Particle Physics and Gravitational Waves as complementary windows on the Universe
Fuente:
arXiv
Gespeichert in:
| Hauptverfasser: | , , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Veröffentlicht: |
2026
|
| Schlagworte: | |
| Online-Zugang: | |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| _version_ | 1866910075850850304 |
|---|---|
| author | Bass, Steven D. Baudis, Laura Bertone, Gianfranco Buchmueller, Oliver Döbrich, Babette Genzel, Reinhard Green, Anne M. Helbing, Klaus Heurs, Michèle Jakobs, Karl Klute, Markus Nissanke, Samaya Peiris, Hiranya Perego, Albino Pokorski, Stefan Schott, Matthias Vitale, Stefano Weiglein, Georg Weller, Jochen |
| author_facet | Bass, Steven D. Baudis, Laura Bertone, Gianfranco Buchmueller, Oliver Döbrich, Babette Genzel, Reinhard Green, Anne M. Helbing, Klaus Heurs, Michèle Jakobs, Karl Klute, Markus Nissanke, Samaya Peiris, Hiranya Perego, Albino Pokorski, Stefan Schott, Matthias Vitale, Stefano Weiglein, Georg Weller, Jochen |
| contents | Particle physics and gravitational waves provide complementary probes of the deep structure of the Universe. Gravitational waves from the mergers of neutron stars and black holes are sensitive to the structure of dense quark matter and to different dark matter scenarios. Measurements of stochastic gravitational waves backgrounds can teach us about possible first order phase transitions in the early Universe, including providing sensitivity to the TeV scale which is of key interest to future particle collider experiments. Gravitational waves measurements will also give new probes of the evolution and expansion of the Universe, complementary to measurements with electromagnetic radiation. This Perspectives article explores the physics synergies between the science opportunities provided by next generation gravitational waves measurements and particle physics experiments. Gravitational waves can also probe deep into the early Universe reaching physics much above possible collider energies if the signals can be detected. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2603_25578 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Particle Physics and Gravitational Waves as complementary windows on the Universe Bass, Steven D. Baudis, Laura Bertone, Gianfranco Buchmueller, Oliver Döbrich, Babette Genzel, Reinhard Green, Anne M. Helbing, Klaus Heurs, Michèle Jakobs, Karl Klute, Markus Nissanke, Samaya Peiris, Hiranya Perego, Albino Pokorski, Stefan Schott, Matthias Vitale, Stefano Weiglein, Georg Weller, Jochen Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Experiment High Energy Physics - Phenomenology Nuclear Theory Particle physics and gravitational waves provide complementary probes of the deep structure of the Universe. Gravitational waves from the mergers of neutron stars and black holes are sensitive to the structure of dense quark matter and to different dark matter scenarios. Measurements of stochastic gravitational waves backgrounds can teach us about possible first order phase transitions in the early Universe, including providing sensitivity to the TeV scale which is of key interest to future particle collider experiments. Gravitational waves measurements will also give new probes of the evolution and expansion of the Universe, complementary to measurements with electromagnetic radiation. This Perspectives article explores the physics synergies between the science opportunities provided by next generation gravitational waves measurements and particle physics experiments. Gravitational waves can also probe deep into the early Universe reaching physics much above possible collider energies if the signals can be detected. |
| title | Particle Physics and Gravitational Waves as complementary windows on the Universe |
| topic | Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Experiment High Energy Physics - Phenomenology Nuclear Theory |
| url | https://arxiv.org/abs/2603.25578 |