GDR Terascale@Palaiseau
→
Europe/Paris
Ecole Polytechnique
Ecole Polytechnique
Route de Saclay, 91128 Palaiseau
Christophe Ochando
(LLR),
Dirk Zerwas
(LAL Orsay),
Gilbert Moultaka
(L2C Montpellier, UMR5221-UM2/INP/CNRS),
Sylvaine Pieyre
(LLR communication)
Description
We are looking forward to welcome you at the LLR, Palaiseau, from June 2 to 4 for the meeting of the GDR Terascale. Please register as soon as possible, the registration deadline is Mai 25, 2014.
Your contribution to the programme is welcome. Please contact the coordinators of the corresponding session if you would like to give a talk:
Higgs: Sandrine Laplace, Christophe Ochando, Pietro Slavich
BSM: Marie-Helene Genest, Stephane Lavignac, Ana Teixeira, Patrice Verdier
Dark Universe: Emmanuel Moulin, Marco Cirelli
Tools: Benjamin Fuks and Nikola Makovec
You can find their e-mail addresses on the Web-page of the GDR Terascale. The GDR will offer the lunches on Monday, Tuesday and Wednesday as well as the dinner on Tuesday evening.
Your contribution to the programme is welcome. Please contact the coordinators of the corresponding session if you would like to give a talk:
Higgs: Sandrine Laplace, Christophe Ochando, Pietro Slavich
BSM: Marie-Helene Genest, Stephane Lavignac, Ana Teixeira, Patrice Verdier
Dark Universe: Emmanuel Moulin, Marco Cirelli
Tools: Benjamin Fuks and Nikola Makovec
You can find their e-mail addresses on the Web-page of the GDR Terascale. The GDR will offer the lunches on Monday, Tuesday and Wednesday as well as the dinner on Tuesday evening.
Participants
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11:00
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14:30
Registration
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14:30
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14:45
WelcomePrésidents de session: Dirk Zerwas (LAL Orsay), Gilbert Moultaka (L2C Montpellier, UMR5221-UM2/INP/CNRS)
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14:45
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15:55
Higgs Amphithéâtre Becquerel
Amphithéâtre Becquerel
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Dr Christophe Ochando (LLR), Dr Pietro Slavich (LPTHE Paris), Mme Sandrine Laplace (LPNHE)- 14:45
- 15:10
- 15:35
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15:55
→
16:25
Coffee Break 30m
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16:25
→
18:00
Higgs Amphithéâtre Becquerel
Amphithéâtre Becquerel
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Dr Christophe Ochando (LLR), Dr Pietro Slavich (LPTHE Paris), Mme Sandrine Laplace (LPNHE)-
16:25
Exotic Higgs decays at the LHC 20mOrateur: M. Adam Falkowski (LPT Orsay)
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16:45
boosted Higgs decays into gamma and a Z in the NMSSM 25mOrateur: Vincent Bizouard (LAPTh)
- 17:10
- 17:30
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16:25
- 18:00 → 20:00
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11:00
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14:30
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09:00
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10:05
Higgs Amphithéâtre Carnot
Amphithéâtre Carnot
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Dr Christophe Ochando (LLR), Dr Pietro Slavich (LPTHE Paris), Mme Sandrine Laplace (LPNHE)- 09:00
- 09:20
- 09:40
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10:05
→
11:05
Methods & Tools Amphithéâtre Carnot
Amphithéâtre Carnot
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Benjamin Fuks (IPHC Strasbourg / CERN), M. Nikola Makovec (LAL Orsay)- 10:05
- 10:35
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11:05
→
11:30
Coffee Break 25m
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11:30
→
12:30
Methods & Tools Amphithéâtre Carnot
Amphithéâtre Carnot
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Benjamin Fuks (IPHC Strasbourg / CERN), M. Nikola Makovec (LAL Orsay)- 11:30
- 12:00
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12:30
→
13:50
Lunch Break 1h 20m Restaurant Magnan
Restaurant Magnan
Ecole Polytechnique
Route de Saclay, 91128 Palaiseau -
13:50
→
14:40
Methods & Tools Amphithéâtre Carnot
Amphithéâtre Carnot
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Benjamin Fuks (IPHC Strasbourg / CERN), M. Nikola Makovec (LAL Orsay)- 13:50
- 14:20
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14:40
→
16:10
BSM Amphithéâtre Carnot
Amphithéâtre Carnot
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Ana M. Teixeira (LPC Clermont), Marie-Hélène Genest (LPSC), Dr Patrice Verdier (IPN Lyon), Dr Stéphane Lavignac (SPhT Saclay)- 14:40
- 15:10
- 15:40
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16:10
→
16:30
Coffee Break 20m
-
16:30
→
18:30
BSM Amphithéâtre Carnot
Amphithéâtre Carnot
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Ana M. Teixeira (LPC Clermont), Marie-Hélène Genest (LPSC), Dr Patrice Verdier (IPN Lyon), Dr Stéphane Lavignac (SPhT Saclay)- 16:30
- 17:00
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17:30
Jet substructure and top tagging to search for new physics 30mOrateur: Dr Pierre-Antoine Delsart (LPSC)
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18:00
Stop searches with boosted tops and transverse variables. 30mOrateur: Dr Dipan Sengupta (LPSC, Grenoble)
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20:30
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23:00
Dinner 2h 30m "La Terrasse du Laurier" in Paris, 145 Boulevard Saint-Michel,RER-B Port-Royal
"La Terrasse du Laurier" in Paris, 145 Boulevard Saint-Michel,RER-B Port-Royal
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09:00
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10:05
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09:00
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10:30
BSM Amphithéâtre Becquerel
Amphithéâtre Becquerel
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Ana M. Teixeira (LPC Clermont), Marie-Hélène Genest (LPSC), Dr Patrice Verdier (IPN Lyon), Dr Stéphane Lavignac (SPhT Saclay)- 09:00
- 09:30
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10:00
Flavoured scalar triplet leptogenesis 30mOrateur: Benoit Schmauch (CEA Scalay)
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10:30
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10:55
Coffee Break 25m
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10:55
→
12:30
Dark Universe Amphithéâtre Becquerel
Amphithéâtre Becquerel
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Dr Emmanuel Moulin (IRFU/SPP), M. Marco CIRELLI (CNRS IPhT Saclay)-
10:55
Mainly axion cold dark matter from natural SUSY 45mBy eschewing fine-tuning from the electroweak and QCD sectors of supersymmetry (natural supersymmetry or SUSY), and by invoking the Kim-Nilles solution to the SUSY mu problem, one is lead to models wherein the dark matter is comprised of a mixture of axions and higgsino-like WIMPs. Over a large range of Peccei-Quinn breaking scale f_a~ 10^9-10^{12} GeV, one then expects about 90-95% axion dark matter. In such a scenario, both axion and WIMP direct detection may be expected.Orateur: Prof. Eung Jin Chun (KIAS Seoul)
- 11:40
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10:55
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12:30
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14:00
Lunch 1h 30m Restaurant Magnan
Restaurant Magnan
Ecole Polytechnique
Route de Saclay, 91128 Palaiseau -
14:00
→
16:00
Dark Universe Amphithéâtre Becquerel
Amphithéâtre Becquerel
Ecole Polytechnique
Route de Saclay, 91128 PalaiseauPrésidents de session: Dr Emmanuel Moulin (IRFU/SPP), M. Marco CIRELLI (CNRS IPhT Saclay)-
14:00
BICEP2 and its implications for cosmology and particle physics 30mIn this talk, after a very brief description of inflation and its predictions for the properties Cosmic Microwave Background radiation, I will discuss the results by the BICEP2 collaboration, that recently claimed detection of the so-called primordial B modes in the CMB. In particular, my talk will focus on the implications that such a detection would have for inflationary model building and for particle physics.Orateur: Dr Lorenzo Sorbo (University of Massachusetts, Amherst)
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14:30
Fitting the Fermi-LAT GeV excess: on the importance of the propagation of electrons from dark matter 30mAn excess of gamma rays at GeV energies has been detected in the Fermi-LAT data. This signal comes from a narrow region around the Galactic Center and has been interpreted as possible evidence for light (30 GeV) dark matter particles. Focussing on the prompt gamma-ray emission, previous work found that the best fit to the data corresponds to annihilations proceeding into b quarks, with a dark matter profile ~ r^{-1.2}. In this talk, I will show that this is not the only possible annihilation set-up. More specifically, I will show how including the contributions to the gamma-ray spectrum from inverse Compton scattering and bremsstrahlung from electrons produced in dark matter annihilations, and undergoing diffusion through the Galactic magnetic field, modifies the spectrum, in particular for leptonic final states.Orateur: Thomas Lacroix
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15:00
DM with supersymmetric triplets 30mThe Triplet extension of the MSSM (TMSSM) alleviates the little hierarchy problem and provides a significant enhancement of the loop-induced diphoton rate of the lightest CP-even Higgs h. In this I will present the first computation of the h into Z + gamma decay. I will show that the rates of loop-induced decays are correlated and their signal strengths can rise up to 40% - 60% depending on the channel. I will furthermore study the dark matter phenomenology of the TMSSM. The lightest neutralino is a good dark matter candidate in two regions. The first one is related to the Higgs and Z resonances and the LSP is mostly Bino. The second one is achieved for a mass larger than 90 GeV and the LSP behaves as the well-tempered neutralino. An advantage of the triplet contribution is that the well-tempered neutralino can be a Bino-Triplino mixture, relieving the problem of achieving M_2 ~ M_1 in unified scenarios. The dark matter constraints strongly affect the Higgs phenomenology, reducing the potential enhancements of the diphoton and of the Z + photon channels by 20% at most. In the near future, complementarity of dark matter direct searches and collider experiments will be crucial to probe most of the parameter space where the neutralino is the dark matter candidate.Orateur: Dr Chiara Arina (IAP)
- 15:30
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14:00
- 16:00 → 16:10
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09:00
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10:30