Suggestions for future topics:

• arXiv:1409.0492 Is the Standard Model saved asymptotically by conformal symmetry?

• arXiv:1410.6157 UltraViolet freeze-in

• arXiv:1403.6078 Higgs inflation at the critical point

• arXiv:1403.4638 Relic Gravity Waves and 7 keV Dark Matter from a GeV scale inflaton

• arXiv:1411.2162 Differences between axions and generic Light Scalars in lab experiments

• arXiv:1411.5124 Spontaneous radiatively induced breaking of conformal invariance in SM

• arXiv:1411.5633 An upper limit on the scale of new physics phenomena from high multiplicity Higgs and vector boson events

• arXiv:1411.2424 Is the principle of least action a must?

• arXiv:1411.1772 Yukawa Bound States of a Large Number of Fermions

• arXiv:1411.4673 Attempts at determination of \alpha from first principles: An overview

• arXiv:1406.6105 WIMPy baryogenesis with sterile neutrinos and other realizations

• arXiv:1401.6704 Chiral molecule in the standard model

• arXiv:1402.3409 Spectra and drag force of free-streaming neutrinos

• arXiv:1402.3848 Electric charge as magnetic dipole when in magnetic field

• arXiv:1402.3620 Muon g-2, Rare K decays and parity violation from dark bosons

• arXiv:1401.7891 Multiple scales in Pati-Salam models

• arXiv:1312.1772 Quantum tunneling in real time

• arXiv:1309.6894 Optimal number of terms in QED series

• arXiv:1401.5217 A cosmological bound on e^+ - e^- mass difference

• arXiv:1309.2746 How to see an antistar

Previous semesters:
SS 2013
WS 2013/2014
SS 2014