Cookies

We use cookies to ensure that we give you the best experience on our website. You can change your cookie settings at any time. Otherwise, we'll assume you're OK to continue.

Research

Research lectures, seminars and events

The events listed in this area are research seminars, workshops and lectures hosted by Durham University departments and research institutes. If you are not a member of the University, but  wish to enquire about attending one of the events please contact the organiser or host department.


 

October 2018
SunMonTueWedThuFriSat
September 2018 November 2018
1 2 3 4 5 6
7 8 9 10 11 12 13
14 15 16 17 18 19 20
21 22 23 24 25 26 27
28 29 30 31

Events for 19 October 2018

Ömer Gürdoğan: Cluster Adjacency and the NMHV 7-particle amplitude in N=4 super Yang-Mills at 4 loops

1:00pm, CM101

The idea of constructing scattering amplitudes from their
singularities has been a very powerful method for their computation. We
introduce the principle of Cluster Adjacency, which governs the analytic
structure of amplitudes at tree and loop level. We use this to compute the
NMHV scattering amplitude of seven particles in N=4 super Yang-Mills at
four loops.

Contact christiana.pantelidou@durham.ac.uk, mathew.r.bullimore@durham.ac.uk for more information about this event.


Roger Scott: Magnetic Structures at the Boundary of the Closed Corona

3:00pm, CM301

The topology of coronal magnetic fields near the open-closed magnetic flux boundary is important to the the process of interchange reconnection, whereby plasma is exchanged between open and closed flux domains. Maps of the magnetic squashing factor in coronal field models reveal the presence of the Separatrix-Web (S-Web), a network of separatrix surfaces and quasi-separatrix layers, along which interchange reconnection is highly likely. Under certain configurations, interchange reconnection within the S-Web could potentially release coronal material from the closed magnetic field regions to high-latitude regions far from the heliospheric current sheet where it is observed as slow solar wind. It has also been suggested that transport along the S-Web may be a possible cause for the observed large longitudinal spreads of some impulsive, 3He-rich solar energetic particle events. Here we demonstrate that certain features of the S-Web reveal structural aspects of the underlying magnetic field, specifically regarding the arcing bands of highly squashed magnetic flux observed at the outer boundary of global magnetic field models. In order for these S-Web arcs to terminate or intersect away from the helmet streamer apex, there must be a null spine line that maps a finite segment of the photospheric open-closed boundary up to a singular point in the open flux domain. We propose that this association between null spine lines and arc termination points may be used to identify locations in the heliosphere that are preferential for the appearance of solar energetic particles and plasma from the closed corona, with characteristics that may inform our understanding of interchange reconnection and the acceleration of the slow solar wind.

Contact christopher.prior@durham.ac.uk for more information about this event.