Relevant bibliographies by topics / Xenon136

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Book chapters
  4. Conference papers

Academic literature on the topic 'Xenon136'

Author: Grafiati
Published: 4 June 2021
Last updated: 10 February 2022

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'Xenon136.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "Xenon136"

1

Davide, Ferella Alfredo. "Direct WIMP searches with XENON100 and XENON1T." EPJ Web of Conferences 95 (2015): 04019. http://dx.doi.org/10.1051/epjconf/20159504019.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Alfonsi, Matteo. "The XENON Dark Matter project: from XENON100 to XENON1T." Nuclear and Particle Physics Proceedings 273-275 (April 2016): 373–77. http://dx.doi.org/10.1016/j.nuclphysbps.2015.09.053.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Fieguth, Alexander. "Search for doubleβ-decays of124Xe with XENON100 & XENON1T". Journal of Physics: Conference Series 888 (вересень 2017): 012251. http://dx.doi.org/10.1088/1742-6596/888/1/012251.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Persiani, Rino. "RESULTS FROM THE XENON100 EXPERIMENT." Acta Polytechnica 53, A (2013): 555–59. http://dx.doi.org/10.14311/ap.2013.53.0555.

Full text
Abstract:
The XENON program consists in operating and developing double-phase time projection chambers using liquid xenon as the target material. It aims to directly detect dark matter in the form of WIMPs via their elastic scattering off xenon nuclei. The current phase is XENON100, located at the Laboratori Nazionali del Gran Sasso (LNGS), with a 62 kg liquid xenon target. We present the 100.9 live days of data, acquired between January and June 2010, with no evidence of dark matter, as well as the new results of the last scientific run, with about 225 live days. The next phase, XENON1T, will increase
APA, Harvard, Vancouver, ISO, and other styles
5

BAO, SHOU-SHAN, XUE GONG, ZONG-GUO SI, and YU-FENG ZHOU. "FOURTH GENERATION MAJORANA NEUTRINO, DARK MATTER AND HIGGS PHYSICS." International Journal of Modern Physics A 29, no. 02 (2014): 1450010. http://dx.doi.org/10.1142/s0217751x14500109.

Full text
Abstract:
We consider extensions of the standard model with fourth generation fermions (SM4) in which extra symmetries are introduced such that the transitions between the fourth generation fermions and the ones in the first three generations are forbidden. In these models, the stringent lower bounds on the masses of fourth generation quarks from direct searches can be relaxed, and the lightest fourth neutrino is allowed to be stable and light enough to trigger the Higgs boson invisible decay. In addition, the fourth Majorana neutrino can be a subdominant but highly detectable dark matter component. We
APA, Harvard, Vancouver, ISO, and other styles
6

Ni, Kaixuan, Jianyang Qi, Evan Shockley, and Yuehuan Wei. "Sensitivity of a Liquid Xenon Detector to Neutrino–Nucleus Coherent Scattering and Neutrino Magnetic Moment from Reactor Neutrinos." Universe 7, no. 3 (2021): 54. http://dx.doi.org/10.3390/universe7030054.

Full text
Abstract:
Liquid xenon is one of the leading targets to search for dark matter via its elastic scattering on nuclei or electrons. Due to their low-threshold and low-background capabilities, liquid xenon detectors can also detect coherent elastic neutrino–nucleus scattering (CEνNS) or neutrino–electron scattering. In this paper, we investigate the feasibility of a compact and movable liquid xenon detector with an active target mass of O(10∼100) kg and single-electron sensitivity to detect CEνNS from anti-neutrinos from a nuclear reactor. Assuming a single- and few-electron background rate at the level ac
APA, Harvard, Vancouver, ISO, and other styles
7

Lang, Rafael F. "Status of XENON100." Journal of Physics: Conference Series 375, no. 1 (2012): 012001. http://dx.doi.org/10.1088/1742-6596/375/1/012001.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Di Gangi, Pietro. "The Xenon Road to Direct Detection of Dark Matter at LNGS: The XENON Project." Universe 7, no. 8 (2021): 313. http://dx.doi.org/10.3390/universe7080313.

Full text
Abstract:
Dark matter is a milestone in the understanding of the Universe and a portal to the discovery of new physics beyond the Standard Model of particles. The direct search for dark matter has become one of the most active fields of experimental physics in the last few decades. Liquid Xenon (LXe) detectors demonstrated the highest sensitivities to the main dark matter candidates (Weakly Interactive Massive Particles, WIMP). The experiments of the XENON project, located in the underground INFN Laboratori Nazionali del Gran Sasso (LNGS) in Italy, are leading the field thanks to the dual-phase LXe time
APA, Harvard, Vancouver, ISO, and other styles
9

Schumann, Marc. "XENON100 – Results and Prospects." Journal of Physics: Conference Series 309 (August 10, 2011): 012011. http://dx.doi.org/10.1088/1742-6596/309/1/012011.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Aprile, E., K. Arisaka, F. Arneodo, et al. "The XENON100 dark matter experiment." Astroparticle Physics 35, no. 9 (2012): 573–90. http://dx.doi.org/10.1016/j.astropartphys.2012.01.003.

Full text
APA, Harvard, Vancouver, ISO, and other styles
More sources

Dissertations / Theses on the topic "Xenon136"

1

Levy, Cecilia [Verfasser], and Christian [Akademischer Betreuer] Weinheimer. "Light propagation and reflection off teflon in liquid xenon detectors for the XENON100 and XENON1T dark matter experiments / Cecilia Levy ; Betreuer: Christian Weinheimer." Münster : Universitäts- und Landesbibliothek Münster, 2014. http://d-nb.info/113828226X/34.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Rauch, Franz Ludwig [Verfasser], and Undagoitia Teresa [Akademischer Betreuer] Marrodan. "From Final Dark Matter Results and Background Shape Uncertainties in XENON100 to First Light in XENON1T / Franz Ludwig Rauch ; Betreuer: Teresa Marrodan Undagoitia." Heidelberg : Universitätsbibliothek Heidelberg, 2017. http://d-nb.info/1178008754/34.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Micheneau, Kévin. "Etude des électrons résiduels dans XENON100." Thesis, Nantes, 2018. http://www.theses.fr/2018NANT4036/document.

Full text
Abstract:
Plusieurs phénomènes gravitationnels indiquent la présence d’une matière non lumineuse, appelée matière noire. Cette dernière est responsable d’environ un quart du budget énergétique total de l’univers. L’un des candidats pressentis pour décrire la matière noire est le WIMP. Pour révéler cette particule par détection directe, la collaboration XENON a développé une chambre à projection temporelle (TPC) à deux phases de xénon : liquide et gazeux. Lorsqu’une particule interagit avec le détecteur XENON100, celle-ci va exciter et ioniser les atomes de xénon. Les photons libérés par la relaxation de
APA, Harvard, Vancouver, ISO, and other styles
4

Toschi, Francesco. "Study of the electronic recoil background of the XENON1T experiment." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2018. http://amslaurea.unibo.it/15785/.

Full text
Abstract:
Uno dei principali protagonisti della caccia alla Materia Oscura è il Progetto XENON presso i LNGS, con l'obiettivo di rivelare le WIMP. Forti dell'esperienza proveniente dalle precedenti fasi del Progetto, l'attuale esperimento XENON1T è il primo che contiene circa 3.2 t di xenon liquido, di cui circa 2 t costituiscono la massa attiva della TPC a doppia fase. E questa è la prima TPC con massa attiva superiore a 1 t e con il più basso livello di fondo tra tutti gli esperimenti di questo tipo. Nel 2017, con un tempo di esposizione di soli 34.2 giorni, XENON1T ha ottenuto uno dei miglior limit
APA, Harvard, Vancouver, ISO, and other styles
5

Geis, Christopher Werner [Verfasser]. "The XENON1T water Cherenkov muon veto system and commissioning of the XENON1T Dark Matter experiment / Christopher Werner Geis." Mainz : Universitätsbibliothek Mainz, 2018. http://d-nb.info/116644936X/34.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Rossi, Monica. "Studio delle interazioni dei neutroni nell'esperimento xenon1t." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2013. http://amslaurea.unibo.it/6158/.

Full text
Abstract:
La presenza di materia oscura nell'universo venne ipotizzata negli anni '30 a seguito di alcune anomalie nei risultati sperimentali ottenuti in astrofisica e cosmologia. La distribuzione di materia ottenuta non concordava infatti con i dati provenienti dalle osservazioni astronomiche e gli scienziati ipotizzarono l'esistenza di un tipo di materia, denominata appunto materia oscura, che interagisse debolmente con la radiazione elettromagnetica e fosse quindi interamente invisibile ai telescopi, sia che fossero a radiofrequenze che operanti nel campo del visibile o con raggi gamma e X, ma che pr
APA, Harvard, Vancouver, ISO, and other styles
7

Girotti, Paolo. "Simulazione Monte Carlo del muon veto dell'esperimento XENON1T." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/12022/.

Full text
Abstract:
Numerose osservazioni astrofisiche e cosmologiche compiute a partire dagli anni '30 confermano che circa il 26% dell'Universo è costituito da materia oscura. Tale materia ha la particolarità di interagire solo gravitazionalmente e, forse, debolmente: essa si presenta massiva e neutra. Tra le numerose ipotesi avanzate riguardanti la natura della materia oscura una delle più accreditate è quella delle WIMP (Weakly Interacting Massive Particle). Il progetto all'avanguardia nella ricerca diretta delle WIMP è XENON presso i Laboratori Nazionali del Gran Sasso (LNGS). Tale esperimento è basato sul
APA, Harvard, Vancouver, ISO, and other styles
8

Lamblin, Jacob. "XENON100 et MIMAC, des détecteurs à la recherche de matière noire." Habilitation à diriger des recherches, Université de Grenoble, 2013. http://tel.archives-ouvertes.fr/tel-00845580.

Full text
Abstract:
Le document présente la problématique de la détection directe de matière noire dans le cadre des expériences XENON100 et MIMAC. Après une introduction générale sur la matière noire et sur les signaux attendus dans un détecteur terrestre, les deux projets sont passés en revue en se concentrant sur les aspects expérimentaux. L'accent est mis particulièrement sur la caractérisation des performances des détecteurs et sur les bruits de fonds associés.
APA, Harvard, Vancouver, ISO, and other styles
9

Massoli, Fabio Valerio <1987&gt. "The XENON1T experiment: Monte Carlo background estimation and sensitivity curves study." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2015. http://amsdottorato.unibo.it/6776/.

Full text
Abstract:
Despite the scientific achievement of the last decades in the astrophysical and cosmological fields, the majority of the Universe energy content is still unknown. A potential solution to the “missing mass problem” is the existence of dark matter in the form of WIMPs. Due to the very small cross section for WIMP-nuleon interactions, the number of expected events is very limited (about 1 ev/tonne/year), thus requiring detectors with large target mass and low background level. The aim of the XENON1T experiment, the first tonne-scale LXe based detector, is to be sensitive to WIMP-nucleon cross
APA, Harvard, Vancouver, ISO, and other styles
10

Di, Gangi Pietro. "Study of the sensitivity of the XENON1T experiment with the profile likelihood method." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2015. http://amslaurea.unibo.it/8348/.

Full text
Abstract:
Oggi sappiamo che la materia ordinaria rappresenta solo una piccola parte dell'intero contenuto in massa dell'Universo. L'ipotesi dell'esistenza della Materia Oscura, un nuovo tipo di materia che interagisce solo gravitazionalmente e, forse, tramite la forza debole, è stata avvalorata da numerose evidenze su scala sia galattica che cosmologica. Gli sforzi rivolti alla ricerca delle cosiddette WIMPs (Weakly Interacting Massive Particles), il generico nome dato alle particelle di Materia Oscura, si sono moltiplicati nel corso degli ultimi anni. L'esperimento XENON1T, attualmente in costruzione
APA, Harvard, Vancouver, ISO, and other styles
More sources

Book chapters on the topic "Xenon136"

1

Scovell, Paul. "The Xenon100 Detector." In Springer Proceedings in Physics. Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-7241-0_13.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Aprile, Elena. "The Xenon1T Dark Matter Search Experiment." In Springer Proceedings in Physics. Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-7241-0_14.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Li, Tianjun, James A. Maxin, Dimitri V. Nanopoulos, and Joel W. Walker. "Supersymmetric Dark Matter at XENON100 and the LHC: No-Scale $$ \mathcal{F} $$ -SU(5) Stringy Correlations." In Springer Proceedings in Physics. Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-7241-0_4.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Mee, Nicholas. "Most of the Universe is Missing!" In The Cosmic Mystery Tour. Oxford University Press, 2019. http://dx.doi.org/10.1093/oso/9780198831860.003.0009.

Full text
Abstract:
Most of the matter in the universe exists in an unknown form called dark matter. All estimates of the mass of galaxies and galaxy clusters suggest they contain far more matter than is visible to us in the form of stars. Conventional explanations, such as the existence of large quantities of burnt-out stars known as MACHOs or dark gas clouds, have been ruled out. The most popular explanation is that dark matter consists of vast quantities of hypothetical stable particles known as WIMPs that were produced in vast quantities in the very early universe. Many laboratories around the world are searching for signs of these particles. These include the Italian Gran Sasso laboratory running the XENON100 experiment. Some theorists have suggested the evidence for dark matter would disappear if we had a better theory of gravity. Analysis of the Bullet Cluster indicates such proposals will not work.
APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "Xenon136"

1

ALFONSI, MATTEO. "The XENON Dark Matter programme: from XENON100 to XENON1T." In VIII International Workshop on the Dark Side of the Universe. Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.161.0047.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

SCHUMANN, Marc. "First Results of XENON100." In Identification of Dark Matter 2010. Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.110.0029.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Tziaferi, E., Jean-Michel Alimi, and André Fuözfa. "The XENON100 Dark Matter Experiment." In INVISIBLE UNIVERSE: Proceedings of the Conference. AIP, 2010. http://dx.doi.org/10.1063/1.3462671.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Schumann, Marc, and Marvin L. Marshak. "The XENON100 Dark Matter Experiment." In 10TH CONFERENCE ON THE INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS. AIP, 2009. http://dx.doi.org/10.1063/1.3293798.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Aprile, Elena, and Shaaban Khalil. "The XENON100 Dark Matter Experiment." In THE DARK SIDE OF THE UNIVERSE: 4th International Workshop on the Dark Side of the Universe. AIP, 2009. http://dx.doi.org/10.1063/1.3131526.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Ferella, Alfredo D. "Status of the XENON100 experiment for WIMP direct detection." In European Physical Society Europhysics Conference on High Energy Physics. Sissa Medialab, 2010. http://dx.doi.org/10.22323/1.084.0093.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Weber, Marc. "A Study of Radon Background in the XENON100 Experiment." In TOPICAL WORKSHOP ON LOW RADIOACTIVITY TECHNIQUES: LRT-2010. AIP, 2011. http://dx.doi.org/10.1063/1.3579583.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Aprile, Elena, Pyungwon Ko, and Deog Ki Hong. "The Search for Dark Matter with the XENON100 Experiment." In SUPERSYMMETRY AND THE UNIFICATION OF FUNDAMENTAL INTERACTIONS. AIP, 2008. http://dx.doi.org/10.1063/1.3052018.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

BAUDIS, Laura. "WIMP Searches with Liquid Xenon: the XENON10 Experiment." In International Europhysics Conference on High Energy Physics. Sissa Medialab, 2007. http://dx.doi.org/10.22323/1.021.0006.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Selvi, Marco. "XENON1T results from 1 tonne×year WIMP search." In Neutrino Oscillation Workshop. Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.337.0094.

Full text
APA, Harvard, Vancouver, ISO, and other styles
You might also be interested in the extended bibliographies on the topic 'Xenon136' for particular source types:
Journal articles Dissertations / Theses
We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!

To the bibliography