Israeli Joint Particle Physics Meetings, Spring-Summer 2020
from
Wednesday 22 April 2020 (11:00)
to
Wednesday 30 June 2021 (12:00)
Monday 20 April 2020
Tuesday 21 April 2020
Wednesday 22 April 2020
11:00
Supersoft Stops
-
Matthew Philip Mccullough
(
CERN
)
Supersoft Stops
Matthew Philip Mccullough
(
CERN
)
11:00 - 12:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/754833484?pwd=dWVjSjNOYWhFYkRSRDVkVzJ1U29sQT09 Meeting ID: 754 833 484 Password: HEP_Joint
Thursday 23 April 2020
Friday 24 April 2020
Saturday 25 April 2020
Sunday 26 April 2020
Monday 27 April 2020
Tuesday 28 April 2020
Wednesday 29 April 2020
Thursday 30 April 2020
Friday 1 May 2020
Saturday 2 May 2020
Sunday 3 May 2020
Monday 4 May 2020
Tuesday 5 May 2020
Wednesday 6 May 2020
11:00
Charm Physics Confronts High-$p_T$ Lepton Tails
-
Admir Greljo
(
CERN
)
Charm Physics Confronts High-$p_T$ Lepton Tails
Admir Greljo
(
CERN
)
11:00 - 12:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/99512131810?pwd=dS9Ma0JYTVJzajRuME1Wemo0Y3E5dz09 Meeting ID: 995 1213 1810 Password: HEP_Joint
Thursday 7 May 2020
Friday 8 May 2020
Saturday 9 May 2020
Sunday 10 May 2020
Monday 11 May 2020
Tuesday 12 May 2020
Wednesday 13 May 2020
13:00
Optimized CP probes of the top quark Yukawa at hadron colliders
-
Jernej Fesel Kamenik
(
Jozef Stefan Institute (SI)
)
Optimized CP probes of the top quark Yukawa at hadron colliders
Jernej Fesel Kamenik
(
Jozef Stefan Institute (SI)
)
13:00 - 14:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/94720014121?pwd=Vld0NmlINE4xTE5iMkx0SlliOFltdz09 Meeting ID: 947 2001 4121 Password: HEP_Joint
Thursday 14 May 2020
Friday 15 May 2020
Saturday 16 May 2020
Sunday 17 May 2020
Monday 18 May 2020
Tuesday 19 May 2020
Wednesday 20 May 2020
11:00
En$t\bar{t}$anglement detection at the LHC
-
Yoav Afik
(
Technion- Israel Institute of Technology (IL)
)
En$t\bar{t}$anglement detection at the LHC
Yoav Afik
(
Technion- Israel Institute of Technology (IL)
)
11:00 - 12:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/95323835114?pwd=VlZFQzVNQW54TElQUzFJTFM1OGpvUT09 Meeting ID: 953 2383 5114 Password: HEP_Joint
Thursday 21 May 2020
Friday 22 May 2020
Saturday 23 May 2020
Sunday 24 May 2020
Monday 25 May 2020
Tuesday 26 May 2020
Wednesday 27 May 2020
16:00
Gamma-Ray Tests of Elusive Dark Matter Candidates
-
Tracy Slatyer
Gamma-Ray Tests of Elusive Dark Matter Candidates
Tracy Slatyer
16:00 - 17:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/96160656142?pwd=MzlYMUEvVmp0a0RMY2l0RUgyMWFXUT09 Meeting ID: 961 6065 6142 Password: HEP_Joint Abstract: I will discuss the ability of current and future gamma-ray datasets to constrain dark matter candidates that are otherwise very difficult to probe, focusing on the cases of asteroid-mass primordial black holes and thermal winos and higgsinos. I will present new constraints on the PBH mass and DM fraction from INTEGRAL data, briefly outline recent theoretical progress in computing the expected annihilation signals of winos and higgsinos, and show that the upcoming CTA gamma-ray telescope array should still have sensitivity to the thermal higgsino even once a range of systematic uncertainties are taken into account.
Thursday 28 May 2020
Friday 29 May 2020
Saturday 30 May 2020
Sunday 31 May 2020
Monday 1 June 2020
Tuesday 2 June 2020
Wednesday 3 June 2020
16:00
Searching for axion light particles using flavor violating transitions
-
Jure Zupan
(
University of Cincinnati
)
Searching for axion light particles using flavor violating transitions
Jure Zupan
(
University of Cincinnati
)
16:00 - 17:00
Thursday 4 June 2020
Friday 5 June 2020
Saturday 6 June 2020
Sunday 7 June 2020
Monday 8 June 2020
Tuesday 9 June 2020
Wednesday 10 June 2020
Thursday 11 June 2020
Friday 12 June 2020
Saturday 13 June 2020
Sunday 14 June 2020
Monday 15 June 2020
Tuesday 16 June 2020
Wednesday 17 June 2020
11:00
Non-Cold Dark Matter from Primordial Black Hole Evaporation
-
Iason Baldes
(
Universite Libre de Bruxelles
)
Non-Cold Dark Matter from Primordial Black Hole Evaporation
Iason Baldes
(
Universite Libre de Bruxelles
)
11:00 - 12:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/93346299032?pwd=V2JJdmxqM0JkQzBYN2FVS0F4bldjQT09 Meeting ID: 933 4629 9032 Password: HEP_Joint Abstract: Dark matter coupled solely gravitationally can be produced through the decay of primordial black holes in the early universe. If the dark matter is lighter than the initial black hole temperature, it can be warm enough to be subject to structure formation constraints. I will present an overview of this scenario and discuss some recent progress in calculating the structure formation constraint with greater precision. Taking into account the red-shifted phase space of DM particles from the black hole evaporation, we used the Boltzmann code CLASS to determine the corresponding matter power spectrum, which we find to match closely to those of warm dark matter models. This allowed us to rule out the possibility, consistent with analytic estimates, of primordial black holes having come to dominate the energy density of the universe and simultaneously given rise to all the DM through their decay. Consequences and implications for dark radiation and leptogenesis will be briefly discussed.
Thursday 18 June 2020
Friday 19 June 2020
Saturday 20 June 2020
Sunday 21 June 2020
Monday 22 June 2020
Tuesday 23 June 2020
Wednesday 24 June 2020
15:00
A New Mask for An Old Suspect -- Testing the Sensitivity of the Galactic Center Excess to the Point Source Mask
-
Samuel McDermott
A New Mask for An Old Suspect -- Testing the Sensitivity of the Galactic Center Excess to the Point Source Mask
Samuel McDermott
15:00 - 16:00
The talk will be given remotely: Join Zoom Meeting https://huji.zoom.us/j/98293801426?pwd=T3Bpajk5aytmK0dSOUJrb1phdW4xQT09 Meeting ID: 982 9380 1426 Password: HEP_Joint Abstract: The Galactic center excess has lingered as a possible, but ambiguous, signal of new physics for several years. It has previously been argued that certain details of the excess emission imply that it likely originates from a population of point sources, but this remains a topic of vigorous debate. In this talk, I will report on recent work, relying on a new point source catalog (obtained by the Fermi-LAT collaboration), that sheds light on this controversial topic. After giving some background on the excess, I will discuss various metrics that have been used to try to understand its true nature. I will show that the large majority of bright sources that were previously suggested to be members of the excess are indeed contained in the new Fermi-LAT point source catalog -- and yet, despite masking out these sources (so that they cannot contribute to the excess), the excess remains just as bright in our new fit to the data. I will go on to discuss the implications of our findings for the two most popular interpretations of the excess and I will show some preliminary next steps to further clarify the nature of the excess.
Thursday 25 June 2020
Friday 26 June 2020
Saturday 27 June 2020
Sunday 28 June 2020
Monday 29 June 2020
Tuesday 30 June 2020
Wednesday 1 July 2020
11:00
Audible Axions: Probing axion-like particles using gravitational waves
-
Pedro Schwaller
(
Argonne National Laboratory/UIC chicago
)
Audible Axions: Probing axion-like particles using gravitational waves
Pedro Schwaller
(
Argonne National Laboratory/UIC chicago
)
11:00 - 12:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/94690471513?pwd=NXEyeitvaXY5dzYrMExDMnZ1ZXRxUT09 Meeting ID: 946 9047 1513 Password: HEP_Joint Abstract: Gravitational waves offer a new possibility to probe the early universe. After a brief overview, I will focus on the audible axion scenario, in which dynamics of the axion after inflation leads to an observable GW signal with distinct characteristics.
Thursday 2 July 2020
Friday 3 July 2020
Saturday 4 July 2020
Sunday 5 July 2020
Monday 6 July 2020
Tuesday 7 July 2020
Wednesday 8 July 2020
16:00
KOTO vs NA62
-
Kohsaku Tobioka
KOTO vs NA62
Kohsaku Tobioka
16:00 - 17:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/97286428374?pwd=Z2lyb0RKVjJLNE9PaENBMmxpMytIZz09 Meeting ID: 972 8642 8374 Password: HEP_Joint
Thursday 9 July 2020
Friday 10 July 2020
Saturday 11 July 2020
Sunday 12 July 2020
Monday 13 July 2020
Tuesday 14 July 2020
Wednesday 15 July 2020
12:00
ESPP discussion
-
Eliezer Rabinovici
(
The Hebrew University of Jerusalem (IL)
)
Halina Abramowicz
(
Tel Aviv University (IL)
)
Gilad Perez
(
Weizmann
)
ESPP discussion
Eliezer Rabinovici
(
The Hebrew University of Jerusalem (IL)
)
Halina Abramowicz
(
Tel Aviv University (IL)
)
Gilad Perez
(
Weizmann
)
12:00 - 13:15
1. Gilad Perez - brief introduction. 2. Halina Abramowicz - perspective on the output 3. Eliezer Rabinovici - perspective on the process and lessons for the future 4. Halina and Eliezer - addressing questions sent in advance 5. Open discussion
Thursday 16 July 2020
Friday 17 July 2020
Saturday 18 July 2020
Sunday 19 July 2020
Monday 20 July 2020
Tuesday 21 July 2020
Wednesday 22 July 2020
11:00
More Axions from Strings
-
Marco Gorghetto
(
SISSA
)
More Axions from Strings
Marco Gorghetto
(
SISSA
)
11:00 - 12:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/93901756968?pwd=NkRUTnY4N2l4YlFFdXI0aDFDbyswZz09 Meeting ID: 939 0175 6968 Password: HEP_Joint Abstract: The axion solution to the strong CP problem also provides a natural dark matter candidate. If the PQ symmetry has ever been restored after inflation, topological defects of the axion field would have formed and produced relic axions, whose abundance is in principle calculable. We study the contribution to the abundance produced by string defects during the so-called scaling regime. Clear evidence of scaling violations is found, the most conservative extrapolation of which strongly suggests a large number of axions from strings. The overall result is a lower bound on the QCD axion mass in the post-inflationary scenario that is substantially stronger than the naive one from misalignment.
Thursday 23 July 2020
Friday 24 July 2020
Saturday 25 July 2020
Sunday 26 July 2020
Monday 27 July 2020
Tuesday 28 July 2020
Wednesday 29 July 2020
Thursday 30 July 2020
Friday 31 July 2020
Saturday 1 August 2020
Sunday 2 August 2020
Monday 3 August 2020
Tuesday 4 August 2020
Wednesday 5 August 2020
Thursday 6 August 2020
Friday 7 August 2020
Saturday 8 August 2020
Sunday 9 August 2020
Monday 10 August 2020
Tuesday 11 August 2020
Wednesday 12 August 2020
16:00
Nonlinear Isotope Shift in Yb$^+$ Search for Physics beyond the Standard Model
-
Vladan Vuletić
(
MIT
)
Nonlinear Isotope Shift in Yb$^+$ Search for Physics beyond the Standard Model
Vladan Vuletić
(
MIT
)
16:00 - 17:00
The talk will be given remotely: Join Zoom Meeting https://technion.zoom.us/j/99809009276?pwd=MjVZZ0hoRmFvUThnblQzU29FWUhuUT09 Meeting ID: 998 0900 9276 Passcode: HEP_Joint Abstract: Recently it has been proposed to search for particles outside the Standard Model (SM) in an intermediate mass range (100 eV to 100 MeV) by means of precision isotope shift spectroscopy on narrow optical transitions. We perform such measurements on two quadrupole $S \to D$ transitions and one octupole $S \to F$ transition for five bosonic isotopes of Yb$^+$ with an accuracy below 1kHz, and observe nonlinearities in the corresponding King plots. Such a nonlinearity can indicate physics beyond the SM, or higher-order effects within the SM. Our data indicate that there are at least two distinct sources of nonlinearity. We identify the second-order field shift as the leading-order effect within the SM for Yb$^+$, and discuss possibilities for the other source of nonlinearity. In the future, more precise measurements on more transition available for Yb$^+$ and Yb, in combination with improved electronic-structure calculations, can be used to distinguish between effects within and outside the SM.
Thursday 13 August 2020
Friday 14 August 2020
Saturday 15 August 2020
Sunday 16 August 2020
Monday 17 August 2020
Tuesday 18 August 2020
Wednesday 19 August 2020
Thursday 20 August 2020
Friday 21 August 2020
Saturday 22 August 2020
Sunday 23 August 2020
Monday 24 August 2020
Tuesday 25 August 2020
Wednesday 26 August 2020
Thursday 27 August 2020
Friday 28 August 2020
Saturday 29 August 2020
Sunday 30 August 2020
Monday 31 August 2020
Tuesday 1 September 2020
Wednesday 2 September 2020
Thursday 3 September 2020
Friday 4 September 2020
Saturday 5 September 2020
Sunday 6 September 2020
Monday 7 September 2020
Tuesday 8 September 2020
Wednesday 9 September 2020
Thursday 10 September 2020
Friday 11 September 2020
Saturday 12 September 2020
Sunday 13 September 2020
Monday 14 September 2020
Tuesday 15 September 2020
Wednesday 16 September 2020
Thursday 17 September 2020
Friday 18 September 2020
Saturday 19 September 2020
Sunday 20 September 2020
Monday 21 September 2020
Tuesday 22 September 2020
Wednesday 23 September 2020
Thursday 24 September 2020
Friday 25 September 2020
Saturday 26 September 2020
Sunday 27 September 2020
Monday 28 September 2020
Tuesday 29 September 2020
Wednesday 30 September 2020
Thursday 1 October 2020
Friday 2 October 2020
Saturday 3 October 2020
Sunday 4 October 2020
Monday 5 October 2020
Tuesday 6 October 2020
Wednesday 7 October 2020
Thursday 8 October 2020
Friday 9 October 2020
Saturday 10 October 2020
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