KOLOKIUM FISIKA “Generation of particle number asymmetry from interacting scalars”

🔖 PEMATERI:

Apriadi Salim Adam, Sc.D
Pusat Penelitian Fisika Teori Energi Tinggi
Pusat Penelitian Fisika LIPI

🗒 KAPAN?

17 Maret 2021 (Rabu)
10.00-11.30 WIB

🏡 DI MANA?

Zoom Meeting LIPI Physics:
Meeting ID : 994 5135 8455
Passcode : 039636

https://zoom.us/j/99451358455?pwd=S2pUNVlyZUg1MW15Rm5QMDQrRWNOUT09

📌 Kapasitas ruangan virtual Zoom terbatas bagi 100 pendaftar.

📌 Kolokium disiarkan pula secara TERBUKA melalui Live FB @lipiphysics (silakan manfaatkan bagi yang tidak berhasil mendaftar melalui Zoom)

📒 ABSTRAK:

The origin of the asymmetry of the universe is the one of unresolved problem of the fundamental physics in both cosmology and particle physics. From the standard model point of view, it is insufficient to accommodate such a problem. Therefore, this indicates a need to extend the standard model.
In this work, we develop a mechanism to generate particle number asymmetry (PNA) which is realized with a Lagrangian including a complex scalar field and a neutral scalar field.
The complex scalar carries U(1) charge which is associated with the PNA. It is written in terms of the condensation and Green’s function, which is obtained with two-particle irreducible (2PI) closed time path (CTP) effective action (EA). In the spatially flat universe with a time-dependent scale factor, the time evolution of the PNA is computed. We start with an initial condition where only the condensation of the neutral scalar is non-zero. The initial condition for the fields is specified by a density operator parameterized by the temperature of the universe. With the above initial conditions, the PNA vanishes at the initial time and later it is generated through the interaction between the complex scalar and the condensation of the neutral scalar. We investigate the case that both the interaction and the expansion rate of the universe are small and include their effects up to the first order of the perturbation. The expanding universe causes the effects of the dilution of the PNA, freezing interaction and the redshift of the particle energy. As for the time dependence of the PNA, we found that PNA oscillates at the early time and it begins to dump at the later time. The period and the amplitude of the oscillation depend on the mass spectrum of the model, the temperature and the expansion rate of the universe. In addition to the discussion on BAU, we also estimate the numerical value of the PNA over entropy density.

📝 CATATAN:

📌 Kolokium daring ini GRATIS dan TERBUKA untuk umum, terutama mahasiswa, dosen, dan peneliti di bidang terkait judul kolokium.

📌 Mohon maaf penyelenggara tidak menyediakan sertifikat.

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