Bio
I am a theoretical physicist working on Beyond the Standard Model (BSM) particle physics phenomenology. In particular, I am interested in using particle colliders to probe BSM models via their Higgs sector and in unraveling the nature of Dark Matter via model building and experimental probes such as Direct Detection type experiments.
Professional Education
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Bachelor of Science, University of Hamburg (2014)
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Doctor of Philosophy, Stockholm University (2019)
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Master of Science, Uppsala Universitet (2015)
All Publications
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The tiny (g-2) muon wobble from small-mu, supersymmetry
JOURNAL OF HIGH ENERGY PHYSICS
2022
View details for DOI 10.1007/JHEP01(2022)025
View details for Web of Science ID 000740386900004
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Nucleation is more than critical: A case study of the electroweak phase transition in the NMSSM
JOURNAL OF HIGH ENERGY PHYSICS
2021
View details for DOI 10.1007/JHEP03(2021)055
View details for Web of Science ID 000626530400003
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New Projections for Dark Matter Searches with Paleo-Detectors
Instruments
2021; 5
View details for DOI 10.3390/instruments5020021
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Galactic Geology: Probing Time-Varying Dark Matter Signals with Paleo-Detectors
Physical Review D
2021; 104 (12)
View details for DOI 10.1103/PhysRevD.104.123015
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Axion-photon conversion in strongly magnetised plasmas
Journal of Cosmology and Astroparticle Physics
2021; 11
View details for DOI 10.1088/1475-7516/2021/11/013
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Measuring Changes in the Atmospheric Neutrino Rate over Gigayear Timescales.
Physical review letters
2020; 125 (23): 231802
Abstract
Measuring the cosmic ray flux over timescales comparable to the age of the Solar System, ∼4.5 Gyr, could provide a new window on the history of the Earth, the Solar System, and even our Galaxy. We present a technique to indirectly measure the rate of cosmic rays as a function of time using the imprints of atmospheric neutrinos in "paleo-detectors," natural minerals that record damage tracks from nuclear recoils. Minerals commonly found on Earth are ≲1 Gyr old, providing the ability to look back across cosmic ray history on timescales of the same order as the age of the Solar System. Given a collection of differently aged samples dated with reasonable accuracy, this technique is particularly well-suited to measuring historical changes in the cosmic ray flux at Earth and is broadly applicable in astrophysics and geophysics.
View details for DOI 10.1103/PhysRevLett.125.231802
View details for PubMedID 33337188
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Measuring Changes in the Atmospheric Neutrino Rate over Gigayear Timescales
PHYSICAL REVIEW LETTERS
2020; 125 (23)
View details for DOI 10.1103/PhysRevLett.125.231802
View details for Web of Science ID 000594131200001
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Hunting for scalar lepton partners at future electron colliders
PHYSICAL REVIEW D
2020; 102 (1)
View details for DOI 10.1103/PhysRevD.102.015026
View details for Web of Science ID 000553248600003
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Paleodetectors for Galactic supernova neutrinos
PHYSICAL REVIEW D
2020; 101 (10)
View details for DOI 10.1103/PhysRevD.101.103017
View details for Web of Science ID 000532120800001
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Constraints on new scalar and vector mediators from LHC dijet searches
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS
2020; 47 (5)
View details for DOI 10.1088/1361-6471/ab6949
View details for Web of Science ID 000521458300001
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Searching for dark matter with paleo-detectors
PHYSICS LETTERS B
2020; 803
View details for DOI 10.1016/j.physletb.2020.135325
View details for Web of Science ID 000521730300059
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Impact of a XENONnT signal on LHC dijet searches
JOURNAL OF HIGH ENERGY PHYSICS
2019
View details for DOI 10.1007/JHEP07(2019)015
View details for Web of Science ID 000474426000006
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The NMSSM is within reach of the LHC: mass correlations & decay signatures
JOURNAL OF HIGH ENERGY PHYSICS
2019
View details for DOI 10.1007/JHEP04(2019)011
View details for Web of Science ID 000463637400002
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Digging for dark matter: Spectral analysis and discovery potential of paleo-detectors
PHYSICAL REVIEW D
2019; 99 (4)
View details for DOI 10.1103/PhysRevD.99.043541
View details for Web of Science ID 000459913000001
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Paleo-detectors: Searching for dark matter with ancient minerals
PHYSICAL REVIEW D
2019; 99 (4)
View details for DOI 10.1103/PhysRevD.99.043014
View details for Web of Science ID 000459912000002
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Dark Matter implications of DAMA/LIBRA-phase2 results
PHYSICS LETTERS B
2019; 789: 262–69
View details for DOI 10.1016/j.physletb.2018.12.036
View details for Web of Science ID 000457165400036
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Two Higgs doublets and a complex singlet: disentangling the decay topologies and associated phenomenology
JOURNAL OF HIGH ENERGY PHYSICS
2018
View details for DOI 10.1007/JHEP12(2018)044
View details for Web of Science ID 000453294300007
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Higgs portals for thermal Dark Matter. EFT perspectives and the NMSSM
JOURNAL OF HIGH ENERGY PHYSICS
2018
View details for DOI 10.1007/JHEP04(2018)069
View details for Web of Science ID 000430130300001
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Determining dark matter properties with a XENONnT/LZ signal and LHC Run 3 monojet searches
PHYSICAL REVIEW D
2018; 97 (8)
View details for DOI 10.1103/PhysRevD.97.083002
View details for Web of Science ID 000428993600002
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Dilute and dense axion stars
PHYSICS LETTERS B
2018; 777: 64–72
View details for DOI 10.1016/j.physletb.2017.12.010
View details for Web of Science ID 000423930700006
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NMSSM Higgs boson search strategies at the LHC and the mono-Higgs signature in particular
PHYSICAL REVIEW D
2017; 95 (11)
View details for DOI 10.1103/PhysRevD.95.115036
View details for Web of Science ID 000404472700009
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Dark matter capture, subdominant WIMPs, and neutrino observatories
PHYSICAL REVIEW D
2017; 95 (4)
View details for DOI 10.1103/PhysRevD.95.043007
View details for Web of Science ID 000394664300001
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Detecting solar chameleons through radiation pressure
PHYSICS LETTERS B
2014; 739: 167–73
View details for DOI 10.1016/j.physletb.2014.10.055
View details for Web of Science ID 000346002000027