The Israel Physical Society
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2020 IPS Conference
Study Materials
Corporate Members
Home
About/Contact
Newsletters
Events/Seminars
2020 IPS Conference
Study Materials
Corporate Members
Lecture Time | Speaker | Lecture subject |
---|---|---|
16:00-16:11 | Anna Ivina |
Search for a light charged Higgs boson in t\rightarrow H^{+}b decays, with H^{+}\rightarrow c\bar{b} in the lepton+jet final state in pp collisions at \sqrt{s}=13 TeV with the ATLAS detector A search for a light charged Higgs boson in t→H^{+}b decays with H^{+} decay to c\bar{b} is presented. |
16:11-16:22 | Yoav Afik |
Searching for New Physics with $b\bar{b} \ell^+ \ell^-$ Contact Interactions We study the impact of contact interactions involving two leptons (electrons or muons) and two $b$-quarks ($b \bar{b} \e... |
16:22-16:33 | Tao Xu |
Displaced Lepton Jet Signatures from Self-Interacting Dark Matter Bound States We study self-interacting dark matte |
16:33-16:44 | Nadav Tamir |
Boosted Di-Taus in ATLAS Many BSM scenarios predict the existance of new particles that couple to the third-generation fermions, and some can lea... |
16:44-16:55 | Guy Koren |
Search for the SM Higgs boson decay to a pair of charm quarks with the ATLAS detector I will present a search for the SM Higgs boson produced in association with a vector boson, and decaying into a pair of... |
16:55-17:06 | Maria Josefina Alconada Verzini |
Search for very low mass resonances in the $\gamma\gamma$ channel with the ATLAS experiment Current searches for resonances in the $\gamma\gamma$ channel, show an unexplored region below 65 GeV in the mass spectr... |
17:06-17:17 | Oz Davidi [1] |
Searching for a Solar Relaxion or Scalar Particle with XENON1T and LUX We consider liquid xenon dark matter detectors for searching a light scalar particle produced in the solar core, specifi... |
17:17-17:28 | Micha Weiss |
XENONnT - increasing the sensitivity of LXe detectors for dark matter XENON1T is the most sensitive WIMP-like dark matter detector in the world, with sensitivity reaching the scale of 10^-47... |