[Astro] [CAPT] Journal club talk by summer intern Louis Herwig (11 am Thursday)

[Lauren Gaughan]

Hi all,

This is a gentle reminder of the talk by Louis in ~1.5 hours.

There will also be doughnuts.

Thanks,
Lauren
________________________________
From: Particles <particles-bounces at lists.nottingham.ac.uk> on behalf of Swagat Mishra <Swagat.Mishra at nottingham.ac.uk>
Sent: 11 September 2024 12:29
To: capt at nottingham.ac.uk <capt at nottingham.ac.uk>; maths-quantum-gravity-group at lists.nottingham.ac.uk <maths-quantum-gravity-group at lists.nottingham.ac.uk>; O365-Gravity Laboratory <o365-gravitylaboratory at UniofNottm.onmicrosoft.com>
Cc: Louis Herwig <herwig.louis at gmail.com>
Subject: Re: [Particles] [CAPT] Journal club talk by summer intern Louis Herwig (11 am Thursday)

Dear All,

This is to inform that the talk by Louis Herwig will be held at 11 am on Thursday, instead of 3 pm. The details are given below.  (Sorry for the short notice.)

With Regards,
-Swagat

    We have Louis Herwig, a master's student from MPI (Physics) in Munich, who is visiting Clare Burrage for an internship this summer. Louis will be giving a talk on coming Thursday (journal club time, but Particle Cosmology Seminar Link, see below).

Venue: A 113
Date: 12th  September 2024
Time: 11 am UK time

Title: Dark matter constraints from quadratic interactions

Abstract: Conventional haloscopes are limited by a narrow frequency range, whereas ferromagnetic haloscopes address this limitation by introducing a tunable resonant frequency, offering the potential for broadband axion detection. Haloscopes exploit the axion-photon coupling, whereas ferromagnetic haloscopes exploit the axion-electron (electron spin resonance) coupling. The induced effective magnetic field from axions depends on their mass and coupling. Current models have mostly only considered linear axion interactions. This work investigates quadratic axion interactions, which could measurably change the effective magnetic field leading to a different output power.
Link to join online:

https://teams.microsoft.com/l/meetup-join/19%3ameeting_OGM3OTk5NzQtZWEwZS00ZmUyLTk3MGUtZjFhY2M5OTU2MjI1%40thread.v2/0?context=%7b%22Tid%22%3a%2267bda7ee-fd80-41ef-ac91-358418290a1e%22%2c%22Oid%22%3a%22f3250584-4b5f-48fa-a897-08e77f2246b7%22%7d

With Regards,
-Swagat


Swagat Saurav Mishra,

Postdoctoral Research Associate

​

Particle Cosmology Group,

Centre for Astronomy and Particle Theory,

University of Nottingham, Nottingham NG7 2RD, UK.

Website: https://swagatam18.wordpress.com/

Research Link:https://inspirehep.net/authors/1517353

________________________________
From: Swagat Mishra (staff) <ppzsm5 at exmail.nottingham.ac.uk>
Sent: 07 September 2024 16:47
To: capt at nottingham.ac.uk <capt at nottingham.ac.uk>; maths-quantum-gravity-group at lists.nottingham.ac.uk <maths-quantum-gravity-group at lists.nottingham.ac.uk>; O365-Gravity Laboratory <o365-gravitylaboratory at UniofNottm.onmicrosoft.com>
Cc: Louis Herwig <ppxlh3 at exmail.nottingham.ac.uk>
Subject: Journal club talk by summer intern Louis Herwig

Dear All,

    We have Louis Herwig, a master's student from MPI (Physics) in Munich, who is visiting Clare Burrage for an internship this summer. Louis will be giving a talk on coming Thursday (journal club time, but Particle Cosmology Seminar Link, see below).

Venue: A 113
Date: 12th  September 2024
Time: 3 pm UK time

Title: Dark matter constraints from quadratic interactions

Abstract: Conventional haloscopes are limited by a narrow frequency range, whereas ferromagnetic haloscopes address this limitation by introducing a tunable resonant frequency, offering the potential for broadband axion detection. Haloscopes exploit the axion-photon coupling, whereas ferromagnetic haloscopes exploit the axion-electron (electron spin resonance) coupling. The induced effective magnetic field from axions depends on their mass and coupling. Current models have mostly only considered linear axion interactions. This work investigates quadratic axion interactions, which could measurably change the effective magnetic field leading to a different output power.
Link to join online:

https://teams.microsoft.com/l/meetup-join/19%3ameeting_OGM3OTk5NzQtZWEwZS00ZmUyLTk3MGUtZjFhY2M5OTU2MjI1%40thread.v2/0?context=%7b%22Tid%22%3a%2267bda7ee-fd80-41ef-ac91-358418290a1e%22%2c%22Oid%22%3a%22f3250584-4b5f-48fa-a897-08e77f2246b7%22%7d

With Regards,
-Swagat


Swagat Saurav Mishra,

Postdoctoral Research Associate

​

Particle Cosmology Group,

Centre for Astronomy and Particle Theory,

University of Nottingham, Nottingham NG7 2RD, UK.

Website: https://swagatam18.wordpress.com/

Research Link:https://inspirehep.net/authors/1517353

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