BEGIN:VCALENDAR
METHOD:PUBLISH
PRODID:www-physik-nat-fau-de//Events//DE
VERSION:2.0
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: N.N.
UID:040000008200E00074C5B7101A82E00800000000905FF02621BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: t.b.a. Abstract: t.b.a. Sprecher / Speaker: t.b.a. 
 Kontakt / Contact: t.b.a.
DTSTART:20260617T100000Z
DTEND:20260617T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: Prof. Dr. Martin B. Plenio - t.b.a.
UID:040000008200E00074C5B7101A82E00800000000E078AD2821BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: t.b.a. Abstract: t.b.a. Sprecher / Speaker: Prof. D
 r. Martin B. Plenio\, Universität Ulm Kontakt / Contact: Prof. Dr. Da
 niel Burgarth
DTSTART:20260701T100000Z
DTEND:20260701T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: N.N.
UID:040000008200E00074C5B7101A82E00800000000D0B1972921BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: t.b.a. Abstract: t.b.a. Sprecher / Speaker: t.b.a. 
 Kontakt / Contact: t.b.a.
DTSTART:20260708T100000Z
DTEND:20260708T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: Dr. Phillipp Eller - Towards a Unif
 ied Picture of Atmospheric Neutrino Oscillations
UID:040000008200E00074C5B7101A82E00800000000904ED82721BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: Towards a Unified Picture of Atmospheric Neutrino O
 scillations Abstract: Atmospheric neutrinos provide a unique probe of 
 neutrino oscillations over a wide range of energies and baselines\, tr
 aversing the Earth through regions of varying matter density. Over the
  past decades\, experiments such as Super‑Kamiokande and IceCube&#82
 11\;and more recently KM3NeT/ORCA&#8211\;have collected large atmosphe
 ric neutrino data sets\, each offering complementary strengths in ener
 gy coverage\, angular resolution\, and control of systematic uncertain
 ties. In this talk\, I will present a combined analysis of atmospheric
  neutrino data from these experiments\, aiming to exploit their comple
 mentarity within a common oscillation framework. By bringing together 
 measurements from water‑ and ice‑Cherenkov detectors with differen
 t energy thresholds and detector configurations\, this approach provid
 es a more global and robust view of atmospheric neutrino oscillations\
 , reducing sensitivity to detector‑specific effects. Beyond the phys
 ics results\, this analysis also follows a new avenue by being fully o
 pen‑source from the outset\, enabling transparent\, community‑driv
 en development and establishing a flexible foundation for future neutr
 ino oscillation studies and global fits. Sprecher / Speaker: Dr. Phill
 ipp Eller\, TU München Kontakt / Contact: Prof. Dr. Claudio Kopper
DTSTART:20260624T100000Z
DTEND:20260624T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: Prof. Dr. Gerd Schröder-Turk - Dev
 elopment of optical Gyroid nanostructures in green butterflies
UID:040000008200E00074C5B7101A82E00800000000303D812C21BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: Development of optical Gyroid nanostructures in gre
 en butterflies Abstract: Several green butterflies generate their gree
 n coloration as a photonic crystal effect using a 3D nanostructure kno
 wn as the Gyroid. The structure of the mature butterfly nanostructures
  is easy to image by electron and X-ray microscopy and well characteri
 sed\, and its photonic properties are well understood. However\, the m
 echanisms by which the butterfly forms these nanostructures\, and part
 icularly how it stabilises a highly ordered geometry at the large leng
 th scale of 100s of nanometers\, is not fully understood. In this talk
 \, I will discuss our optical microscopy observations on living butter
 fly pupae that are suitably dissected to reveal the area of interest. 
 Like any conventional microscopy\, our optical data cannot resolve the
  nanostructure\; it is below the diffraction limit. However\, we can r
 esolve the reflectances that the nanostructure causes. Together with e
 lectron microscopy analyses of tissue samples\, these reflectances can
  be used to at least provide information of the timing of nanostructur
 e development. When we carried out these analyses\, we made the surpri
 sing finding that\, at the early stages of development\, the nanostruc
 ture is composed of fibrils woven together to form the 3D nanostructur
 e\; how it transitions to the smooth nanostructural form observed in m
 ature butterflies is not currently known. Sprecher / Speaker: Prof. Dr
 . Gerd Schröder-Turk Kontakt / Contact: Prof. Dr. Ben Fabry
DTSTART:20260715T100000Z
DTEND:20260715T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: N.N.
UID:040000008200E00074C5B7101A82E00800000000709FB7F420BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: t.b.a. Abstract: t.b.a. Sprecher / Speaker: t.b.a. 
 Kontakt / Contact: t.b.a.
DTSTART:20260422T100000Z
DTEND:20260422T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: N.N.
UID:040000008200E00074C5B7101A82E00800000000B02A211F21BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: t.b.a. Abstract: t.b.a. Sprecher / Speaker: t.b.a. 
 Kontakt / Contact: t.b.a.
DTSTART:20260429T100000Z
DTEND:20260429T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: Prof. Dr. Robert König - Quantum f
 ault-tolerance with noisy circuits and entanglement generation
UID:040000008200E00074C5B7101A82E00800000000608D672021BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: Quantum fault-tolerance with noisy circuits and ent
 anglement generation Abstract: A fundamental question in quantum infor
 mation science is: what can noisy quantum circuits actually do? Unders
 tanding the computational and communication power of realistic\, imper
 fect quantum hardware is essential for both near-term applications and
  the long-term development of quantum technologies. A paradigmatic pro
 blem in this context is long-range entanglement generation\, i.e.\, cr
 eating high-quality entangled states between distant qubits using only
  noisy local operations. This task is central to quantum networking an
 d distributed quantum computing\, where shared entanglement across lar
 ge distances serves as the key resource. We study this problem on a re
 ctangular grid of qubits in 2D\, subject to local stochastic Pauli noi
 se. This is a setup that\, depending on the length scale\, describes b
 oth a single quantum device with geometrically limited connectivity an
 d a planar network of constant-sized quantum stations. We give a proto
 col that\, for noise below a constant threshold\, generates a constant
 -fidelity Bell pair between qubits separated by an arbitrarily large d
 istance R. The required grid dimensions scale as Θ(R) × Θ(poly(log 
 R))\, and the protocol runs in constant time (single-shot)\, producing
  a Bell state up to a known Pauli correction. This contrasts with exis
 ting approaches\, which either require local devices whose size grows 
 with the target distance\, or need a distance-dependent number of roun
 ds. Our work provides the first example of a short-range entangled sta
 te in 2D from which long-range Bell pairs can be reliably extracted de
 spite noise\, as well as a 2D-local stabilizer Hamiltonian whose therm
 al states retain this property at constant positive temperature. The t
 alk is based on joint work with Dylan Harley\, arXiv:2604.05870. Sprec
 her / Speaker: Prof. Dr. Robert König\, TU München Kontakt / Contact
 : Prof. Dr. Daniel Burgarth
DTSTART:20260506T100000Z
DTEND:20260506T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: N.N.
UID:040000008200E00074C5B7101A82E0080000000020D9642121BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: t.b.a. Abstract: t.b.a. Sprecher / Speaker: t.b.a. 
 Kontakt / Contact: t.b.a.
DTSTART:20260513T100000Z
DTEND:20260513T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: Prof. Dr. Denis Golez - Optical Det
 ection and Control of Exciton Condensates
UID:040000008200E00074C5B7101A82E0080000000060E3232221BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: Optical Detection and Control of Exciton Condensate
 s Abstract: t.b.a. Sprecher / Speaker: Prof. Dr. Denis Golez\, Jozef S
 tefan Institute\, University of Ljubljana Kontakt / Contact: Prof. Dr.
  Daniele Fausti
DTSTART:20260520T100000Z
DTEND:20260520T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: N.N.
UID:040000008200E00074C5B7101A82E0080000000010E8D22221BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: t.b.a. Abstract: t.b.a. Sprecher / Speaker: t.b.a. 
 Kontakt / Contact: t.b.a.
DTSTART:20260527T100000Z
DTEND:20260527T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: Dr. Paul Bennet - Proper Motions in
  and beyond the Local Group of Galaxies
UID:040000008200E00074C5B7101A82E00800000000A0F3DB2321BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: Proper Motions in and beyond the Local Group of Gal
 axies Abstract: Proper motions are the on sky motions of astronomical 
 objects. Unlike line of sight velocities\, that can be readily obtaine
 d from spectroscopy\, proper motions are very difficult to determine f
 or most objects requiring extremely precise measurements of position i
 n the sky separated by many years. This means\, for most objects\, the
 y are the final components of position velocity information to be obta
 ined. With full 6D position-velocity information we can tell not only 
 the present of an object but use its trajectory to understand its past
  and future. This allows us to examine many problems in astrophysics a
 nd physics more broadly\, such as when and where do galaxies stop form
 ing new stars and what is the dark matter content of the Milky Way? It
  also gives insight in the nature of dark matter models including if d
 ark matter is self-interacting or a purely non-interactive particle. S
 precher / Speaker: Dr. Paul Bennet\, Space Telescope Science Institute
 \, Baltimore Kontakt / Contact: Prof. Dr. Jörn Wilms
DTSTART:20260603T100000Z
DTEND:20260603T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physikalisches Kolloquium: N.N.
UID:040000008200E00074C5B7101A82E00800000000807F052521BDDC010000000000
 00000010000000BEB060FEC9762C43927071AB32719CD2
DESCRIPTION:Titel: t.b.a. Abstract: t.b.a. Sprecher / Speaker: t.b.a. 
 Kontakt / Contact: t.b.a.
DTSTART:20260610T100000Z
DTEND:20260610T110000Z
LOCATION:Hörsaal D\, Staudtstr. 5\, 91058 Erlangen
DTSTAMP:20260516T074412Z
END:VEVENT
END:VCALENDAR