[Okc-wp4] EO meeting Thu Oct 22 @ 13:15 via Zoom

[Andre Schneider]

Hi,



if you would like to watch a recording of this week's EO meeting, it is now available in the link below:


https://drive.google.com/drive/folders/1YaKCwf4M8oEHUOh8o6cX5Ls4t8rX5LGY?usp=sharing


I intend to record and upload the talks to this folder from now on if the speaker has no objections to it.



Best,


---------------------------------

André da Silva Schneider

Department of Astronomy

Stockholm University



________________________________
From: Okc-wp4-at-fysik.su.se <okc-wp4-at-fysik.su.se-bounces at lists.su.se> on behalf of Andre Schneider <andre.schneider at astro.su.se>
Sent: Thursday, October 22, 2020 3:22:24 AM
To: Okc-wp4 at fysik.su.se; people at nordita.org
Subject: Re: [Okc-wp4] EO meeting Thu Oct 22 @ 13:15 via Zoom




Reminder of the EO meeting today at 13:15.

https://stockholmuniversity.zoom.us/j/61161537684



---------------------------------

André da Silva Schneider

Department of Astronomy

Stockholm University



________________________________
From: Okc-wp4-at-fysik.su.se <okc-wp4-at-fysik.su.se-bounces at lists.su.se> on behalf of Andre Schneider <andre.schneider at astro.su.se>
Sent: Monday, October 19, 2020 10:52:52 PM
To: Okc-wp4 at fysik.su.se; people at nordita.org
Subject: [Okc-wp4] EO meeting Thu Oct 22 @ 13:15 via Zoom




Dear colleagues,


our next EO meeting will take place this Thursday Oct 22 at 13:15 via Zoom.
The meeting will be online. To join access https://stockholmuniversity.zoom.us/j/61161537684
You will be able to enter the meeting room from 13:00. See below for other methods to participate.


This week Lorenzo Nativi from Stockholm Univrsity will present



Title:  Can jets make radioactively-powered emission from neutron star mergers bluer?

Abstract:

Besides being sources of gravitational waves, neutron star mergers eject neutron-rich material suitable for the production of heavy r-process nuclei. The radioactive decay of these freshly synthesised elements powers a rapidly evolving thermal transient (named "macronova" or "kilonova"), whose spectral properties strongly depend on the ejecta composition. In particular, the high opacities associated to the heaviest nuclei powers a transient peaking in the red-infrared bands over time scales of weeks.
The first detection of a binary neutron star merger was also accompanied by the detection of a relativistic jet. Despite being ascertained the presence of two dynamical components, mildly-relativistic ejecta and ultra-relativistic outflow, the observational consequences of the interplay between the two is still unclear.
In this talk I will discuss the consequences of jet propagation on the radioactively powered transient, by simulating the interaction with dedicated special-relativistic hydrodynamics simulations. Firstly, I will present the observational evidence of the two dynamical components. Second, I will discuss the simulations setup focusing on the initial ejecta distribution as obtained from previous dedicated works. Lastly, I will show how a relativistic jet can "punch-away" a fraction of high-opacity material before the brightening of the macronova, resulting in the transient getting brighter and bluer for on-axis observers in the first few days.






Andre da Silva Schneider is inviting you to a scheduled Zoom meeting.

Topic: EO Meeting
Time: Oct 22, 2020 01:00 PM Stockholm

Join Zoom Meeting
https://stockholmuniversity.zoom.us/j/61161537684

Meeting ID: 611 6153 7684
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---------------------------------

André da Silva Schneider

Department of Astronomy

Stockholm University


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