnras/stt1290. S2CID 119277476.
• Wang, Yun; Mukherjee, P (Mayu 2004). "Ƙuntatawa mai zaman kanta a kan ƙarancin makamashi mai duhu daga ƙididdigar ƙididdiga na nau'in Ia supernova data". Jaridar Astrophysical. 606 (2): 654–63. arXiv:astro-ph/0312192. Bibcode: 2004ApJ... 606.. 654W. [Hotuna a shafi na 1086/383196.] S2CID 119387792. (Lokacin da aka ambata: 203) Wang, Yun; Mukherjee, P (May 2004). "Model-independent constraints on dark energy density from flux-averaging analysis of type Ia supernova data". Astrophysical Journal. 606 (2): 654–63. arXiv:astro-ph/0312192. Bibcode:2004ApJ...606..654W. doi:10.1086/383196. S2CID 119387792.
• (Lokacin da aka ambata:203) Wang, Yun; Tegmark, M (May 2005). "Uncorrelated Measurements of the Cosmic Expansion History and Dark Energy from Supernovae". Physical Review. D71 (10): 103513–63. arXiv:astro-ph/0501351. Bibcode:2005PhRvD..71j3513W. doi:10.1103/PhysRevD.71.103513. S2CID 15503044.

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