00:24:35	Sekazi Mtingwa:	Latest measurement of proton radius: https://www.nature.com/articles/d41586-019-03432-4
00:25:55	Wlodek Guryn:	Thanks for the reference.
00:40:25	brynna Moran:	What does it physically mean for those forces to be P and T symmetrical?
00:40:25	Letrell Harris:	Can you explain more in depth about what “we wouldn’t be here means.”?
00:42:33	brynna Moran:	That was a very helpful and clear explanation, thank you very much!
00:44:41	Mary Bishai:	Emi Noether was a very famous mathematician. One of her greatest contribution to physics was the concept that symmetries in nature lead to conservation laws: https://en.wikipedia.org/wiki/Noether%27s_theorem
00:44:43	Letrell Harris:	Thank you, that was very helpful
00:45:44	Mary Bishai:	And don't thrust the Wikipedia entry - I just had that at hand ;)
00:49:02	Ambar Rodriguez:	How does the weak force break the symmetries?
00:49:45	Wlodek Guryn:	We’ll ask in  moment.
00:50:56	Ambar Rodriguez:	The interactions would require different particles when changing symmetries then?
00:52:23	Ambar Rodriguez:	Ok ok, now I think it is more clear, thank you!
00:53:59	Mary Bishai:	On the history of the discovery of CP symmetry (or time symmetry) violation in weak decays of quarks: https://cerncourier.com/a/cp-violations-early-days/
00:54:12	Mary Bishai:	This was a Nobel prize winning experiment at BNL.
00:56:50	Wlodek Guryn:	Thank you Mary!
01:03:05	Letrell Harris:	What do you mean by “anomalous”?
01:03:52	Wlodek Guryn:	We’ll ask in a moment
01:07:17	Letrell Harris:	Thank you
01:15:06	Sekazi Mtingwa:	Fabulous lecture!!!  Thanks, Bill.
01:15:12	Karan Kumar:	Why mean of theoretical value of g of Davier et al. (10) is quite different from other theoretical predictions?
01:19:39	Sekazi Mtingwa:	Will the slides be available for the students?
01:20:42	Wlodek Guryn:	Yes, both slides and recording shall be made available.
01:21:08	Wlodek Guryn:	You need to go to the webpage of the Summer Lectures
01:38:00	David Zimmerman:	Bill - thank you for the lectgure.  It was great.