Elena Aprile

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Elena Aprile
ProfessorElenaAprile.jpg
Born (1954-03-12) March 12, 1954 (age 69)
Milan, Italy
Alma mater University of Naples
University of Geneva
Known for XENON Dark Matter Search
Scientific career
Fields Physics
Institutions Columbia University
Doctoral students Reshmi Mukherjee

Elena Aprile (born March 12, 1954) is an Italian-American experimental particle physicist. She has been a professor of physics at Columbia University since 1986. She is the founder and spokesperson of the XENON Dark Matter Experiment. Aprile is well known for her work with noble liquid detectors and for her contributions to particle astrophysics in the search for dark matter. [1] [2]

Contents

Education and academic career

Aprile studied physics at the University of Naples and completed her masters thesis at CERN under the supervision of Professor Carlo Rubbia. [3] After receiving her Laurea degree in 1978, she enrolled at the University of Geneva, from which she received her Ph.D. in physics in 1982. She moved to Harvard University in 1983 as a postdoctoral researcher in Carlo Rubbia's group. Aprile joined the faculty of Columbia University in 1986, [3] attaining her full professorship in 2001. From 2003 to 2009, Aprile served as co-director of the Columbia Astrophysics Laboratory.

Research

Aprile is a specialist in noble liquid detectors and their application in particle physics and astrophysics. [4] She began working on liquid argon detectors as a graduate student at CERN, continuing her research as a postdoctoral fellow at Harvard. At Columbia she investigated the properties of noble liquids for radiation spectroscopy and imaging in astrophysics. [5] This work led to the realization of the first liquid xenon time projection chamber (LXeTPC) as a Compton telescope for MeV gamma rays.

From 1996 to 2001, Aprile was spokesperson of the NASA-sponsored Liquid Xenon Gamma-Ray Imaging Telescope (LXeGRIT) project, leading the first engineering test of the telescope in a near-space environment and subsequent science campaigns with long-duration balloon flights. LXeGRIT used a liquid xenon time projection chamber as a Compton telescope for imaging cosmic sources in the 0.15 to 10 MeV energy band. A total of about 36 hours of data were gathered from two long-duration flights in 1999 and 2000, at an average altitude of 39 km. [6] [7] [8]

Since 2001, Aprile's research focus shifted to particle astrophysics, specifically to direct detection of dark matter with liquid xenon. [9] Aprile is the founder and spokesperson of the XENON dark matter experiment, which aims to discover WIMPs as they scatter off xenon atoms in massive yet ultra-low background [10] liquid xenon detectors operated deep underground. [11]

Awards

Related Research Articles

<span class="mw-page-title-main">Dark matter</span> Hypothetical form of matter

Dark matter is a hypothetical form of matter thought to be the predominant type of matter in the universe. It is called "dark" because it does not appear to interact with the electromagnetic field, which means it does not absorb, reflect, or emit electromagnetic radiation and is, therefore, difficult to detect. Its existence is implied by various astrophysical observations which cannot be explained by general relativity unless more matter is present than can be seen. Evidence for dark matter comes from many different angles, such as galaxy dynamics and formation, gravitational lensing, and the cosmic microwave background, along with astronomical observations of the observable universe's current structure, the formation and evolution of galaxies, mass location during galactic collisions, and the motion of galaxies within galaxy clusters. In the standard Lambda-CDM model of cosmology, the mass–energy content of the universe is 5% ordinary matter, 26.8% dark matter, and 68.2% a form of energy known as dark energy. Thus, dark matter constitutes 85% of the total mass, while dark energy and dark matter constitute 95% of the total mass–energy content.

Weakly interacting massive particles (WIMPs) are hypothetical particles that are one of the proposed candidates for dark matter.

An axion is a hypothetical elementary particle originally postulated by the Peccei–Quinn theory in 1977 to resolve the strong CP problem in quantum chromodynamics (QCD). If axions exist and have low mass within a specific range, they are of interest as a possible component of cold dark matter.

The XENON dark matter research project, operated at the Italian Gran Sasso National Laboratory, is a deep underground detector facility featuring increasingly ambitious experiments aiming to detect hypothetical dark matter particles. The experiments aim to detect particles in the form of weakly interacting massive particles (WIMPs) by looking for rare nuclear recoil interactions in a liquid xenon target chamber. The current detector consists of a dual phase time projection chamber (TPC).

The ArDM Experiment was a particle physics experiment based on a liquid argon detector, aiming at measuring signals from WIMPs, which may constitute the Dark Matter in the universe. Elastic scattering of WIMPs from argon nuclei is measurable by observing free electrons from ionization and photons from scintillation, which are produced by the recoiling nucleus interacting with neighbouring atoms. The ionization and scintillation signals can be measured with dedicated readout techniques, which constituted a fundamental part of the detector.

<span class="mw-page-title-main">Katherine Freese</span> American astrophysicist

Katherine Freese is a theoretical astrophysicist. She is currently a professor of physics at the University of Texas at Austin, where she holds the Jeff and Gail Kodosky Endowed Chair in Physics. She is known for her work in theoretical cosmology at the interface of particle physics and astrophysics.

<span class="mw-page-title-main">Large Underground Xenon experiment</span>

The Large Underground Xenon experiment (LUX) aimed to directly detect weakly interacting massive particle (WIMP) dark matter interactions with ordinary matter on Earth. Despite the wealth of (gravitational) evidence supporting the existence of non-baryonic dark matter in the Universe, dark matter particles in our galaxy have never been directly detected in an experiment. LUX utilized a 370 kg liquid xenon detection mass in a time-projection chamber (TPC) to identify individual particle interactions, searching for faint dark matter interactions with unprecedented sensitivity.

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<span class="mw-page-title-main">ZEPLIN-III</span> 2006–2011 dark matter experiment in England

The ZEPLIN-III dark matter experiment attempted to detect galactic WIMPs using a 12 kg liquid xenon target. It operated from 2006 to 2011 at the Boulby Underground Laboratory in Loftus, North Yorkshire. This was the last in a series of xenon-based experiments in the ZEPLIN programme pursued originally by the UK Dark Matter Collaboration (UKDMC). The ZEPLIN-III project was led by Imperial College London and also included the Rutherford Appleton Laboratory and the University of Edinburgh in the UK, as well as LIP-Coimbra in Portugal and ITEP-Moscow in Russia. It ruled out cross-sections for elastic scattering of WIMPs off nucleons above 3.9 × 10−8 pb from the two science runs conducted at Boulby.

The Particle and Astrophysical Xenon Detector, or PandaX, is a dark matter detection experiment at China Jinping Underground Laboratory (CJPL) in Sichuan, China. The experiment occupies the deepest underground laboratory in the world, and is among the largest of its kind.

The Cryogenic Low-Energy Astrophysics with Noble liquids (CLEAN) experiment by the DEAP/CLEAN collaboration is searching for dark matter using noble gases at the SNOLAB underground facility. CLEAN has studied neon and argon in the MicroCLEAN prototype, and running the MiniCLEAN detector to test a multi-ton design.

<span class="mw-page-title-main">LZ experiment</span> Experiment in South Dakota, United States

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]

Kerstin Perez is an Associate Professor of Particle Physics at the Massachusetts Institute of Technology. She is interested in physics beyond the standard model. She leads the silicon detector program for the General AntiParticle Spectrometer (GAPS) and the high-energy X-ray analysis community for the NuSTAR telescope array.

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References

  1. Kolata, Gina (2011-06-06). "Women Atop Their Fields Dissect the Scientific Life". The New York Times. New York.
  2. "Discover Interview: The Dark Hunter".
  3. 1 2 Nathaniel Herzberg (2017-05-29). "Elena Aprile, la chasseuse de matière noire". Le Monde (in French). Retrieved 2017-05-29.
  4. E. Aprile, A. E. Bolotnikov, A. I. Bolozdynya, T. Doke: Noble Gas Detectors. Wiley 2006.
  5. Aprile, E.; Doke, T. (2010). "Liquid xenon detectors for particle physics and astrophysics". Reviews of Modern Physics. 82 (3): 2053–2097. arXiv: 0910.4956 . Bibcode:2010RvMP...82.2053A. doi:10.1103/RevModPhys.82.2053. S2CID   118576462.
  6. Aprile, E.; et al. (2004). "Calibration and in-flight performance of the Compton telescope prototype LXeGRIT". New Astronomy Reviews. 48 (1–4): 257–262. Bibcode:2004NewAR..48..257A. doi:10.1016/j.newar.2003.11.053.
  7. Aprile, E.; Curioni, A.; Giboni, K.-L.; Kobayashi, M.; Ni, K.; Oberlack, U.G. (2003). "A New Light Readout System for the LXeGRIT Time Projection Chamber" (PDF). IEEE Transactions on Nuclear Science. 50 (5): 1303–1308. Bibcode:2003ITNS...50.1303A. doi:10.1109/TNS.2003.818235.
  8. "LXeGRIT - A Liquid Xenon Gamma-Ray Imaging Telescope". 2002-10-22. Retrieved 2015-02-12.
  9. Aprile, E.; et al. (2006). "Simultaneous Measurement of Ionization and Scintillation from Nuclear Recoils in Liquid Xenon for a Dark Matter Experiment". Physical Review Letters. 97 (8): 081302. arXiv: astro-ph/0601552 . Bibcode:2006PhRvL..97h1302A. doi:10.1103/PhysRevLett.97.081302. PMID   17026288. S2CID   2974093.
  10. Aprile, E.; et al. (XENON100 Collaboration) (2011). "Study of the electromagnetic background in the XENON100 experiment". Physical Review D. 83 (82001): 082001. arXiv: 1101.3866 . Bibcode:2011PhRvD..83h2001A. doi:10.1103/physrevd.83.082001. S2CID   85451637.
  11. Aprile, E.; et al. (2005). "The XENON dark matter search experiment". New Astronomy Reviews. 49 (2–6): 289–295. arXiv: astro-ph/0407575 . Bibcode:2005NewAR..49..289A. doi:10.1016/j.newar.2005.01.035. S2CID   18045108.
  12. "Ufficiale Ordine al Merito della Repubblica Italiana" (in Italian). 2015. Archived from the original on 2015-03-16.
  13. "268686 Elenaaprile (2006 GW)". Minor Planet Center. Retrieved 5 September 2019.
  14. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 5 September 2019.
  15. "Elena Aprile of XENON1T to Receive 2019 Berkeley Prize". AAS – American Astronomical Society. 18 June 2018. Retrieved 5 September 2019.
  16. "UC San Diego Announces Margaret Burbidge Visiting Professorship". ucsdnews.ucsd.edu. Retrieved 2020-03-05.
  17. "New members". American Academy of Arts and Sciences. 2020. Retrieved 2020-09-27.