The University of Southampton

- Event

Date:
24th of February, 2023  @  13:00 - 14:15
Venue:
46/5081 and on Teams

Event details

We consider the effective theory of perturbative quantum gravity coupled to a point particle, quantizing fluctuations of both the gravitational field and the particle's position around flat space. Using a recent relational approach to construct gauge-invariant observables, we compute one-loop graviton corrections to the invariant metric perturbation, whose time-time component gives the Newtonian gravitational potential. The resulting quantum correction consists of two parts: the first stems from graviton loops and agrees with the correction derived by other methods, while the second one is sourced by the quantum fluctuations of the particle's position and energy-momentum, and may be viewed as an analog of a ``Zitterbewegung''. As a check on the computation, we also recover classical corrections which agree with the perturbative expansion of the Schwarzschild metric. Based on joint work with C. Rein and R. Verch, arXiv:2109.09753 [JHEP 01 (2022) 180].
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- Event

Date:
17th of February, 2023  @  13:00 - 14:15
Venue:
Microsoft Teams

Event details

Lepton asymmetries present in the early universe can source helical hypermagnetic fields through the chiral plasma instability. If these hypermagnetic fields survive until the electroweak phase transition, they source a contribution to the baryon asymmetry of the universe. In this talk I will explain how this phenomenon can, one the one hand, be used to set the to date strongest bounds on primordial lepton flavour asymmetries and on the other hand, can play a key role in viable baryogenesis models.

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- Event

Date:
3rd of February, 2023  @  15:00 - 16:15
Venue:
Microsoft Teams

Event details

Whether neutrinos are Majorana or Dirac particles is an open question. Theoretically, it is also possible that neutrinos are pseudo-Dirac, which are fundamentally Majorana fermions, but essentially act like Dirac fermions in most experimental settings due to extremely small active-sterile mass splitting. However, they can be differentiated through active-sterile oscillations with an astrophysical baseline. In this talk, we will show that the recent identification of ultra-high energy neutrino sources by the IceCube Neutrino Observatory provides us with such an astrophysical baseline, thus improving the reach of terrestrial experiments by more than a billion for the mass-squared difference.

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- Event

Date:
27th of January, 2023  @  13:00 - 14:15
Venue:
46/5081 and on Teams

Event details

​We study an infinite family of Massive Type IIA backgrounds that holographically describe the twisted compactification of N=(1,0) six-dimensional SCFTs to four dimensions. The analysis of the branes involved suggests a four dimensional linear quiver QFT, that deconstructs the theory in six dimensions. For the case in which the system reaches a strongly coupled fixed point, we calculate some observables that we compare with holographic results. Two quantities measuring the number of degrees of freedom for the flow across dimensions are studied.

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- Event

Date:
18th of May, 2023  @  13:00 - 14:00
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- Event

Date:
9th of February, 2023  @  13:00 - 14:00
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- Event

Date:
26th of January, 2023  @  13:00 - 14:00
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- Event

Date:
10th of February, 2023  @  13:00 - 14:15
Venue:
46/5081 and on Teams

Event details

​𝑉_{𝑢𝑏} is the smallest and least known of all CKM matrix elements; it's currently determined primarily through the exclusive process B \to \pi \ell \bar{
u}. I will present progress toward a lattice QCD determination of the 𝑉_{𝑢𝑏}​ matrix element from a novel transition -- the B \to \pi \pi \ell \bar{
u} process, where the π π system is in a P-wave and features the \rho(770) resonance as an enhancement. The calculation is performed an ensemble with 𝑁_𝑓=2+1 isotropic clover fermions wiht 𝐿≈3.6 fm and a pion mass of 320 MeV; for the b-quark we use the anisotropic clover action. After a brief overview of the theoretical framework, I will discuss some preliminary results.

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